The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice

L. Cremonesi; A. Connolly; P. Allison; O. Banerjee; L. Batten; J. J. Beatty; K. Bechtol; K. Belov; D. Z. Besson; W. R. Binns; V. Bugaev; P. Cao; C. C. Chen; C. H. Chen; P. Chen; J. M. Clem; B. Dailey; C. Deaconu; P. F. Dowkontt; B. D. Fox; J. W.H. Gordon; P. W. Gorham; B. Hill; J. J. Huang; K. Hughes; R. Hupe; M. H. Israel; K. M. Liewer; S. Y. Lin; T. C. Liu; A. B. Ludwig; L. Macchiarulo; S. Matsuno; K. McBride; C. Miki; K. Mulrey; J. Nam; R. J. Nichol; A. Novikov; E. Oberla; S. Prohira; B. F. Rauch; J. M. Roberts; A. Romero-Wolf; B. Rotter; J. W. Russell; D. Saltzberg; D. Seckel; H. Schoorlemmer; J. Shiao; S. Stafford; J. Stockham; M. Stockham; B. Strutt; J. Stuhr; M. Sutherland; G. S. Varner; A. G. Vieregg; S. H. Wang; S. A. Wissel

doi:10.1088/1748-0221/14/08/P08011

The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice

L. Cremonesi^*, A. Connolly, P. Allison, O. Banerjee, L. Batten, J. J. Beatty, K. Bechtol, K. Belov, D. Z. Besson, W. R. Binns, V. Bugaev, P. Cao, C. C. Chen, C. H. Chen, P. Chen, J. M. Clem, B. Dailey, C. Deaconu, P. F. Dowkontt, B. D. FoxJ. W.H. Gordon, P. W. Gorham, B. Hill, J. J. Huang, K. Hughes, R. Hupe, M. H. Israel, K. M. Liewer, S. Y. Lin, T. C. Liu, A. B. Ludwig, L. Macchiarulo, S. Matsuno, K. McBride, C. Miki, K. Mulrey, J. Nam, R. J. Nichol, A. Novikov, E. Oberla, S. Prohira, B. F. Rauch, J. M. Roberts, A. Romero-Wolf, B. Rotter, J. W. Russell, D. Saltzberg, D. Seckel, H. Schoorlemmer, J. Shiao, S. Stafford, J. Stockham, M. Stockham, B. Strutt, J. Stuhr, M. Sutherland, G. S. Varner, A. G. Vieregg, S. H. Wang, S. A. Wissel

^*此作品的通信作者

電子物理學系

研究成果: Article › 同行評審

6 引文斯高帕斯（Scopus）

摘要

A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.

原文	English
文章編號	P08011
期刊	Journal of Instrumentation
卷	14
發行號	8
DOIs	https://doi.org/10.1088/1748-0221/14/08/P08011
出版狀態	Published - 8 8月 2019

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10.1088/1748-0221/14/08/P08011

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Cremonesi, L., Connolly, A., Allison, P., Banerjee, O., Batten, L., Beatty, J. J., Bechtol, K., Belov, K., Besson, D. Z., Binns, W. R., Bugaev, V., Cao, P., Chen, C. C., Chen, C. H., Chen, P., Clem, J. M., Dailey, B., Deaconu, C., Dowkontt, P. F., ... Wissel, S. A. (2019). The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice. Journal of Instrumentation, 14(8), 文章 P08011. https://doi.org/10.1088/1748-0221/14/08/P08011

@article{a1b98d7c78e2417cbcd208468bba6c60,

title = "The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice",

abstract = "A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.",

keywords = "Balloon instrumentation, Neutrino detectors, Particle detectors, Simulation methods and programs",

author = "L. Cremonesi and A. Connolly and P. Allison and O. Banerjee and L. Batten and Beatty, {J. J.} and K. Bechtol and K. Belov and Besson, {D. Z.} and Binns, {W. R.} and V. Bugaev and P. Cao and Chen, {C. C.} and Chen, {C. H.} and P. Chen and Clem, {J. M.} and B. Dailey and C. Deaconu and Dowkontt, {P. F.} and Fox, {B. D.} and Gordon, {J. W.H.} and Gorham, {P. W.} and B. Hill and Huang, {J. J.} and K. Hughes and R. Hupe and Israel, {M. H.} and Liewer, {K. M.} and Lin, {S. Y.} and Liu, {T. C.} and Ludwig, {A. B.} and L. Macchiarulo and S. Matsuno and K. McBride and C. Miki and K. Mulrey and J. Nam and Nichol, {R. J.} and A. Novikov and E. Oberla and S. Prohira and Rauch, {B. F.} and Roberts, {J. M.} and A. Romero-Wolf and B. Rotter and Russell, {J. W.} and D. Saltzberg and D. Seckel and H. Schoorlemmer and J. Shiao and S. Stafford and J. Stockham and M. Stockham and B. Strutt and J. Stuhr and M. Sutherland and Varner, {G. S.} and Vieregg, {A. G.} and Wang, {S. H.} and Wissel, {S. A.}",

