# Difference between revisions of "G2p Analysis Minutes"

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==10/15/2014== | ==10/15/2014== | ||

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Present: Chao, Jie, Pengjia, Min, Melissa <br> | Present: Chao, Jie, Pengjia, Min, Melissa <br> | ||

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*Jie | *Jie | ||

**Gave more details on his update to the energy loss model. Previously, he showed a comparison of data with simulation, including <br>only the energy loss due to ionization in the simulation, and found that the simulation result was wider than the data. The ionization <br>model used in SAMC is a Landau distribution with the most probable value at 0 and a FWHM at 4ε. He updated the model to have <br> a most probably value of -0.22278 and a FWHM of ε. He compared both landau distributions to a fluctuation model, and found that <br>the updated Landau model (with FWHM=ε) matched much better than the previous model (with FWHM=4ε). He also showed a<br> comparison of data from a carbon run without helium with simulation results including the complete energy loss model (ionization,<br> internal and external Bremsstrahlung), which match reasonably well. Next he will work on comparing data with simulation for other <br>target types. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_10_08_simulation/Simulation_update_2014_10_08.pdf here]. | **Gave more details on his update to the energy loss model. Previously, he showed a comparison of data with simulation, including <br>only the energy loss due to ionization in the simulation, and found that the simulation result was wider than the data. The ionization <br>model used in SAMC is a Landau distribution with the most probable value at 0 and a FWHM at 4ε. He updated the model to have <br> a most probably value of -0.22278 and a FWHM of ε. He compared both landau distributions to a fluctuation model, and found that <br>the updated Landau model (with FWHM=ε) matched much better than the previous model (with FWHM=4ε). He also showed a<br> comparison of data from a carbon run without helium with simulation results including the complete energy loss model (ionization,<br> internal and external Bremsstrahlung), which match reasonably well. Next he will work on comparing data with simulation for other <br>target types. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_10_08_simulation/Simulation_update_2014_10_08.pdf here]. | ||

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==10/8/2014== | ==10/8/2014== | ||

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Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Melissa <br> | Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Melissa <br> | ||

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*Jie | *Jie | ||

**Gave a quick update on the energy loss model for g2psim. The main update is that the Landau distribution used for the ionization model should <br>be Landau(x,ε) instead of Landau(x,4ε). He will give more details next week. His slides can be seen [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_10_08_simulation/Simulation_update_2014_10_08.pdf here]. | **Gave a quick update on the energy loss model for g2psim. The main update is that the Landau distribution used for the ionization model should <br>be Landau(x,ε) instead of Landau(x,4ε). He will give more details next week. His slides can be seen [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_10_08_simulation/Simulation_update_2014_10_08.pdf here]. | ||

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'''General Discussion:''' | '''General Discussion:''' | ||

*A room has been booked for the collaboration meeting on November 14th. Kalyan will set up a formal registration for the meeting. | *A room has been booked for the collaboration meeting on November 14th. Kalyan will set up a formal registration for the meeting. | ||

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==10/1/2014== | ==10/1/2014== | ||

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Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa <br> | Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa <br> | ||

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*Based on the results of the poll, November 14th is the best day for a collaboration meeting. Each student will give a summary of analysis <br> | *Based on the results of the poll, November 14th is the best day for a collaboration meeting. Each student will give a summary of analysis <br> | ||

progress (~30 minutes) and there will be time for discussion of thesis topics. | progress (~30 minutes) and there will be time for discussion of thesis topics. | ||

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==9/24/2014== | ==9/24/2014== | ||

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Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa <br> | Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa <br> | ||

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*Pengjia will be at JLab for 3 months. We should have another discussion soon about analysis tasks for students as some projects start to finish up. | *Pengjia will be at JLab for 3 months. We should have another discussion soon about analysis tasks for students as some projects start to finish up. | ||

*Will we try to have a collaboration meeting in mid November. Kalyan has set up a Doodle Poll to select a date - please respond! | *Will we try to have a collaboration meeting in mid November. Kalyan has set up a Doodle Poll to select a date - please respond! | ||

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==9/17/2014== | ==9/17/2014== | ||

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Present: JP, Kalyan, Min, Jie, Chao, Jixie, Melissa <br> | Present: JP, Kalyan, Min, Jie, Chao, Jixie, Melissa <br> | ||

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*Chao | *Chao | ||

**Gave an optics status update, specifically a revision of the y-target calibration. Using the beam position scan isn't ideal; since we only took data at <br>dp=0%, the calibration will only work for a small dp range. Jixie results (using geant4) suggest that the upstream window of the target chamber has <br>some acceptance by the Q1 entrance. Since they have seen something upstream in the optics data, he will try to use this data to do the y-target <br>calibration. This result will be more reliable, as it will take all dp settings into account. He identified the data from the window, and used a vertex cut <br>to select them. In each setting, one hole was selected to do the calibration. The calibration result was compared to the known location of the sieve <br>hole. There was good agreement, which suggests the method is working. He is currently on figuring out how to check that the data is actually <br>coming from the upstream window. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/chao/20140917/Chao_WeeklyMeeting_09172014.pdf here]. | **Gave an optics status update, specifically a revision of the y-target calibration. Using the beam position scan isn't ideal; since we only took data at <br>dp=0%, the calibration will only work for a small dp range. Jixie results (using geant4) suggest that the upstream window of the target chamber has <br>some acceptance by the Q1 entrance. Since they have seen something upstream in the optics data, he will try to use this data to do the y-target <br>calibration. This result will be more reliable, as it will take all dp settings into account. He identified the data from the window, and used a vertex cut <br>to select them. In each setting, one hole was selected to do the calibration. The calibration result was compared to the known location of the sieve <br>hole. There was good agreement, which suggests the method is working. He is currently on figuring out how to check that the data is actually <br>coming from the upstream window. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/chao/20140917/Chao_WeeklyMeeting_09172014.pdf here]. | ||

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==9/10/2014== | ==9/10/2014== | ||

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Present: Chao, JP, Jie, Jixie, Kalyan, Melissa <br> | Present: Chao, JP, Jie, Jixie, Kalyan, Melissa <br> | ||

