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The observed galactic 511 keV line has been interpreted in a number of papers as a possible signal of dark matter annihilation within the galactic bulge. If this is the case then we should expect a similar spectral feature associated with…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-08 Kyle Lawson , Ariel Zhitnitsky

We discuss the possibility that the recent detection of 511 keV gamma-rays from the galactic bulge, as observed by INTEGRAL, is a consequence of low mass (~MeV) particle dark matter annihilations. We discuss the type of halo profile favored…

Astrophysics · Physics 2009-11-10 Celine Boehm , Dan Hooper , Joseph Silk , Michel Casse

We show that a tangle of light superconducting strings in the Milky Way could be the source of the observed 511 KeV emission from electron-positron annihilation in the Galactic bulge. The scenario predicts a flux that is in agreement with…

Astrophysics · Physics 2007-05-23 Francesc Ferrer , Tanmay Vachaspati

It has recently been pointed out that the 511 keV emission line detected by Integral/SPI from the bulge of our galaxy could be explained by annihilations of light Dark Matter particles into e^+ e^-. If such a signature is confirmed, then…

High Energy Physics - Phenomenology · Physics 2009-02-20 C. Boehm , P. Fayet , J. Silk

We propose that a dark matter (DM) spike around the Galactic Center's (GC) supermassive black hole, Sgr A*, could account for most of the bulge's measured 511 keV line intensity while remaining cosmologically compatible. DM annihilation can…

High Energy Astrophysical Phenomena · Physics 2025-09-08 Pedro De la Torre Luque , Shyam Balaji , Malcolm Fairbairn , Filippo Sala , Joseph Silk

Observations of the Milky Way by the SPI/INTEGRAL satellite have confirmed the presence of a strong 511 KeV gamma-ray line emission from the bulge, which require an intense source of positrons in the galactic center. These observations are…

Astrophysics · Physics 2008-11-26 Francesc Ferrer , Tanmay Vachaspati

Gamma ray emission of 511 keV lines arising from electron-positron annihilation has been detected from the Galaxy since the 70s. Spatially resolved observations using the INTEGRAL satellite have shown its full sky distribution to be…

High Energy Astrophysical Phenomena · Physics 2014-07-11 Hagai B. Perets

We present a possible explanation of the recently observed 511 keV $\gamma$-ray anomaly with a new ``millicharged'' fermion. The new fermion is light (${\cal O}({\rm MeV})$) but has never been observed by any collider experiments mainly…

Astrophysics · Physics 2008-11-26 Ji-Haeng Huh , Jihn E. Kim , Jong-Chul Park , Seong Chan Park

A number of signals involving charged cosmic rays and high-energy photons have been interpreted as being due to annihilating dark matter. This article provides an overview of the experimental evidence and discusses in particular detections…

Astrophysics · Physics 2007-05-23 U. Schwanke

Several independent observations of the galactic core suggest hitherto unexplained sources of energy. The most well known case is the 511 keV line which has proven very difficult to explain with conventional astrophysical positron sources.…

Astrophysics · Physics 2009-06-23 Kyle Lawson , Ariel R. Zhitnitsky

We propose a possible explanation for the recently observed anomalous 511 keV line with a new "millicharged" fermion. This new fermion is light [${\cal O}({\rm MeV})$]. Nevertheless, it has never been observed by any collider experiments by…

High Energy Physics - Phenomenology · Physics 2009-02-02 Ji-Haeng Huh , Jihn E. Kim , Jong-Chul Park , Seong Chan Park

The first gamma-ray line originating from outside the solar system that was ever detected is the 511 keV emission from positron annihilation in the Galaxy. Despite 30 years of intense theoretical and observational investigation, the main…

High Energy Astrophysical Phenomena · Physics 2015-05-20 N. Prantzos , C. Boehm , A. M. Bykov , R. Diehl , K. Ferriere , N. Guessoum , P. Jean , J. Knoedlseder , A. Marcowith , I. V. Moskalenko , A. Strong , G. Weidenspointner

I describe a novel dark matter candidate in which the dark matter is composed of macroscopically large "nuggets" of ordinary quarks and antiquarks in a colour-superconducting phase. The physical properties of these objects are described…

High Energy Astrophysical Phenomena · Physics 2009-06-03 K. Lawson

If annihilating MeV-scale dark matter particles are responsible for the observed 511 keV emission from the Galactic bulge, then new light gauge bosons which mediate the dark matter annihilations may have other observable consequences. In…

High Energy Physics - Phenomenology · Physics 2008-11-26 Dan Hooper

The SPI spectrometer aboard of the INTEGRAL satellite has released a map of the e+e- annihilation emission line of unprecedented quality, showing that most of the photons arise from a region coinciding with the stellar bulge of the Milky…

Astrophysics · Physics 2009-11-11 Michel Casse , Pierre Fayet

An excess of 511 keV photons has been detected from the central region of the Milky Way. It has been suggested that the positrons responsible for this signal could be produced through the Hawking evaporation of primordial black holes. After…

Cosmology and Nongalactic Astrophysics · Physics 2022-04-11 Celeste Keith , Dan Hooper

The bulk of the extragalactic background between 10 keV and 10 GeV is likely to be explained by the emission of Seyfert galaxies, type Ia supernovae, and blazars. However, as revealed by the INTEGRAL satellite, the bulge of our galaxy is an…

It has been recently proposed that the observed 511 keV emission from the Galactic bulge could be the product of very light (1-100 MeV) annihilating dark matter particles. Other possible explanations for this signal are associated with…

It has been suggested ``that DM particles are strongly interacting composite macroscopically large objects ... made of well known light quarks (or ... antiquarks)." In doing so it is argued that these compact composite objects (CCOs) are…

Astrophysics · Physics 2008-11-26 Daniel T. Cumberbatch , Glenn D. Starkman , Joseph Silk

The origin of both the diffuse high-latitude MeV gamma-ray emission and the 511 keV line flux from the Galactic bulge are uncertain. Previous studies have invoked dark matter physics to independently explain these observations, though as…

Astrophysics · Physics 2008-11-26 Jose A. R. Cembranos , Louis E. Strigari
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