year = "2019",

month = aug,

day = "8",

doi = "10.1088/1748-0221/14/08/P08011",

language = "English",

volume = "14",

journal = "Journal of Instrumentation",

issn = "1748-0221",

publisher = "IOP Publishing Ltd.",

number = "8",

}

Cremonesi, L, Connolly, A, Allison, P, Banerjee, O, Batten, L, Beatty, JJ, Bechtol, K, Belov, K, Besson, DZ, Binns, WR, Bugaev, V, Cao, P, Chen, CC, Chen, CH, Chen, P, Clem, JM, Dailey, B, Deaconu, C, Dowkontt, PF, Fox, BD, Gordon, JWH, Gorham, PW, Hill, B, Huang, JJ, Hughes, K, Hupe, R, Israel, MH, Liewer, KM, Lin, SY, Liu, TC, Ludwig, AB, Macchiarulo, L, Matsuno, S, McBride, K, Miki, C, Mulrey, K, Nam, J, Nichol, RJ, Novikov, A, Oberla, E, Prohira, S, Rauch, BF, Roberts, JM, Romero-Wolf, A, Rotter, B, Russell, JW, Saltzberg, D, Seckel, D, Schoorlemmer, H, Shiao, J, Stafford, S, Stockham, J, Stockham, M, Strutt, B, Stuhr, J, Sutherland, M, Varner, GS, Vieregg, AG, Wang, SH & Wissel, SA 2019, 'The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice', Journal of Instrumentation, 卷 14, 編號 8, P08011. https://doi.org/10.1088/1748-0221/14/08/P08011

TY - JOUR

T1 - The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice

AU - Cremonesi, L.

AU - Connolly, A.

AU - Allison, P.

AU - Banerjee, O.

AU - Batten, L.

AU - Beatty, J. J.

AU - Bechtol, K.

AU - Belov, K.

AU - Besson, D. Z.

AU - Binns, W. R.

AU - Bugaev, V.

AU - Cao, P.

AU - Chen, C. C.

AU - Chen, C. H.

AU - Chen, P.

AU - Clem, J. M.

AU - Dailey, B.

AU - Deaconu, C.

AU - Dowkontt, P. F.

AU - Fox, B. D.

AU - Gordon, J. W.H.

AU - Gorham, P. W.

AU - Hill, B.

AU - Huang, J. J.

AU - Hughes, K.

AU - Hupe, R.

AU - Israel, M. H.

AU - Liewer, K. M.

AU - Lin, S. Y.

AU - Liu, T. C.

AU - Ludwig, A. B.

AU - Macchiarulo, L.

AU - Matsuno, S.

AU - McBride, K.

AU - Miki, C.

AU - Mulrey, K.

AU - Nam, J.

AU - Nichol, R. J.

AU - Novikov, A.

AU - Oberla, E.

AU - Prohira, S.

AU - Rauch, B. F.

AU - Roberts, J. M.

AU - Romero-Wolf, A.

AU - Rotter, B.

AU - Russell, J. W.

AU - Saltzberg, D.

AU - Seckel, D.

AU - Schoorlemmer, H.

AU - Shiao, J.

AU - Stafford, S.

AU - Stockham, J.

AU - Stockham, M.

AU - Strutt, B.

AU - Stuhr, J.

AU - Sutherland, M.

AU - Varner, G. S.

AU - Vieregg, A. G.

AU - Wang, S. H.

AU - Wissel, S. A.

PY - 2019/8/8

Y1 - 2019/8/8

N2 - A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.

AB - A Monte Carlo simulation program for the radio detection of Ultra High Energy (UHE) neutrino interactions in the Antarctic ice as viewed by the Antarctic Impulsive Transient Antenna (ANITA) is described in this article. The program, icemc, provides an input spectrum of UHE neutrinos, the parametrization of the Askaryan radiation generated by their interaction in the ice, and the propagation of the radiation through ice and air to a simulated model of the third and fourth ANITA flights. This paper provides an overview of the icemc simulation, descriptions of the physics models used and of the ANITA electronics processing chain, data/simulation comparisons to validate the predicted performance, and a summary of the impact of published results.

KW - Balloon instrumentation

KW - Neutrino detectors

KW - Particle detectors

KW - Simulation methods and programs

UR - http://www.scopus.com/inward/record.url?scp=85072712424&partnerID=8YFLogxK

U2 - 10.1088/1748-0221/14/08/P08011

DO - 10.1088/1748-0221/14/08/P08011

M3 - Article

AN - SCOPUS:85072712424

SN - 1748-0221

VL - 14

JO - Journal of Instrumentation

JF - Journal of Instrumentation

IS - 8

M1 - P08011

ER -

The simulation of the sensitivity of the Antarctic Impulsive Transient Antenna (ANITA) to Askaryan radiation from cosmogenic neutrinos interacting in the Antarctic Ice

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