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*Ryan | *Ryan | ||

**Gave an update on using SAMC to compare the Bosted model to SAGDH nitrogen cross sections. SAMC can include both energy loss and inelastic <br>radiative corrections, which makes it the best comparison to the SAGDH cross sections. However, the radiative corrections take a long time to run, <br>so it may not be worthwhile. To test the results of SAMC, he threw 10M events for each momentum setting, but did not turn on energy loss. He <br>compared this to his previous method of averaging the Bosted model result over the scattering angle. The ratio of the two methods is close to 1, <br>suggesting that both methods give similar results. He also did the same comparison, but first radiating SAMC/angle averaged Bosted model, (see <br>slide for equations). There was some discussion on whether this is the proper method to apply these corrections, but it seems that Ryan's method is <br>consistent with what was done previously. Of the two methods, Ryan concluded that the SAMC method isn't any better than his previous method, so <br>it is not worth the extra time it takes to run. JP suggested checking how much the scattering angle varies over the length of the target; if it is linear, <br>than using the average is a good approximation, but this may not be the case. Since there is no SAGDH carbon data that matches our kinematics (that <br>has been analyzed), we won't be able to do a comparison of nitrogen/carbon. Ryan plans to nail down the Bosted model so that it can be used instead; <br>he will scale the Bosted model to match SAGDH nitrogen data, do the same with the SAGDH carbon data, then use the ratio of these to translate the <br>results to our data. More details can be seen in his slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_091014.pdf here]. | **Gave an update on using SAMC to compare the Bosted model to SAGDH nitrogen cross sections. SAMC can include both energy loss and inelastic <br>radiative corrections, which makes it the best comparison to the SAGDH cross sections. However, the radiative corrections take a long time to run, <br>so it may not be worthwhile. To test the results of SAMC, he threw 10M events for each momentum setting, but did not turn on energy loss. He <br>compared this to his previous method of averaging the Bosted model result over the scattering angle. The ratio of the two methods is close to 1, <br>suggesting that both methods give similar results. He also did the same comparison, but first radiating SAMC/angle averaged Bosted model, (see <br>slide for equations). There was some discussion on whether this is the proper method to apply these corrections, but it seems that Ryan's method is <br>consistent with what was done previously. Of the two methods, Ryan concluded that the SAMC method isn't any better than his previous method, so <br>it is not worth the extra time it takes to run. JP suggested checking how much the scattering angle varies over the length of the target; if it is linear, <br>than using the average is a good approximation, but this may not be the case. Since there is no SAGDH carbon data that matches our kinematics (that <br>has been analyzed), we won't be able to do a comparison of nitrogen/carbon. Ryan plans to nail down the Bosted model so that it can be used instead; <br>he will scale the Bosted model to match SAGDH nitrogen data, do the same with the SAGDH carbon data, then use the ratio of these to translate the <br>results to our data. More details can be seen in his slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_091014.pdf here]. | ||

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==9/3/2014== | ==9/3/2014== | ||

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Present: Chao, Kalyan, Jie, Min, JP, Jixie, Melissa <br> | Present: Chao, Kalyan, Jie, Min, JP, Jixie, Melissa <br> | ||

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*Jie | *Jie | ||

**Gave an update on the energy loss model. Last time he showed a comparison of the ionization models used in geant4 and SAMC. This time, he looked <br>at how internal and external Bremsstrahlung are included in SAMC and the g2psim package. Ryan suggested looking at the size of the contribution from <br>internal/external Bremsstrahlung to the overall energy loss, as he found it was much smaller than the contribution from ionization. Jie showed a comparison <br>between data and simulation including two different ionization models; in one case (geant4 model) the simulation was too narrow compared to the data, in <br>the other case (SAMC model), the simulation was wider than the data. Jixie suggested to only look at the data from one sieve hole when comparing with <br>simulation, as opposed to all the sieve holes. More details can be seen in Jie's slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_09_03_simulation/Simulation_update_2014_09_03.pdf here]. | **Gave an update on the energy loss model. Last time he showed a comparison of the ionization models used in geant4 and SAMC. This time, he looked <br>at how internal and external Bremsstrahlung are included in SAMC and the g2psim package. Ryan suggested looking at the size of the contribution from <br>internal/external Bremsstrahlung to the overall energy loss, as he found it was much smaller than the contribution from ionization. Jie showed a comparison <br>between data and simulation including two different ionization models; in one case (geant4 model) the simulation was too narrow compared to the data, in <br>the other case (SAMC model), the simulation was wider than the data. Jixie suggested to only look at the data from one sieve hole when comparing with <br>simulation, as opposed to all the sieve holes. More details can be seen in Jie's slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jie/2014_09_03_simulation/Simulation_update_2014_09_03.pdf here]. | ||

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==8/27/2014== | ==8/27/2014== | ||

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Present: Min, JP, Jie, Jixie, Melissa <br> | Present: Min, JP, Jie, Jixie, Melissa <br> | ||

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*Ryan | *Ryan | ||

**Gave an update on using SAMC to generate nitrogen cross sections. He got the version of SAMC setup for SAGDH experimental conditions from Vince,<br> and used the Bosted model as the cross section model. An advantage of using SAMC is that it can include energy loss corrections and inelastic radiative <br>corrections. This will probably allow for the best comparison between the Bosted model and SAGDH nitrogen cross sections. However, the radiative <br>take a long time to run, so it may not be worthwhile. For next time, he will work on comparing the SAMC results for the XS with his method for averaging <br>the cross section over the acceptance as well as the SAMC radiative corrections with his method of radiative corrections. More details can be seen his <br>slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_082714.pdf here]. | **Gave an update on using SAMC to generate nitrogen cross sections. He got the version of SAMC setup for SAGDH experimental conditions from Vince,<br> and used the Bosted model as the cross section model. An advantage of using SAMC is that it can include energy loss corrections and inelastic radiative <br>corrections. This will probably allow for the best comparison between the Bosted model and SAGDH nitrogen cross sections. However, the radiative <br>take a long time to run, so it may not be worthwhile. For next time, he will work on comparing the SAMC results for the XS with his method for averaging <br>the cross section over the acceptance as well as the SAMC radiative corrections with his method of radiative corrections. More details can be seen his <br>slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_082714.pdf here]. | ||

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==8/20/2014== | ==8/20/2014== | ||

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Present: Kalyan, Min, JP, Jie, Jixie Melissa <br> | Present: Kalyan, Min, JP, Jie, Jixie Melissa <br> | ||

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*Jixie | *Jixie | ||

**Simulated optics events scattering from the target chamber window to see if they make it to the focal plane. He used a 1cm raster with no target field, and <br>found that events originating from the target chamber entrance window do indeed make it to the focal plane. The ratio of events from the chamber window to <br>events from the target is 3.6%. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jixie/20140820_SCWin_Sim/G2P_SC_win_elas.pdf here]. | **Simulated optics events scattering from the target chamber window to see if they make it to the focal plane. He used a 1cm raster with no target field, and <br>found that events originating from the target chamber entrance window do indeed make it to the focal plane. The ratio of events from the chamber window to <br>events from the target is 3.6%. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/jixie/20140820_SCWin_Sim/G2P_SC_win_elas.pdf here]. | ||

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==8/13/2014== | ==8/13/2014== | ||

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Present: Kalyan, Min, JP, Jixie Melissa <br> | Present: Kalyan, Min, JP, Jixie Melissa <br> | ||

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*Pengjia | *Pengjia | ||

**Posted yields calculated from pass-3 rootfiles to the ELog. The unusual shape seen in some cases is most likely due to acceptance. There is still a <br>discrepancy in the yields between different runs for some settings. | **Posted yields calculated from pass-3 rootfiles to the ELog. The unusual shape seen in some cases is most likely due to acceptance. There is still a <br>discrepancy in the yields between different runs for some settings. | ||

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==8/6/2014== | ==8/6/2014== | ||

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Present: Min, JP, Jie, Jixie, Melissa <br> | Present: Min, JP, Jie, Jixie, Melissa <br> | ||

