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A New Limit on the Flux of Cosmic Antihelium

A very sensitive search for cosmic-ray antihelium was performed using data obtained from three scientific flights of BESS magnetic rigidity spectrometer. We have not observed any antihelium; this places a model-independent upper limit (95 % C.L.) on the antihelium flux of 6*10**(-4) m**(-2)sr**(-1)s...

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Detalles Bibliográficos
Autores principales: Saeki, T, Anraku, K, Orito, S, Ormes, J F, Imori, M, Kimbell, B L, Makida, Y, Matsumoto, H, Matsunaga, H, Mitchell, J, Motoki, M, Nishimura, J, Nozaki, M, Otoba, M, Sanuki, T, Streitmatter, R E, Suzuki, J, Tanaka, K, Ueda, I, Yajima, N, Yamagami, T, Yamamoto, A, Yoshida, T, Yoshimura, K
Lenguaje:eng
Publicado: 1998
Materias:
Acceso en línea:https://dx.doi.org/10.1016/S0370-2693(98)00131-2
http://cds.cern.ch/record/336649
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author Saeki, T
Anraku, K
Orito, S
Ormes, J F
Imori, M
Kimbell, B L
Makida, Y
Matsumoto, H
Matsunaga, H
Mitchell, J
Motoki, M
Nishimura, J
Nozaki, M
Otoba, M
Sanuki, T
Streitmatter, R E
Suzuki, J
Tanaka, K
Ueda, I
Yajima, N
Yamagami, T
Yamamoto, A
Yoshida, T
Yoshimura, K
author_facet Saeki, T
Anraku, K
Orito, S
Ormes, J F
Imori, M
Kimbell, B L
Makida, Y
Matsumoto, H
Matsunaga, H
Mitchell, J
Motoki, M
Nishimura, J
Nozaki, M
Otoba, M
Sanuki, T
Streitmatter, R E
Suzuki, J
Tanaka, K
Ueda, I
Yajima, N
Yamagami, T
Yamamoto, A
Yoshida, T
Yoshimura, K
author_sort Saeki, T
collection CERN
description A very sensitive search for cosmic-ray antihelium was performed using data obtained from three scientific flights of BESS magnetic rigidity spectrometer. We have not observed any antihelium; this places a model-independent upper limit (95 % C.L.) on the antihelium flux of 6*10**(-4) m**(-2)sr**(-1)s**(-1) at the top of the atmosphere in the rigidity region 1 to 16 GV, after correcting for the estimated interaction loss of antihelium in the air and in the instrument. The corresponding upper limit on the Hebar/He flux ratio is 3.1*10**(-6), 30 times more stringent than the limits obtained in similar rigidity regions with magnetic spectrometers previous to BESS.
id cern-336649
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 1998
record_format invenio
spelling cern-3366492019-09-30T06:29:59Zdoi:10.1016/S0370-2693(98)00131-2http://cds.cern.ch/record/336649engSaeki, TAnraku, KOrito, SOrmes, J FImori, MKimbell, B LMakida, YMatsumoto, HMatsunaga, HMitchell, JMotoki, MNishimura, JNozaki, MOtoba, MSanuki, TStreitmatter, R ESuzuki, JTanaka, KUeda, IYajima, NYamagami, TYamamoto, AYoshida, TYoshimura, KA New Limit on the Flux of Cosmic AntiheliumAstrophysics and AstronomyA very sensitive search for cosmic-ray antihelium was performed using data obtained from three scientific flights of BESS magnetic rigidity spectrometer. We have not observed any antihelium; this places a model-independent upper limit (95 % C.L.) on the antihelium flux of 6*10**(-4) m**(-2)sr**(-1)s**(-1) at the top of the atmosphere in the rigidity region 1 to 16 GV, after correcting for the estimated interaction loss of antihelium in the air and in the instrument. The corresponding upper limit on the Hebar/He flux ratio is 3.1*10**(-6), 30 times more stringent than the limits obtained in similar rigidity regions with magnetic spectrometers previous to BESS.astro-ph/9710228oai:cds.cern.ch:3366491998
spellingShingle Astrophysics and Astronomy
Saeki, T
Anraku, K
Orito, S
Ormes, J F
Imori, M
Kimbell, B L
Makida, Y
Matsumoto, H
Matsunaga, H
Mitchell, J
Motoki, M
Nishimura, J
Nozaki, M
Otoba, M
Sanuki, T
Streitmatter, R E
Suzuki, J
Tanaka, K
Ueda, I
Yajima, N
Yamagami, T
Yamamoto, A
Yoshida, T
Yoshimura, K
A New Limit on the Flux of Cosmic Antihelium
title A New Limit on the Flux of Cosmic Antihelium
title_full A New Limit on the Flux of Cosmic Antihelium
title_fullStr A New Limit on the Flux of Cosmic Antihelium
title_full_unstemmed A New Limit on the Flux of Cosmic Antihelium
title_short A New Limit on the Flux of Cosmic Antihelium
title_sort new limit on the flux of cosmic antihelium
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1016/S0370-2693(98)00131-2
http://cds.cern.ch/record/336649
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