Search Publications

Restrictions on parameters of sterile neutrino dark matter from observations of galaxy clusters
DOI: 10.1103/PhysRevD.74.103506 Bibcode: 2006PhRvD..74j3506B

Neronov, A.; Boyarsky, A.; Ruchayskiy, O. +1 more

We find restrictions on the mass and mixing angle of the dark matter sterile neutrinos using x-ray observations of Coma and Virgo galaxy clusters with XMM-Newton satellite. In the absence of clearly detectable line, we present detailed analysis of various methods of putting restrictions on mass and mixing angle of sterile neutrino. Our analysis pr…

2006 Physical Review D
XMM-Newton 128
Continuum γ-ray emission from light dark matter positrons and electrons
DOI: 10.1103/PhysRevD.74.063514 Bibcode: 2006PhRvD..74f3514S

Schanne, S.; Sizun, P.; Cassé, M.

The annihilation of light dark matter was recently advocated as a possible explanation of the large positron injection rate at the Galactic center deduced from observations by the SPI spectrometer aboard INTEGRAL. The modelling of internal Bremsstrahlung and in-flight annihilation radiations associated to this process drastically reduced the mass …

2006 Physical Review D
INTEGRAL 80
Constraint on the post-Newtonian parameter γ on galactic size scales
DOI: 10.1103/PhysRevD.74.061501 Bibcode: 2006PhRvD..74f1501B

Bolton, Adam S.; Burles, Scott; Rappaport, Saul

We constrain the post-Newtonian gravity parameter γ on kiloparsec scales by comparing the masses of 15 elliptical lensing galaxies from the Sloan Lens ACS Survey as determined in two independent ways. The first method assumes only that Newtonian gravity is correct and is independent of γ, while the second uses gravitational lensing which depends o…

2006 Physical Review D
eHST 61
Soft gamma-ray background and light dark matter annihilation
DOI: 10.1103/PhysRevD.73.103518 Bibcode: 2006PhRvD..73j3518R

Fayet, Pierre; Cordier, Bertrand; Teyssier, Romain +4 more

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 intense source of a 511 keV gamma-ray line, indicating the production of a large number of positrons that an…

2006 Physical Review D
INTEGRAL 39
Hubble imaging excludes cosmic string lens
DOI: 10.1103/PhysRevD.73.087302 Bibcode: 2006PhRvD..73h7302A

Hogan, Craig J.; Agol, Eric; Plotkin, Richard M.

The galaxy image pair Capodimonte-Sternberg-Lens Candidate no. 1 (CSL-1) has been a leading candidate for a cosmic string lens. High quality imaging data from the Hubble Space Telescope presented here show that it is not a lens but a pair of galaxies. The galaxies show different orientations of their principal axes, not consistent with any lens mo…

2006 Physical Review D
eHST 21