Results from the Anita experiment

Andrea Silvestri; S. W. Barwick; J. J. Beatty; D. Z. Besson; W. R. Binns; B. Cai; J. M. Clem; A. Connolly; D. F. Cowen; P. F. Dowkontt; M. A. Du Vernois; P. A. Evenson; D. Goldstein; P. W. Gorham; C. L. Hebert; M. H. Israel; J. G. Learned; K. M. Liewer; J. T. Link; S. Matsuno; P. Miocinovic; J. Nam; C. J. Naudet; R. Nichol; K. Palladino; M. Rosen; D. Saltzberg; D. Seckel; A. Silvestri; B. T. Stokes; G. S. Varner; F. Wu

doi:10.1142/S0217732307024279

Results from the Anita experiment

Andrea Silvestri
, S. W. Barwick
, J. J. Beatty
, D. Z. Besson
, W. R. Binns
, B. Cai
, J. M. Clem
, A. Connolly
, D. F. Cowen
, P. F. Dowkontt
, M. A. Du Vernois
, P. A. Evenson
, D. Goldstein
, P. W. Gorham
, C. L. Hebert
, M. H. Israel
, J. G. Learned
, K. M. Liewer
, J. T. Link
, S. Matsuno

P. Miocinovic, J. Nam, C. J. Naudet, R. Nichol, K. Palladino, M. Rosen, D. Saltzberg, D. Seckel, A. Silvestri, B. T. Stokes, G. S. Varner, F. Wu

Research output: Contribution to journal › Review article › peer-review

2 Scopus citations

Abstract

The ANtarctic Impulse Transient Antenna (ANITA) is the first long-duration balloon experiment designed to search and measure the flux of Greisen-Zapsepin-Kuzmin (GZK) neutrinos. We present new limits on neutrinos fluxes of astronomical origin from data collected with the successful launch of a 2-antenna prototype instrument, called ANITA-lite, that circled the Antarctic continent for 18.4 days in January 2004. We performed a search for Ultra-High-Energy (UHE) neutrinos with energies above 3 × 10¹⁸ eV. No excess events above the background expectation were observed and a neutrino flux following E^-2 spectrum for all neutrino flavors, is limited to E_v^-2F < 1.6 × 10^-6 GeV cm^-2 s^-1 sr^-1 for 10^18.5 eV < E_v < 10^23.5 eV at 90% confidence level. The launch of ANITA is scheduled for December 2006. Looking beyond ANITA, we describe a new idea, called ARIANNA (Antarctic Ross Iceshelf ANtenna Neutrino Array), to increase the sensitivity for GZK neutrinos by one order of magnitude better than ANITA.

Original language	English (US)
Pages (from-to)	2237-2246
Number of pages	10
Journal	Modern Physics Letters A
Volume	22
Issue number	30
DOIs	https://doi.org/10.1142/S0217732307024279
State	Published - Sep 28 2007

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics
Astronomy and Astrophysics
General Physics and Astronomy

Access to Document

10.1142/S0217732307024279

Cite this

Silvestri, A., Barwick, S. W., Beatty, J. J., Besson, D. Z., Binns, W. R., Cai, B., Clem, J. M., Connolly, A., Cowen, D. F., Dowkontt, P. F., Du Vernois, M. A., Evenson, P. A., Goldstein, D., Gorham, P. W., Hebert, C. L., Israel, M. H., Learned, J. G., Liewer, K. M., Link, J. T., ... Wu, F. (2007). Results from the Anita experiment. Modern Physics Letters A, 22(30), 2237-2246. https://doi.org/10.1142/S0217732307024279

