1 / 32

Topics

Topics. History General framework Details Some results Topics of interest. E( w ), A( w ), J( x,t ) components phases separation of variables, convolution. Normalization, spectrum of secondaries Longitudinal Transverse Shower front. CROME n(z) and inclined showers

giza
Télécharger la présentation

Topics

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. D. Seckel, Univ. of Delaware

  2. Topics • History • General framework • Details • Some results • Topics of interest • E(w), A(w), J(x,t) • components • phases • separation of variables, convolution • Normalization, spectrum of secondaries • Longitudinal • Transverse • Shower front • CROME • n(z) and inclined showers • Proposal for fitting

  3. History • 2009/2010: ANITA – 16 hpol events • energy uncertain, models for lower f, reflection, geometry • Attempt semi-analytic model with n(z) • Apply to Haverah Park (Allan) • Apply to some LOPES events • Get lost on shower detail … pause • Resolve shower details • Compare to REAS-3. [Remove n(z), disable some terms] • Use for RASTA … pause • Add in non-REAS, n(z) features • Test higher freq - ANITA, CROME ?

  4. E and A General In-Ice

  5. Separation and Convolution

  6. Convolution over secondary energies

  7. Components of j

  8. Co-ordinates & Displacements

  9. Charge Excess and Dipole

  10. Transverse currents

  11. Terms in current

  12. Normalization • Scale to 1 PeV shower in-ice

  13. Spectrum of secondaries Shape is by eye to Fluka/Geant 100 GeV showers – not crazy, but could do better.

  14. Longitudinal Integral

  15. Effective emission height • At high freq, phase dominates over shower profile.

  16. Transverse profile • started with Gaussian profiles • tried to reproduce 50 yrs of work on shower physics • give up and use NKG • Integrate over secondary particle energy from 10 MeV – 100 GeV

  17. Shower Front • time delays taken from Lafebre, etal • Also scales with secondary energies

  18. Some results: A south pole shower

  19. Part of a rasta event

  20. overall event comparison

  21. 100 events … 74 antennas

  22. Adding in other terms

  23. CROME

  24. CROME-II

  25. Proposal to describe shower

  26. Summary • semi-analytic with B • components of radiation • phases to second order • shower profiles matter • scale with and integrate over secondary energy • tested against reas for south pole atm. • include additional terms (test against coreas …) • qualitative features of CROME simulation • propose vector E as intermediate for reconstruction

  27. Extra Slides

  28. “true” Cherenkov

  29. Phases to 2nd order in displacement

  30. CPU efficiency • 64 antenna test events … about 50 mins • in Mathematica on my laptop • estimate to compiled version ~1sec/antenna • This is with about 150 frequency points from 100 KHz to 3 GHz, sparsely sampled and interpolated for FFT. • Most time spent in longitudinal integrals

More Related