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*Ryan | *Ryan | ||

**Gave an update on his comparison of the nitrogen XS from SAGDH data with the Bosted model. The raw XS results from SAGDH now include a multi-track<br>analysis study. To find the best scaling factor to match the data with the model, he uses a reduced chi-squared method. Vince gave him the results of an <br>elastic tail Monte Carlo used to simulate the acceptance, which also includes the "punch through" correction. Although this can't be compared to older SAGDH <br>nitrogen analysis (since the acceptance cuts have changed), but he can use the results to compare Vince's method to his. He found that his method is consistent <br>with the Monte Carlo results, and the small difference (which is a maximum of 5% in the tail), is only ~1% difference in the subtracted XS. He showed the <br>comparison of the XS from data with the Bosted for all the SADGH kinematics; each setting has a different scaling factor and shift in nu. The shift in nu is quite <br>large (6-16 MeV). To understand the energy shift, Karl suggested trying to reproduce the shift with a change in scattering angle. JP also suggested making the <br>outgoing thickness of the cell a parameter, as a small change could have a large effect. There was a question of what was included in the radiating of the Bosted <br>model; for next time he will show a comparison of the model before and after radiation. He will also work on full inelastic radiative corrections for the SAGDH data <br>so that he can extract the Born XS, which can then be compared to the Bosted model. More details can be seen in his slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_080614.pdf here]. | **Gave an update on his comparison of the nitrogen XS from SAGDH data with the Bosted model. The raw XS results from SAGDH now include a multi-track<br>analysis study. To find the best scaling factor to match the data with the model, he uses a reduced chi-squared method. Vince gave him the results of an <br>elastic tail Monte Carlo used to simulate the acceptance, which also includes the "punch through" correction. Although this can't be compared to older SAGDH <br>nitrogen analysis (since the acceptance cuts have changed), but he can use the results to compare Vince's method to his. He found that his method is consistent <br>with the Monte Carlo results, and the small difference (which is a maximum of 5% in the tail), is only ~1% difference in the subtracted XS. He showed the <br>comparison of the XS from data with the Bosted for all the SADGH kinematics; each setting has a different scaling factor and shift in nu. The shift in nu is quite <br>large (6-16 MeV). To understand the energy shift, Karl suggested trying to reproduce the shift with a change in scattering angle. JP also suggested making the <br>outgoing thickness of the cell a parameter, as a small change could have a large effect. There was a question of what was included in the radiating of the Bosted <br>model; for next time he will show a comparison of the model before and after radiation. He will also work on full inelastic radiative corrections for the SAGDH data <br>so that he can extract the Born XS, which can then be compared to the Bosted model. More details can be seen in his slides [https://userweb.jlab.org/~rbziel/Weekly_Meetings/g2p_080614.pdf here]. | ||

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==7/30/2014== | ==7/30/2014== | ||

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Present: JP, Melissa <br> | Present: JP, Melissa <br> | ||

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*Toby | *Toby | ||

**Gave an update on dilution analysis. Last time, he showed a comparison of yields from data with the prediction from the Bosted model, and then<br> scaled the model by computing an "acceptance factor". This time, he did the same thing for the 2.2 GeV settings, but found that the same acceptance <br>factor did not work for all energy settings, due to the fact that the scattering angle is different for each energy setting. Since the scattering angle is <br>dependent on nu, the acceptance factor will have to be momentum dependent. He showed plots of the scattering angle vs nu for the 3.3 and 2.2 GeV <br>settings, and fit the distribution with an exponential function (see Jixie's elog post 49 for more details). The parameters from the fit can then be used <br>to calculate the scattering angle for each momentum value in the Bosted model. This method looks promising, but there appears to be a suppression <br>of the delta in our data that does not match with simulation. From this, he will be able to extract a rough value for the dilution factor, which should be <br>available soon. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/toby/g2p%20meetings/07.30.14.pdf here]. | **Gave an update on dilution analysis. Last time, he showed a comparison of yields from data with the prediction from the Bosted model, and then<br> scaled the model by computing an "acceptance factor". This time, he did the same thing for the 2.2 GeV settings, but found that the same acceptance <br>factor did not work for all energy settings, due to the fact that the scattering angle is different for each energy setting. Since the scattering angle is <br>dependent on nu, the acceptance factor will have to be momentum dependent. He showed plots of the scattering angle vs nu for the 3.3 and 2.2 GeV <br>settings, and fit the distribution with an exponential function (see Jixie's elog post 49 for more details). The parameters from the fit can then be used <br>to calculate the scattering angle for each momentum value in the Bosted model. This method looks promising, but there appears to be a suppression <br>of the delta in our data that does not match with simulation. From this, he will be able to extract a rough value for the dilution factor, which should be <br>available soon. More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/toby/g2p%20meetings/07.30.14.pdf here]. | ||

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==7/16/2014== | ==7/16/2014== | ||

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Present: Jie, Min, Jixie, Melissa <br> | Present: Jie, Min, Jixie, Melissa <br> | ||

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'''General Discussion:''' | '''General Discussion:''' | ||

*Ryan and Toby have circulated their abstracts for the GRC. Please provide feedback! | *Ryan and Toby have circulated their abstracts for the GRC. Please provide feedback! | ||

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==7/9/2014== | ==7/9/2014== | ||

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Present: Jie, Min, Melissa <br> | Present: Jie, Min, Melissa <br> | ||

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*Melissa | *Melissa | ||

**Showed updates to her method to extract the packing fraction. Biggest change is that the input for cross sections for the various materials will be <br>determined using g2psim. Also, different runs, which have consistent beam position information, were used for the analysis. To test the conditions of <br>the simulation, she showed a comparison between simulation and data for a helium dilution run. The parameters of the simulation will need to be <br> adjusted, as there is a clear discrepancy between the simulation and data. Using the updated values for the XS, the value for the packing fraction <br>increases slightly, but will likely change as the simulation results are improved. More details can be seen in her slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/melissac/Elastic/Elastic_7_9.pdf here]. | **Showed updates to her method to extract the packing fraction. Biggest change is that the input for cross sections for the various materials will be <br>determined using g2psim. Also, different runs, which have consistent beam position information, were used for the analysis. To test the conditions of <br>the simulation, she showed a comparison between simulation and data for a helium dilution run. The parameters of the simulation will need to be <br> adjusted, as there is a clear discrepancy between the simulation and data. Using the updated values for the XS, the value for the packing fraction <br>increases slightly, but will likely change as the simulation results are improved. More details can be seen in her slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/melissac/Elastic/Elastic_7_9.pdf here]. | ||

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==7/2/2014== | ==7/2/2014== | ||

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Present: Kalyan, JP, Chao, Jie, Min, Jixie, Melissa <br> | Present: Kalyan, JP, Chao, Jie, Min, Jixie, Melissa <br> | ||

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*Toby | *Toby | ||

**Gave an update on dilution analysis. Last time there was a question about using the radiated vs unradiated Bosted model, this time he showed a comparison <br>of the two. He also updated his method to extract the dilution factor. The number of counts is defined in terms of the acceptance, luminosity, cross section and <br>time. This way, the yield scales by the acceptance, which can be assumed to be the same for each run. The yield from carbon (and helium) can be calculated using <br>dilution runs, which can then be related to a cross section using the P. Bosted model. Using the acceptance scaling factor, he can relate the nitrogen and carbon <br>yields. Using the data from the 3.3 GeV setting, the scaling factor ("a") that relates carbon to nitrogen is 1.17, but this may need to be adjusted regions (quasi-<br>elastic, delta, beyond the delta, etc.) More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/toby/g2p%20meetings/07.02.14.pdf here]. | **Gave an update on dilution analysis. Last time there was a question about using the radiated vs unradiated Bosted model, this time he showed a comparison <br>of the two. He also updated his method to extract the dilution factor. The number of counts is defined in terms of the acceptance, luminosity, cross section and <br>time. This way, the yield scales by the acceptance, which can be assumed to be the same for each run. The yield from carbon (and helium) can be calculated using <br>dilution runs, which can then be related to a cross section using the P. Bosted model. Using the acceptance scaling factor, he can relate the nitrogen and carbon <br>yields. Using the data from the 3.3 GeV setting, the scaling factor ("a") that relates carbon to nitrogen is 1.17, but this may need to be adjusted regions (quasi-<br>elastic, delta, beyond the delta, etc.) More details can be seen in his slides [http://hallaweb.jlab.org/experiment/g2p/collaborators/toby/g2p%20meetings/07.02.14.pdf here]. | ||