@article{b946cd5a4ca74e7fbbc608431897a347,

title = "Results from the Anita experiment",

abstract = "The ANtarctic Impulse Transient Antenna (ANITA) is the first long-duration balloon experiment designed to search and measure the flux of Greisen-Zapsepin-Kuzmin (GZK) neutrinos. We present new limits on neutrinos fluxes of astronomical origin from data collected with the successful launch of a 2-antenna prototype instrument, called ANITA-lite, that circled the Antarctic continent for 18.4 days in January 2004. We performed a search for Ultra-High-Energy (UHE) neutrinos with energies above 3 × 1018 eV. No excess events above the background expectation were observed and a neutrino flux following E-2 spectrum for all neutrino flavors, is limited to Ev-2F < 1.6 × 10-6 GeV cm-2 s-1 sr-1 for 1018.5 eV < Ev < 1023.5 eV at 90\% confidence level. The launch of ANITA is scheduled for December 2006. Looking beyond ANITA, we describe a new idea, called ARIANNA (Antarctic Ross Iceshelf ANtenna Neutrino Array), to increase the sensitivity for GZK neutrinos by one order of magnitude better than ANITA.",

author = "Andrea Silvestri and Barwick, \{S. W.\} and Beatty, \{J. J.\} and Besson, \{D. Z.\} and Binns, \{W. R.\} and B. Cai and Clem, \{J. M.\} and A. Connolly and Cowen, \{D. F.\} and Dowkontt, \{P. F.\} and \{Du Vernois\}, \{M. A.\} and Evenson, \{P. A.\} and D. Goldstein and Gorham, \{P. W.\} and Hebert, \{C. L.\} and Israel, \{M. H.\} and Learned, \{J. G.\} and Liewer, \{K. M.\} and Link, \{J. T.\} and S. Matsuno and P. Miocinovic and J. Nam and Naudet, \{C. J.\} and R. Nichol and K. Palladino and M. Rosen and D. Saltzberg and D. Seckel and A. Silvestri and Stokes, \{B. T.\} and Varner, \{G. S.\} and F. Wu",

note = "Funding Information: The author acknowledges support by the following agencies: NASA Research Opportunities in Space Science (ROSS) — The UH grant number is NASA NAG5-5387, Research Opportunities in Space Science – NSF and Raytheon Polar Services for Antarctic Support — NSBF for Balloon Launching and Operations — TIGER Collaboration for allowing ANITA-lite to fly as a piggyback — the Phi Beta Kappa Alumni in Southern California for providing travel grants — the Astrophysics Associates, Inc. — Italian Ministry of Education, European Physical Society – Ettore Majorana Foundation — Electron Tubes, Ltd. for providing the full scholarship at Erice.",

year = "2007",

month = sep,

day = "28",

doi = "10.1142/S0217732307024279",

language = "English (US)",

volume = "22",

pages = "2237--2246",

journal = "Modern Physics Letters A",

issn = "0217-7323",

publisher = "World Scientific Publishing Co. Pte Ltd",

number = "30",

}

Silvestri, A, Barwick, SW, Beatty, JJ, Besson, DZ, Binns, WR, Cai, B, Clem, JM, Connolly, A, Cowen, DF, Dowkontt, PF, Du Vernois, MA, Evenson, PA, Goldstein, D, Gorham, PW, Hebert, CL, Israel, MH, Learned, JG, Liewer, KM, Link, JT, Matsuno, S, Miocinovic, P, Nam, J, Naudet, CJ, Nichol, R, Palladino, K, Rosen, M, Saltzberg, D, Seckel, D, Silvestri, A, Stokes, BT, Varner, GS & Wu, F 2007, 'Results from the Anita experiment', Modern Physics Letters A, vol. 22, no. 30, pp. 2237-2246. https://doi.org/10.1142/S0217732307024279

TY - JOUR

T1 - Results from the Anita experiment

AU - Silvestri, Andrea

AU - Barwick, S. W.

AU - Beatty, J. J.

AU - Besson, D. Z.

AU - Binns, W. R.

AU - Cai, B.

AU - Clem, J. M.

AU - Connolly, A.

AU - Cowen, D. F.

AU - Dowkontt, P. F.

AU - Du Vernois, M. A.

AU - Evenson, P. A.

AU - Goldstein, D.

AU - Gorham, P. W.

