Stringent constraint on galactic positron production

被引:169
作者
Beacom, John F. [1 ]
Yuksel, Hasan
机构
[1] Ohio State Univ, Dept Phys, Columbus, OH 43210 USA
[2] Ohio State Univ, Dept Astron, Columbus, OH 43210 USA
基金
美国国家科学基金会;
关键词
D O I
10.1103/PhysRevLett.97.071102
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
The intense 0.511 MeV gamma-ray line emission from the Galactic Center observed by INTEGRAL requires a large annihilation rate of nonrelativistic positrons. If these positrons are injected at even mildly relativistic energies, higher-energy gamma rays will also be produced. We calculate the gamma-ray spectrum due to inflight annihilation and compare it with the observed diffuse Galactic gamma-ray data. Even with a simplified but conservative treatment, we find that the positron injection energies must be less than or similar to 3 MeV, which strongly constrains models for Galactic positron production.
引用
收藏
页数:4
相关论文
共 55 条
[41]   Unstable relics as a source of galactic positrons [J].
Picciotto, C ;
Pospelov, M .
PHYSICS LETTERS B, 2005, 605 (1-2) :15-25
[42]   On the intensity and spatial morphology of the 511 keV emission in the Milky Way [J].
Prantzos, N .
ASTRONOMY & ASTROPHYSICS, 2006, 449 (03) :869-878
[43]   MeV-mass dark matter and primordial nucleosynthesis [J].
Serpico, PD ;
Raffelt, GG .
PHYSICAL REVIEW D, 2004, 70 (04)
[44]  
SIGNORE M, 1988, ASTRON ASTROPHYS, V201, P379
[45]   EQUILIBRIUM SPECTRA OF SECONDARY COSMIC-RAY POSITRONS IN GALAXY AND SPECTRUM OF COSMIC GAMMA-RAYS RESULTING FROM THEIR ANNIHILATION [J].
STECKER, FW .
ASTROPHYSICS AND SPACE SCIENCE, 1969, 3 (04) :579-&
[46]  
STEIGMAN G, 1968, THESIS NEW YORK U
[47]  
STRONG A, COMMUNICATION
[48]  
Strong A. W., 1999, ApLC, V39, P209, DOI DOI 10.48550/ARXIV.ASTRO-PH/9811211
[49]   Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI [J].
Strong, AW ;
Diehl, R ;
Halloin, H ;
Schönfelder, V ;
Bouchet, L ;
Mandrou, P ;
Lebrun, F ;
Terrier, R .
ASTRONOMY & ASTROPHYSICS, 2005, 444 (02) :495-U86
[50]   Propagation of cosmic-ray nucleons in the Galaxy [J].
Strong, AW ;
Moskalenko, IV .
ASTROPHYSICAL JOURNAL, 1998, 509 (01) :212-228