Search for Antideuterons of Cosmic Origin Using the BESS-Polar II Magnetic-Rigidity Spectrometer.


Journal

Physical review letters
ISSN: 1079-7114
Titre abrégé: Phys Rev Lett
Pays: United States
ID NLM: 0401141

Informations de publication

Date de publication:
29 Mar 2024
Historique:
received: 21 05 2023
revised: 21 10 2023
accepted: 10 01 2024
medline: 13 4 2024
pubmed: 13 4 2024
entrez: 13 4 2024
Statut: ppublish

Résumé

We searched for antideuterons (d[over ¯]'s) in the 4.7×10^{9} cosmic-ray events observed during the BESS-Polar II flight at solar minimum in 2007-2008 but found no candidates. The resulting 95% C.L. upper limit on the d[over ¯] flux is 6.7×10^{-5}  (m^{2} s sr GeV/n)^{-1} in an energy range from 0.163 to 1.100  GeV/n. The result has improved by more than a factor of 14 from the upper limit of BESS97, which had a potential comparable to that of BESS-Polar II in the search for cosmic-origin d[over ¯]'s and was conducted during the former solar minimum. The upper limit of d[over ¯] flux from BESS-Polar II is the first result achieving the sensitivity to constrain the latest theoretical predictions.

Identifiants

pubmed: 38613296
doi: 10.1103/PhysRevLett.132.131001
doi:

Types de publication

Journal Article

Langues

eng

Sous-ensembles de citation

IM

Pagination

131001

Auteurs

K Sakai (K)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.
Center for Research and Exploration in Space Science and Technology (CRESST).

H Fuke (H)

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210, Japan.

K Yoshimura (K)

Okayama University, Okayama, Okayama 700-8530, Japan.

M Sasaki (M)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.
Center for Research and Exploration in Space Science and Technology (CRESST).

K Abe (K)

Kobe University, Kobe, Hyogo 657-8501, Japan.

S Haino (S)

High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.

T Hams (T)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.
Center for Research and Exploration in Space Science and Technology (CRESST).

M Hasegawa (M)

High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.

K C Kim (KC)

IPST, University of Maryland, College Park, Maryland 20742, USA.

M H Lee (MH)

IPST, University of Maryland, College Park, Maryland 20742, USA.

Y Makida (Y)

High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.

J W Mitchell (JW)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.

J Nishimura (J)

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210, Japan.
The University of Tokyo, Bunkyo, Tokyo 113-0033, Japan.

M Nozaki (M)

High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.

R Orito (R)

Kobe University, Kobe, Hyogo 657-8501, Japan.

J F Ormes (JF)

University of Denver, Denver, Colorado 80208, USA.

E S Seo (ES)

IPST, University of Maryland, College Park, Maryland 20742, USA.

R E Streitmatter (RE)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.

N Thakur (N)

NASA-Goddard Space Flight Center (NASA-GSFC), Greenbelt, Maryland 20771, USA.

A Yamamoto (A)

High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan.

T Yoshida (T)

Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara, Kanagawa 252-5210, Japan.

Classifications MeSH