AU - Hebert, C. L.

AU - Israel, M. H.

AU - Learned, J. G.

AU - Liewer, K. M.

AU - Link, J. T.

AU - Matsuno, S.

AU - Miocinovic, P.

AU - Nam, J.

AU - Naudet, C. J.

AU - Nichol, R.

AU - Palladino, K.

AU - Rosen, M.

AU - Saltzberg, D.

AU - Seckel, D.

AU - Silvestri, A.

AU - Stokes, B. T.

AU - Varner, G. S.

AU - Wu, F.

N1 - Funding Information: The author acknowledges support by the following agencies: NASA Research Opportunities in Space Science (ROSS) — The UH grant number is NASA NAG5-5387, Research Opportunities in Space Science – NSF and Raytheon Polar Services for Antarctic Support — NSBF for Balloon Launching and Operations — TIGER Collaboration for allowing ANITA-lite to fly as a piggyback — the Phi Beta Kappa Alumni in Southern California for providing travel grants — the Astrophysics Associates, Inc. — Italian Ministry of Education, European Physical Society – Ettore Majorana Foundation — Electron Tubes, Ltd. for providing the full scholarship at Erice.

PY - 2007/9/28

Y1 - 2007/9/28

N2 - The ANtarctic Impulse Transient Antenna (ANITA) is the first long-duration balloon experiment designed to search and measure the flux of Greisen-Zapsepin-Kuzmin (GZK) neutrinos. We present new limits on neutrinos fluxes of astronomical origin from data collected with the successful launch of a 2-antenna prototype instrument, called ANITA-lite, that circled the Antarctic continent for 18.4 days in January 2004. We performed a search for Ultra-High-Energy (UHE) neutrinos with energies above 3 × 1018 eV. No excess events above the background expectation were observed and a neutrino flux following E-2 spectrum for all neutrino flavors, is limited to Ev-2F < 1.6 × 10-6 GeV cm-2 s-1 sr-1 for 1018.5 eV < Ev < 1023.5 eV at 90% confidence level. The launch of ANITA is scheduled for December 2006. Looking beyond ANITA, we describe a new idea, called ARIANNA (Antarctic Ross Iceshelf ANtenna Neutrino Array), to increase the sensitivity for GZK neutrinos by one order of magnitude better than ANITA.

AB - The ANtarctic Impulse Transient Antenna (ANITA) is the first long-duration balloon experiment designed to search and measure the flux of Greisen-Zapsepin-Kuzmin (GZK) neutrinos. We present new limits on neutrinos fluxes of astronomical origin from data collected with the successful launch of a 2-antenna prototype instrument, called ANITA-lite, that circled the Antarctic continent for 18.4 days in January 2004. We performed a search for Ultra-High-Energy (UHE) neutrinos with energies above 3 × 1018 eV. No excess events above the background expectation were observed and a neutrino flux following E-2 spectrum for all neutrino flavors, is limited to Ev-2F < 1.6 × 10-6 GeV cm-2 s-1 sr-1 for 1018.5 eV < Ev < 1023.5 eV at 90% confidence level. The launch of ANITA is scheduled for December 2006. Looking beyond ANITA, we describe a new idea, called ARIANNA (Antarctic Ross Iceshelf ANtenna Neutrino Array), to increase the sensitivity for GZK neutrinos by one order of magnitude better than ANITA.

UR - https://www.scopus.com/pages/publications/34548567736

UR - https://www.scopus.com/pages/publications/34548567736#tab=citedBy

U2 - 10.1142/S0217732307024279

DO - 10.1142/S0217732307024279

M3 - Review article

AN - SCOPUS:34548567736

SN - 0217-7323

VL - 22

SP - 2237

EP - 2246

JO - Modern Physics Letters A

JF - Modern Physics Letters A

IS - 30

ER -

Results from the Anita experiment

Abstract

All Science Journal Classification (ASJC) codes

Access to Document

Other files and links

Fingerprint

Cite this