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## Revision as of 14:51, 23 October 2014

Minutes of the weekly analysis meetings

## Contents

- 1 10/15/2014
- 2 10/8/2014
- 3 10/1/2014
- 4 9/24/2014
- 5 9/17/2014
- 6 9/10/2014
- 7 9/3/2014
- 8 8/27/2014
- 9 8/20/2014
- 10 8/13/2014
- 11 8/6/2014
- 12 7/30/2014
- 13 7/16/2014
- 14 7/9/2014
- 15 7/2/2014
- 16 Jan-June 2014
- 17 June-Dec 2013
- 18 Jan-May 2013
- 19 April-Dec 2012
- 20 Jan-March 2012
- 21 July-Dec 2011
- 22 Jan-June 2011

## 10/15/2014

Present: Chao, Jie, Pengjia, Min, Melissa

By Phone: Toby, Ryan, Ellie

**Feature Presentations:**

- Min
- Gave an update on focal plane matching. The goal is to match focal plane data to simulation at the virtual plane. Previously, she

was doing the fit at the virtual plane using (x,θ,y,φ), this time the fit was done using (δ,θ,y,φ). Since δ doesn't change due to the

magnetic field, only θ, y and φ need to be fit. She showed the comparison between data and simulation without the fit and with up

to a 3rd order fit; the results match very well after the fit is applied. Next she will work on projecting onto the focal plane to make

the simulation match the data. More details can be seen in her slides here.

- Gave an update on focal plane matching. The goal is to match focal plane data to simulation at the virtual plane. Previously, she

- Jie
- Gave more details on his update to the energy loss model. Previously, he showed a comparison of data with simulation, including

only the energy loss due to ionization in the simulation, and found that the simulation result was wider than the data. The ionization

model used in SAMC is a Landau distribution with the most probable value at 0 and a FWHM at 4ε. He updated the model to have

a most probably value of -0.22278 and a FWHM of ε. He compared both landau distributions to a fluctuation model, and found that

the updated Landau model (with FWHM=ε) matched much better than the previous model (with FWHM=4ε). He also showed a

comparison of data from a carbon run without helium with simulation results including the complete energy loss model (ionization,

internal and external Bremsstrahlung), which match reasonably well. Next he will work on comparing data with simulation for other

target types. More details can be seen in his slides here.

- Gave more details on his update to the energy loss model. Previously, he showed a comparison of data with simulation, including

## 10/8/2014

Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Melissa

By Phone: Ryan, Ellie, Karl, Vince

**Feature Presentations:**

- Melissa
- Gave an update on packing fraction analysis. In order to combine yields from dummy and production runs, it is necessary to scale

the radiation lengths to match. The yields are generated using two different radiation thicknesses; one using the length of helium in

the dummy run, and the length of helium in the production cell. The ratio of these results gives the factor used to scale the radiation

length of the dummy run to match the radiation length of the production run. The scaling factor from using this method is close to 1.

Instead of using just the radiation length of helium in the production, the contributions from all materials should be considered, which

should make the correction larger. She is also planning to update her fitting routine to determine the contamination to the elastic peak.

Currently, the quasi-elastic peak is fit with a single gaussian, but ideally the fit should account for the helium quasi-elastic, nitrogen

quasi-elastic, and hydrogen elastic peaks. JP also suggested checking for temperature fluctuations in the target nose, since at these low

temperatures, small fluctuations could have a large effect on the density of the helium. More details can be seen in her slides here.

- Gave an update on packing fraction analysis. In order to combine yields from dummy and production runs, it is necessary to scale

- Ryan
- Gave an update on his study of the Small Angle GDH nitrogen cross sections. Showed an overview of his method and a summary of the

saGDH data available. We won't be able to get a ratio of nitrogen/carbon, because the only available carbon data has difference acceptance

cuts than the nitrogen data. He showed an example of unfolding the data for 2.1GeV at 6 degrees, using the Bosted model for the lowest

energy spectrum in the unfolding. Karl suggested checking the effect of changing the central energy of the model. To get an experimental,

unfolded cross section, the difference between the unfolded and radiated interpolated spectrum is applied to the saGDH data. He is using the

difference method, as opposed to the ratio method, because the cross section gets close to zero at some points. He also discussed his method

of error propagation. Based on conversations with Vince, he starts with a 6% systematic, and combines this with contributions from the elastic

tail subtraction and inelastic unfolding. The raw statistical error is scaled using the ratio of the unfolded and inelastic radiated cross sections.

To tune the Bosted model, he is trying to find one set of parameters that describe the saGDH data. JP pointed out that there is a visible difference

between the model and data at the quasi-elastic peak. It's possible the 2MeV binning is too fine; Ryan will look at the 10 MeV bin data to see if

it smooths out the peak. More details can be seen in his slides here.

- Gave an update on his study of the Small Angle GDH nitrogen cross sections. Showed an overview of his method and a summary of the

- Pengjia
- Is working on studying the effect of different acceptance cuts on the physics asymmetry. For each variable (x, y, theta, phi), he split the

distribution into several regions and compared the asymmetry in each region. JP suggested splitting each variable into equal regions statistically

instead of equal regions in size. For now, the dilution factor can be left out, and can be applied later when dilution factor analysis is complete.

His slides can be seen here.

- Is working on studying the effect of different acceptance cuts on the physics asymmetry. For each variable (x, y, theta, phi), he split the

- Chao
- Gave an update on optics analysis, specifically the y calibration using the target chamber upstream window. Last time he showed a first

iteration of the calibration using events from only one large hole in the sieve slit. For the second iteration, he included any possible events from

the target and the aluminum window. In addition, he added a focal plane cut to make it easier to distinguish between the sieve holes. The results

from the second iteration look pretty good, so for the LHRS calibrations he will stop here for now. The RHRS straight through calibration (with good

septum) is completed, so he will start on the longitudinal field setting for the RHRS. More details can be seen in his slides here.

- Gave an update on optics analysis, specifically the y calibration using the target chamber upstream window. Last time he showed a first

- Jie
- Gave a quick update on the energy loss model for g2psim. The main update is that the Landau distribution used for the ionization model should

be Landau(x,ε) instead of Landau(x,4ε). He will give more details next week. His slides can be seen here.

- Gave a quick update on the energy loss model for g2psim. The main update is that the Landau distribution used for the ionization model should

**General Discussion:**

- A room has been booked for the collaboration meeting on November 14th. Kalyan will set up a formal registration for the meeting.

