1 / 11

Simulating photonuclear interactions with MMC

Simulating photonuclear interactions with MMC. Dmitry Chirkin UC Berkeley. The Models. photoproduction. DIS. Q 2. soft. hard. 1 GeV 2. Abramowicz Levin Levy Maor. Bezrukov-Bugaev. Butkevich-Mikheyev. BB 1981. 2002. 1991. 1997. ZEUS 94. Nuclear effects. BB + Hard 03

xenia
Download Presentation

Simulating photonuclear interactions with MMC

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. Simulating photonuclear interactions with MMC Dmitry Chirkin UC Berkeley

  2. The Models photoproduction DIS Q2 soft hard 1 GeV2 Abramowicz Levin Levy Maor Bezrukov-Bugaev Butkevich-Mikheyev BB 1981 2002 1991 1997 ZEUS 94 Nuclear effects BB + Hard 03 Bugaev Shlepin Kokoulin 99 Dutta Smirnov

  3. All photonuclear cross sections • As generated by MMC Standard rock Water

  4. Sources • ALLM: Dutta, Seckel, et al. 2000 • BB, ZEUS, BB+BS, ALLM: Sokalski et al. 2002 • BM, BB: Butkevich, Mikheyev 2002 • BB, BB+BS, ALLM for taus: Bugaev et al. 2003 • BB, BB+BS for taus: Bugaev, Shlepin 2003

  5. ALLM from Dutta Seckel • Photon-nucleon cross section

  6. ALLM from Dutta Seckel • Muon photonuclear cross section from Dutta Seckel

  7. Bezrukov-Bugaev from Sokalski • Comparison of BB1981 and ZEUS95 parameterizations

  8. BB+Bugaev-Shlepin from Bugaev Shlepin Comparison with BB1981, ALLM, and Butkevich-Mikheyev from Sokalski

  9. Butkevich-Mikheyev from Butkevich Mikheyev • BM, BB from Sokalski

  10. BB+Bugaev-Shlepin (taus) from Bugaev • BB+BS, ALLM: tau propagation from Bugaev Shlepin

  11. Conclusions • Plots of photonuclear cross section change from one publication to another, some of this can be explained by use of different shadowing functions. • ALLM 97 parameterization is currently used in AMANDA. Its results are very similar to Butkevich-Mikheyev parameterization. • Switching to the newer nuclear structure function as described in B-M will bring the ALLM 97 model closer to the new BB+BS parameterization.

More Related