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在能量为1.5 - 100 GeV的宇宙射线中存在异常的正电子丰度。

An anomalous positron abundance in cosmic rays with energies 1.5-100 GeV.

作者信息

Adriani O, Barbarino G C, Bazilevskaya G A, Bellotti R, Boezio M, Bogomolov E A, Bonechi L, Bongi M, Bonvicini V, Bottai S, Bruno A, Cafagna F, Campana D, Carlson P, Casolino M, Castellini G, De Pascale M P, De Rosa G, De Simone N, Di Felice V, Galper A M, Grishantseva L, Hofverberg P, Koldashov S V, Krutkov S Y, Kvashnin A N, Leonov A, Malvezzi V, Marcelli L, Menn W, Mikhailov V V, Mocchiutti E, Orsi S, Osteria G, Papini P, Pearce M, Picozza P, Ricci M, Ricciarini S B, Simon M, Sparvoli R, Spillantini P, Stozhkov Y I, Vacchi A, Vannuccini E, Vasilyev G, Voronov S A, Yurkin Y T, Zampa G, Zampa N, Zverev V G

机构信息

University of Florence, Department of Physics, Via Sansone 1, I-50019 Sesto Fiorentino, Florence, Italy.

出版信息

Nature. 2009 Apr 2;458(7238):607-9. doi: 10.1038/nature07942.

DOI:10.1038/nature07942
PMID:19340076
Abstract

Antiparticles account for a small fraction of cosmic rays and are known to be produced in interactions between cosmic-ray nuclei and atoms in the interstellar medium, which is referred to as a 'secondary source'. Positrons might also originate in objects such as pulsars and microquasars or through dark matter annihilation, which would be 'primary sources'. Previous statistically limited measurements of the ratio of positron and electron fluxes have been interpreted as evidence for a primary source for the positrons, as has an increase in the total electron+positron flux at energies between 300 and 600 GeV (ref. 8). Here we report a measurement of the positron fraction in the energy range 1.5-100 GeV. We find that the positron fraction increases sharply over much of that range, in a way that appears to be completely inconsistent with secondary sources. We therefore conclude that a primary source, be it an astrophysical object or dark matter annihilation, is necessary.

摘要

反粒子在宇宙射线中占比很小,已知它们是在宇宙射线原子核与星际介质中的原子相互作用时产生的,这种相互作用被称为“次级源”。正电子也可能起源于脉冲星和微类星体等天体,或者通过暗物质湮灭产生,这将是“初级源”。先前对正电子与电子通量之比的统计测量有限,这些测量结果被解释为正电子存在初级源的证据,在300至600 GeV能量之间的总电子 + 正电子通量增加也被如此解释(参考文献8)。在此,我们报告了在1.5 - 100 GeV能量范围内对正电子份额的测量。我们发现,在该范围的大部分区域,正电子份额急剧增加,其方式似乎与次级源完全不一致。因此,我们得出结论,必须存在一个初级源,无论是天体物理对象还是暗物质湮灭。

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2
BAYESIAN ANALYSIS OF COSMIC RAY PROPAGATION: EVIDENCE AGAINST HOMOGENEOUS DIFFUSION.宇宙射线传播的贝叶斯分析:反对均匀扩散的证据
Astrophys J. 2016 Jun 10;824(1). doi: 10.3847/0004-637x/824/1/16. Epub 2016 Jun 3.
3
Cosmic Rays in the Milky Way and Beyond.银河系及其他星系中的宇宙射线。

本文引用的文献

1
TeV gamma rays from Geminga and the origin of the GeV positron excess.来自 Geminga 的 TeV 伽马射线与 GeV 正电子过量的起源
Phys Rev Lett. 2009 Jul 31;103(5):051101. doi: 10.1103/PhysRevLett.103.051101. Epub 2009 Jul 27.
2
Constraints on WIMP dark matter from the high energy PAMELA p/p data.来自高能帕梅拉质子/反质子数据对弱相互作用大质量粒子暗物质的限制。
Phys Rev Lett. 2009 Feb 20;102(7):071301. doi: 10.1103/PhysRevLett.102.071301.
3
New measurement of the antiproton-to-proton flux ratio up to 100 GeV in the cosmic radiation.
Nucl Phys B Proc Suppl. 2013 Oct;243:85-91. doi: 10.1016/j.nuclphysbps.2013.09.014. Epub 2013 Nov 4.
4
Cosmic-Ray Propagation in Light of the Recent Observation of Geminga.基于近期对Geminga的观测的宇宙射线传播
Astrophys J. 2019 Jul 10;879(2). doi: 10.3847/1538-4357/ab258e.
5
HelMod in the Works: From Direct Observations to the Local Interstellar Spectrum of Cosmic-Ray Electrons.正在研究中的HelMod:从直接观测到宇宙射线电子的本地星际光谱。
Astrophys J. 2018 Feb 20;854(2). doi: 10.3847/1538-4357/aaa75e. Epub 2018 Feb 15.
6
NEW CALCULATION OF ANTIPROTON PRODUCTION BY COSMIC RAY PROTONS AND NUCLEI.宇宙射线质子和原子核产生反质子的新计算
Astrophys J. 2015 Apr 20;803(2). doi: 10.1088/0004-637x/803/2/54. Epub 2015 Apr 14.
7
Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons.直接探测到太电子伏特能区电子和正电子宇宙射线能谱的断裂。
Nature. 2017 Dec 7;552(7683):63-66. doi: 10.1038/nature24475. Epub 2017 Nov 29.
8
Radiation Measurements Performed with Active Detectors Relevant for Human Space Exploration.使用与人类太空探索相关的有源探测器进行的辐射测量。
Front Oncol. 2015 Dec 8;5:273. doi: 10.3389/fonc.2015.00273. eCollection 2015.
9
Advances in antihydrogen physics.反氢物理的进展。
Sci Prog. 2015;98(Pt 1):34-62. doi: 10.3184/003685015X14234978376369.
10
Indirect detection of dark matter with γ rays.利用伽马射线间接探测暗物质。
Proc Natl Acad Sci U S A. 2015 Oct 6;112(40):12264-71. doi: 10.1073/pnas.1308728111. Epub 2014 May 12.
Phys Rev Lett. 2009 Feb 6;102(5):051101. doi: 10.1103/PhysRevLett.102.051101. Epub 2009 Feb 2.
4
An excess of cosmic ray electrons at energies of 300-800 GeV.能量在300 - 800 GeV之间的宇宙射线电子过量。
Nature. 2008 Nov 20;456(7220):362-5. doi: 10.1038/nature07477.
5
New measurement of the cosmic-ray positron fraction from 5 to 15 GeV.5至15GeV宇宙射线正电子分数的新测量。
Phys Rev Lett. 2004 Dec 10;93(24):241102. doi: 10.1103/PhysRevLett.93.241102. Epub 2004 Dec 9.
6
Kaluza-Klein dark matter.
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7
Electrons and positrons in the galactic cosmic rays.银河系宇宙射线中的电子和正电子。
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