## 10/1/2014

Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa

By Phone: Moshe, Toby, Ryan, Ellie, Karl

**Feature Presentations:**

- Toby
- Gave an update on dilution analysis. His current method involves building the total background yield from dilution runs, which are scaled

appropriately to match the radiation lengths between runs. To determine the overall systematic uncertainty, contributions come from the

packing fraction and the scaling factor gamma, which is the radiation length/nucleon scaling factor for scaling carbon dilution runs to

nitrogen. The scaling parameters alpha and beta, which are determined using simulation with the Bosted model, may also contribute to the

overall systematic. The results for the dilution factor (for the 3.3 GeV setting) seem reasonable but have a large uncertainty currently. He

also described a possible new method, which has been used previously for the RSS and SANE experiments. In this method, the yields are

determined from simulation, where the packing fraction value is an input. In this method, some of the systematics will cancel out in the

ratio used to determine the dilution factor. The downside to this method is that it requires the ratio of the simulation/data to be

kinematically independent. JP suggested trying to improve this method to rely less on the model. More details can be seen in his slides here.

- Gave an update on dilution analysis. His current method involves building the total background yield from dilution runs, which are scaled

- Min
- Gave an update on matching focal plane data in SNAKE. Her goal is to match the simulation results and focal plane data at the "virtual

plane", which is located at the entrance of Q1. This location is chosen so that changes can be applied in the septum region, not at the HRS.

She showed the comparison of simulation with data for each sieve hole before and after applying the first order fit. There was much discussion

on how to do the fit; Jixie suggested fixing the parameters a2/b2 to begin with, then tune them during the second iteration and JP suggested

fitting the offset first. There was also some discussion on how to determine the chi-squared value, specifically whether chi-sqared can be

minimized in y and phi at the same time, or whether they should be minimized separately. Jixie and Min will discuss this more offline. More

details can be seen in her slides here.

- Gave an update on matching focal plane data in SNAKE. Her goal is to match the simulation results and focal plane data at the "virtual

**General Discussion:**

- Based on the results of the poll, November 14th is the best day for a collaboration meeting. Each student will give a summary of analysis

progress (~30 minutes) and there will be time for discussion of thesis topics.

## 9/24/2014

Present: JP, Chao, Jie, Pengjia, Min, Kalyan, Jixie, Melissa

By Phone:Toby, Ryan, Ellie, Karl

**Feature Presentations:**

- Pengjia
- Gave a summary of BPM calibrations for entire experimental run. The best situation for calibrations is for data taken between May 3-7, which

includes some optics and production data. For runs taken during this time period, the average beam position and angle is 1mm and 1.1 mrad,

respectively. The biggest uncertainties are seen in data taken between March 29-31 and April 26-30. During March 29-30, both production and

optics data was taken, and the calibration became worse due to large uncertainty in the pedestal. During April 26-30, only production data was

taken and the calibration of BPM B had to be done using BPM A and harp data. JP asked how reliable these uncertainties are; Chao said that optics

data can be used to try to reconstruct the beam position, as a cross check, but he is not sure of the uncertainty of this method. The run-by-run

uncertainties are available in the mysql database. For next time, he will compile a table of contributions to the systematic uncertainty. More details

can be seen in his slides here.

- Gave a summary of BPM calibrations for entire experimental run. The best situation for calibrations is for data taken between May 3-7, which

- Ryan
- Showed a systematic error study for inelastic radiative corrections. He wanted to do a sanity check of his method to unfold/radiatively correct the

nitrogen data. He started with the Bosted model, which he radiated using SAGDH settings. He then unfolded/radiatively corrected this model, and

used the result to compare to the original Bosted model. In radiating the model, he didn't average over the scattering angle at all, and used 3MeV as

the value for Delta-E. To radiatively correct this model, it is not possible to directly unfold the equation to get an experimental Born XS, instead he

must use an iterative procedure. He showed a comparison of the Bosted model, the radiated model, and the unfolded model. The ratio of the Bosted

model compared with the radiated-then-unfolded model agree at low nu to ~1-3%. At higher nu the disagreement becomes larger, but it is never

more than 5%. This is good evidence that his method works, so going forward he will start to unfold the SAGDH data and see if he can tune the Bosted

model to match the SAGDH data set. More details can be seen in his slides here.

- Showed a systematic error study for inelastic radiative corrections. He wanted to do a sanity check of his method to unfold/radiatively correct the

**General Discussion:**

- Pengjia will be at JLab for 3 months. We should have another discussion soon about analysis tasks for students as some projects start to finish up.
- Will we try to have a collaboration meeting in mid November. Kalyan has set up a Doodle Poll to select a date - please respond!

## 9/17/2014

Present: JP, Kalyan, Min, Jie, Chao, Jixie, Melissa

By Phone:Toby, Ryan

**Feature Presentations:**

- Melissa
- Gave an update on packing fraction analysis. As was suggested previously, the differing radiation lengths between the dummy and production runs

needed to be accounted for. Following the method previously described by Toby, the he4 cross section was radiated using two different radiation

thicknesses, one that matched the empty run and one that matched the production run. The ratio of these two cross sections is then used to scale the

yield from the dummy run. The scaling factor was larger than expected, most likely due to the fact that the "radcor" program was used to radiate the

he4 cross section, and is not meant for elastic radiative corrections. Using this scaling factor, the value of the packing fraction is 0.432. The uncertainty

is still large (0.045). This includes a contribution from the difference between the sum and fitting method used to get the area of the peaks. Since the fit

is only used to determine the level of contamination, JP suggested that it shouldn't be included directly in the uncertainty. He also suggested that, in the

fit of the production run, using one gaussian peak to fit the the second peak may not be a good approximation, since the second peak contains

contributions contributions from hydrogen elastic, nitrogen quasi-elastic and helium quai-elastic. More details can be seen in her slides here.

- Gave an update on packing fraction analysis. As was suggested previously, the differing radiation lengths between the dummy and production runs

- Jie
- Gave an update on the energy loss model used in g2psim. He showed several comparisons of simulation results with data using different ionization

models. He showed a simulation results using the ionization model from geant4 combined with the bremsstrahlung model from g2psim, compared to

results using the SAMC energy loss model. There is a shift between the two results, which may result from using the mean value vs the most probable

value of the distribution. Comparing the simulation results with data, the combination of the SAMC ionization model with the SAMC bremsstrahlung

model seems to match best with the data. One update from last time, instead of using data from all sieve holes, he cut on just the center sieve hole. He

showed the step-by-step energy loss process (from SAMC), and tried switching the order to see the effect on the results. JP pointed out that the 3

middle steps actually happen simultaneously, so breaking them into steps is an approximation. More details can be seen in his slides here.

- Gave an update on the energy loss model used in g2psim. He showed several comparisons of simulation results with data using different ionization

- Chao
- Gave an optics status update, specifically a revision of the y-target calibration. Using the beam position scan isn't ideal; since we only took data at

dp=0%, the calibration will only work for a small dp range. Jixie results (using geant4) suggest that the upstream window of the target chamber has

some acceptance by the Q1 entrance. Since they have seen something upstream in the optics data, he will try to use this data to do the y-target

calibration. This result will be more reliable, as it will take all dp settings into account. He identified the data from the window, and used a vertex cut

to select them. In each setting, one hole was selected to do the calibration. The calibration result was compared to the known location of the sieve

hole. There was good agreement, which suggests the method is working. He is currently on figuring out how to check that the data is actually

coming from the upstream window. More details can be seen in his slides here.

- Gave an optics status update, specifically a revision of the y-target calibration. Using the beam position scan isn't ideal; since we only took data at

## 9/10/2014

Present: Chao, JP, Jie, Jixie, Kalyan, Melissa

By Phone: Pengjia, Toby, Ryan, Ellie

**Feature Presentations:**

- Ryan
- Gave an update on using SAMC to compare the Bosted model to SAGDH nitrogen cross sections. SAMC can include both energy loss and inelastic

radiative corrections, which makes it the best comparison to the SAGDH cross sections. However, the radiative corrections take a long time to run,

so it may not be worthwhile. To test the results of SAMC, he threw 10M events for each momentum setting, but did not turn on energy loss. He

compared this to his previous method of averaging the Bosted model result over the scattering angle. The ratio of the two methods is close to 1,

suggesting that both methods give similar results. He also did the same comparison, but first radiating SAMC/angle averaged Bosted model, (see

slide for equations). There was some discussion on whether this is the proper method to apply these corrections, but it seems that Ryan's method is

consistent with what was done previously. Of the two methods, Ryan concluded that the SAMC method isn't any better than his previous method, so

it is not worth the extra time it takes to run. JP suggested checking how much the scattering angle varies over the length of the target; if it is linear,

than using the average is a good approximation, but this may not be the case. Since there is no SAGDH carbon data that matches our kinematics (that

has been analyzed), we won't be able to do a comparison of nitrogen/carbon. Ryan plans to nail down the Bosted model so that it can be used instead;

he will scale the Bosted model to match SAGDH nitrogen data, do the same with the SAGDH carbon data, then use the ratio of these to translate the

results to our data. More details can be seen in his slides here.

- Gave an update on using SAMC to compare the Bosted model to SAGDH nitrogen cross sections. SAMC can include both energy loss and inelastic

## 9/3/2014

Present: Chao, Kalyan, Jie, Min, JP, Jixie, Melissa

By Phone: Pengjia, Toby, Ryan, Ellie, Karl, Alexandre

**Feature Presentations:**

- Toby
- Gave an update on dilution analysis. His previous method for scaling carbon data to the Bosted nitrogen model had some issues; it left a large gap

at the delta resonance, the yield was not continuous at higher values of nu (which is most likely an acceptance issue), and he assumed a constant

scaling factor in nu. In his updated method, he ran the Bosted simulation for both carbon and nitrogen, and used the ratio between the two models

as a bin-by-bin scaling factor for carbon. He also showed a method for matching the radiation lengths of the different materials. To match the

radiation lengths of two different targets, for example carbon and production, he produces two radiated carbon models. The first has the radiation

length of the carbon target, while the second uses the radiation length of the production target. The ratio of these two models is the scaling factor to

matchthe radiation length of carbon to production. JP suggested building both radiation lengths into the model, to make the process one step versus

two. Toby will look into the difference in results for the two methods. The preliminary results for the dilution factor are smaller than expected, but he

is still working on determining the uncertainty. More details can be seen in his slides here.

- Gave an update on dilution analysis. His previous method for scaling carbon data to the Bosted nitrogen model had some issues; it left a large gap

- Min
- Working on matching focal plane data to SNAKE. To accomplish this, she first divides the transport functions into two steps; the target to the virtual

plane, then the virtual plane to the focal plane. She focused on tuning the functions that included contributions from the septum field, and worked on

aligning the center sieve hole. The results look good, so for next time she will work on aligning the other sieve holes. More details can be seen in her

slides here.

- Working on matching focal plane data to SNAKE. To accomplish this, she first divides the transport functions into two steps; the target to the virtual

- Jie
- Gave an update on the energy loss model. Last time he showed a comparison of the ionization models used in geant4 and SAMC. This time, he looked

at how internal and external Bremsstrahlung are included in SAMC and the g2psim package. Ryan suggested looking at the size of the contribution from

internal/external Bremsstrahlung to the overall energy loss, as he found it was much smaller than the contribution from ionization. Jie showed a comparison

between data and simulation including two different ionization models; in one case (geant4 model) the simulation was too narrow compared to the data, in

the other case (SAMC model), the simulation was wider than the data. Jixie suggested to only look at the data from one sieve hole when comparing with

simulation, as opposed to all the sieve holes. More details can be seen in Jie's slides here.

- Gave an update on the energy loss model. Last time he showed a comparison of the ionization models used in geant4 and SAMC. This time, he looked

## 8/27/2014

Present: Min, JP, Jie, Jixie, Melissa

By Phone: Moshe, Pengjia, Toby, Ryan, Ellie, Karl, Alexandre

**Feature Presentations:**

- Moshe
- Gave an update on dilution analysis with GEp data. GEp needs an accurate dilution factor in the hydrogen-elastic region, which is tough to achieve

since there is little data and few good models for nitrogen and helium in the quasi-elastic region. One solution is to use small angle GDH data and

extrapolate to different kinematics. The second solution is to use carbon data, if it is possible to scale the carbon data to nitrogen in the quasi-elastic

setting. He showed results from simulation comparing carbon, nitrogen and helium. In the Bosted model, the quasi-elastic region of carbon and

nitrogen are scaleable, while in the QFS model, carbon, nitrogen and helium are all scaleable. In the elastic region, he scaled carbon and nitrogen data

to the same number of elastic events. With both models, this made a good match at the quasi-elastic region. Following this same procedure for

comparing helium and nitrogen, however, did not give a good match in the quasi-elastic region. Based on his simulation, the contribution from helium

is relatively small in both models. More details can be seen in his slides here.

- Gave an update on dilution analysis with GEp data. GEp needs an accurate dilution factor in the hydrogen-elastic region, which is tough to achieve

- Melissa
- Gave an update on extracting the packing fraction using data. She updated her previous method, which included input from simulation, to include

only production/dilution runs. This method assumes a uniform acceptance throughout the target cell, which can be corrected for once the acceptance

analysis is complete. Toby pointed out that helium and nitrogen have different radiation lengths, which will need to be accounted for. The resulting

value for the packing fraction agrees with the expectation, but with a large uncertainty (~10%). She will work on reducing this uncertainty, as well as

extracting the packing fraction for other materials/settings. More details can be seen in her slides here.

- Gave an update on extracting the packing fraction using data. She updated her previous method, which included input from simulation, to include

- Ryan
- Gave an update on using SAMC to generate nitrogen cross sections. He got the version of SAMC setup for SAGDH experimental conditions from Vince,

and used the Bosted model as the cross section model. An advantage of using SAMC is that it can include energy loss corrections and inelastic radiative

corrections. This will probably allow for the best comparison between the Bosted model and SAGDH nitrogen cross sections. However, the radiative

take a long time to run, so it may not be worthwhile. For next time, he will work on comparing the SAMC results for the XS with his method for averaging

the cross section over the acceptance as well as the SAMC radiative corrections with his method of radiative corrections. More details can be seen his

slides here.

- Gave an update on using SAMC to generate nitrogen cross sections. He got the version of SAMC setup for SAGDH experimental conditions from Vince,

## 8/20/2014

Present: Kalyan, Min, JP, Jie, Jixie Melissa

By Phone: Toby, Ryan, Ellie, Karl, Pengjia, Moshe, Alexandre

**Feature Presentations:**

- Jie
- Gave an update on the energy loss model being used in the g2psim package. Previously, he showed a discrepancy in the delta when comparing

data with simulation results. He was able to better match the data with simulation by using a different ionization model. The old ionization model

(taken from Geant 4) used a continuous energy loss, with fluctuations, below an energy threshold. Above the threshold, the energy loss is simulated

by the explicit secondary particles. The updated ionization model (taken from SAMC) assumes the probability distribution of energy loss by ionization

is a Landau distribution. He showed a comparison of the energy loss from ionization for g2psim and the SAMC model. If g2psim includes continuous

energy loss, but not delta-ray production, it does not match with the model. But, if g2psim includes 1 delta-ray production along with continuous energy

loss, it agrees much better with the model. More details can be seen in his slides here.

- Gave an update on the energy loss model being used in the g2psim package. Previously, he showed a discrepancy in the delta when comparing

- Min
- Gave an update on her acceptance study. Last time, she showed that there is some discrepancy between the peaks (in delta, theta and phi variables),

between data and simulation. She showed comparisons of the data and simulation with the "true" locations, and a sanity check of the transport functions,

which seem to fit our requirements for the resolution. There was some discussion about whether or not the exit/entrance windows (made of kapton and

titanium) were included in the energy loss model. Jie says they are both included right after the sieve slit. In the simulation, Min modified the VDC resolution

to be 0 and made the x-tg inputs the same, and saw good agreement between the data and simulation. However, when the VDC resolution was included back

in, she again saw a discrepancy between the data and simulation. For next time, she will also include focal plane variables. More details can be seen in her

slides here.

- Gave an update on her acceptance study. Last time, she showed that there is some discrepancy between the peaks (in delta, theta and phi variables),

- Jixie
- Simulated optics events scattering from the target chamber window to see if they make it to the focal plane. He used a 1cm raster with no target field, and

found that events originating from the target chamber entrance window do indeed make it to the focal plane. The ratio of events from the chamber window to

events from the target is 3.6%. More details can be seen in his slides here.

- Simulated optics events scattering from the target chamber window to see if they make it to the focal plane. He used a 1cm raster with no target field, and

## 8/13/2014

Present: Kalyan, Min, JP, Jixie Melissa

By Phone: Pengjia, Moshe, Alexandre, Chao

**Feature Presentations:**

- Melissa
- Gave an update on packing fraction analysis. In her current method to extract the packing fraction, the g2psim package is used to determine a value

for the cross section of different materials (nitrogen, hydrogen and helium). She showed an updated comparison of the simulation with data. The results

look better, but there are still some problems (simulation needs to be weighted by cross section, for example). There were also some questions raised

about the fitting routine used to fit the data; the Landau-Gaussian convolution fit does a good job of fitting the elastic peak, but not the radiative tail. Once

radiative corrections are included, the values of Ax (normalization factor used in packing fraction equation) will most likely change; the contribution from

Nitrogen should be larger. A suggestion was made to not use cross sections from simulation as input, but rather just use yields from data instead. She will

try this for next time. More details can be seen in her slides here.

- Gave an update on packing fraction analysis. In her current method to extract the packing fraction, the g2psim package is used to determine a value

- Pengjia
- Posted yields calculated from pass-3 rootfiles to the ELog. The unusual shape seen in some cases is most likely due to acceptance. There is still a

discrepancy in the yields between different runs for some settings.

- Posted yields calculated from pass-3 rootfiles to the ELog. The unusual shape seen in some cases is most likely due to acceptance. There is still a

## 8/6/2014

Present: Min, JP, Jie, Jixie, Melissa

By Phone: Chao, Toby, Ryan, Ellie, Pengjia, Alexandre, Karl

**Feature Presentations:**

- Min
- Gave an update on acceptance studies. In the simulation, the events are generated uniformly over the area of the raster, so she did a study to check

the beam distribution for the data. Within the raster pattern, she divided each event by the XS (which was calculated event by event using the Bosted

model). By doing this, the 2D plot of the raster pattern appears to be uniform. She also showed the corresponding 1D plots of beam x and beam y;

the beam y distribution appears to be flat while the beam x distribution has a slope on the left side. She also used the same procedure, but divided by

the Mott cross section, and saw similar results. - Also showed a comparison between data and simulation for a 2.2 GeV optics run with 0T target field. Last time, she showed a discrepancy between the

two. For this time, she updated the simulation to include a different ionization model and used the same energy loss used in optics calibrations. Using the

updated simulation, there is much better agreement between data and simulation. JP commented that we should make sure we understand where the

discrepancy came from in order to choose the best model, not just choosing the one that matches the data best, so as not to introduce bias to the analysis.

For next time, Jie will show a comparison of the two models. More details can be seen in Min's slides here.

- Gave an update on acceptance studies. In the simulation, the events are generated uniformly over the area of the raster, so she did a study to check

- Ryan
- Gave an update on his comparison of the nitrogen XS from SAGDH data with the Bosted model. The raw XS results from SAGDH now include a multi-track

analysis study. To find the best scaling factor to match the data with the model, he uses a reduced chi-squared method. Vince gave him the results of an

elastic tail Monte Carlo used to simulate the acceptance, which also includes the "punch through" correction. Although this can't be compared to older SAGDH

nitrogen analysis (since the acceptance cuts have changed), but he can use the results to compare Vince's method to his. He found that his method is consistent

with the Monte Carlo results, and the small difference (which is a maximum of 5% in the tail), is only ~1% difference in the subtracted XS. He showed the

comparison of the XS from data with the Bosted for all the SADGH kinematics; each setting has a different scaling factor and shift in nu. The shift in nu is quite

large (6-16 MeV). To understand the energy shift, Karl suggested trying to reproduce the shift with a change in scattering angle. JP also suggested making the

outgoing thickness of the cell a parameter, as a small change could have a large effect. There was a question of what was included in the radiating of the Bosted

model; for next time he will show a comparison of the model before and after radiation. He will also work on full inelastic radiative corrections for the SAGDH data

so that he can extract the Born XS, which can then be compared to the Bosted model. More details can be seen in his slides here.

- Gave an update on his comparison of the nitrogen XS from SAGDH data with the Bosted model. The raw XS results from SAGDH now include a multi-track

## 7/30/2014

Present: JP, Melissa

By Phone: Toby, Ryan, Ellie, Pengjia, Alexandre

**Feature Presentations:**

- Toby
- Gave an update on dilution analysis. Last time, he showed a comparison of yields from data with the prediction from the Bosted model, and then

scaled the model by computing an "acceptance factor". This time, he did the same thing for the 2.2 GeV settings, but found that the same acceptance

factor did not work for all energy settings, due to the fact that the scattering angle is different for each energy setting. Since the scattering angle is

dependent on nu, the acceptance factor will have to be momentum dependent. He showed plots of the scattering angle vs nu for the 3.3 and 2.2 GeV

settings, and fit the distribution with an exponential function (see Jixie's elog post 49 for more details). The parameters from the fit can then be used

to calculate the scattering angle for each momentum value in the Bosted model. This method looks promising, but there appears to be a suppression

of the delta in our data that does not match with simulation. From this, he will be able to extract a rough value for the dilution factor, which should be

available soon. More details can be seen in his slides here.

- Gave an update on dilution analysis. Last time, he showed a comparison of yields from data with the prediction from the Bosted model, and then

## 7/16/2014

Present: Jie, Min, Jixie, Melissa

By Phone: Toby, Ryan, Ellie, Karl, Pengjia

**Feature Presentations:**

- Min
- Working on an acceptance study for the 1st and 3rd septum settings. For looking at data from optics runs, she applies focal plane and target cuts to

get rid of junk events and select only elastic events. For this time, she updated the beam cut to match what Chao used for the optics calibrations. For

the simulation, elastic events are generated according to the beam position in the cut. For the dilution run (empty run), the procedure is similar, but she

applies a target plane graphical cut on the data instead of a focal plane cut. To simulate the empty run, she used the same target plane cuts that were

applied to the data, but generated events in an ellipse. For both the optics and dilution runs, the theta and phi variables agree reasonably well, but there

is a discrepancy in the dp variable. For next time, she will look into this discrepancy as well as look at the other settings. More details can be seen in her

slides here.

- Working on an acceptance study for the 1st and 3rd septum settings. For looking at data from optics runs, she applies focal plane and target cuts to

- Ryan
- Showed a comparison of the Bosted Model with SAGDH data. He generated the nitrogen cross section using the Bosted model for each of the SAGDH

kinematics, then he can radiate the model for each reconstructed scattering angle, within acceptance. In order to compare to SAGDH data, he averaged

over the scattering angles. Previously, he tried to determine a single scaling factor for all the kinematic settings, this time he chose different scaling

factors for each setting to best match the data. For each setting, he found that averaging over the scattering angle decreases the scaling factor by about

5%. Karl suggested using another data set to compare, possibly using our data to extract the carbon cross section. For the future, he will consider the

effect of the punch through from the collimators, which effectively increases the radiation length. He will also look at the SAGDH data for

two settings that he hasn't looked at before (9deg/2234 MeV and 9deg/3319 MeV), among other things. More details can be seen in his slides here.

- Showed a comparison of the Bosted Model with SAGDH data. He generated the nitrogen cross section using the Bosted model for each of the SAGDH

- Jie
- Gave an update on packing fraction analysis. Last time, he used runs from the 2nd septum setting (40-32-16). Since the SNAKE model is not quite

ready for this setting yet, this time he analyzed a set of runs from the 2.2 GeV, 5T, longitudinal setting, which uses the 3rd septum setting (40-00-16).

He applied a 2D graphical cut to select elastic events, though Karl pointed out that this isn't a 100% pure elastic sample, as there could be a tail underneath

the peak. Using this set of runs, he determined the packing fraction to be 0.51, with an uncertainty of 7.6%. The largest contribution to this uncertainty

comes from the uncertainty of the absolute beam position. Ellie suggested showing a comparison of the XS models (that are used as input) to data to test

how well they match, which Jie will work on for next time. More details can be seen in his slides here.

- Gave an update on packing fraction analysis. Last time, he used runs from the 2nd septum setting (40-32-16). Since the SNAKE model is not quite

**General Discussion:**

- Ryan and Toby have circulated their abstracts for the GRC. Please provide feedback!

## 7/9/2014

Present: Jie, Min, Melissa

By Phone: Toby, Ryan, Ellie, Karl, Pengjia

**Feature Presentations:**

- Melissa
- Showed updates to her method to extract the packing fraction. Biggest change is that the input for cross sections for the various materials will be

determined using g2psim. Also, different runs, which have consistent beam position information, were used for the analysis. To test the conditions of

the simulation, she showed a comparison between simulation and data for a helium dilution run. The parameters of the simulation will need to be

adjusted, as there is a clear discrepancy between the simulation and data. Using the updated values for the XS, the value for the packing fraction

increases slightly, but will likely change as the simulation results are improved. More details can be seen in her slides here.

- Showed updates to her method to extract the packing fraction. Biggest change is that the input for cross sections for the various materials will be

## 7/2/2014

Present: Kalyan, JP, Chao, Jie, Min, Jixie, Melissa

By Phone: Toby, Ryan, Ellie, Karl, Pengjia, Alexandre

**Feature Presentations:**

- Min
- Working on an acceptance study for the 3rd ("very bad") septum configuration, using a Monte-Carlo simulation. She started with optics and dilution runs,

since they have a simple target. Loose cuts were applied to throw away junk events, and to select elastic events. She showed a comparison of simulation vs

data; for the 1.7 GeV setting (empty cell run), the simulation results are smaller than the data, but for the 2.2 GeV setting, the simulation is larger than the data.

Also, the shape

of the phi distributions from simulation do not match the data. JP suggested this could be a result of the momentum calibration or energy

loss being slightly off. For next time, she will look at a setting with the "good" septum configuration. Also, she will look into the delta discrepancy for the elastic

setting and will work on tuning the apertures for theta/phi matching (boundary matching). Additionally, the simulation needs to be updated to reflect the true

shape of the beam, which is elliptical, not circular. More details can be seen in her slides here.

- Working on an acceptance study for the 3rd ("very bad") septum configuration, using a Monte-Carlo simulation. She started with optics and dilution runs,

- Jie
- Gave an update on simulations. Last time he showed an update to the event generator. This time, he wanted to check the difference in the phase space

density. He showed a comparison of the density function vs theta for two different values of phi-target; the difference between them was very small. He also

showed an update of the packing fraction uncertainty. He determined the relative uncertainty to be 7.19% for a 1mrad shift in the scattering angle. He showed

the beam information for the 3 runs being used in the packing fraction calculation (a production, dummy and carbon run), and the beam position seemed

consistent for all 3 runs. JP expressed concern that this beam position calibration is too good, and doesn't reflect the actual beam conditions. For next time,

Jie will show the beam position event by event. More details can be seen in his slides here.

- Gave an update on simulations. Last time he showed an update to the event generator. This time, he wanted to check the difference in the phase space

- Ryan
- Showed a comparison of small angle GDH data with the P. Bosted model. He generated a nitrogen cross section using the Bosted model, then inelastically

radiated it so that it could be compared with the SAGDH data (the SAGDH data already has the elastic tail subtracted). He showed comparisons for several

different energy settings, in all cases the Bosted XS had been scaled down by 30%. For next time, he will check the effect of averaging over the scattering angle;

the Bosted model is calculated at one scattering angle, while the SAGDH data is broken up into multiple bins. He will also repeat this study using QFS and do full

inelastic radiative corrections on the SAGDH data in order to extract the Born cross section. More details can be seen in his slides here.

- Showed a comparison of small angle GDH data with the P. Bosted model. He generated a nitrogen cross section using the Bosted model, then inelastically

- Toby
- Gave an update on dilution analysis. Last time there was a question about using the radiated vs unradiated Bosted model, this time he showed a comparison

of the two. He also updated his method to extract the dilution factor. The number of counts is defined in terms of the acceptance, luminosity, cross section and

time. This way, the yield scales by the acceptance, which can be assumed to be the same for each run. The yield from carbon (and helium) can be calculated using

dilution runs, which can then be related to a cross section using the P. Bosted model. Using the acceptance scaling factor, he can relate the nitrogen and carbon

yields. Using the data from the 3.3 GeV setting, the scaling factor ("a") that relates carbon to nitrogen is 1.17, but this may need to be adjusted regions (quasi-

elastic, delta, beyond the delta, etc.) More details can be seen in his slides here.

- Gave an update on dilution analysis. Last time there was a question about using the radiated vs unradiated Bosted model, this time he showed a comparison