Search Publications

Neutrino and Positron Constraints on Spinning Primordial Black Hole Dark Matter
DOI: 10.1103/PhysRevLett.125.101101 Bibcode: 2020PhRvL.125j1101D

Ray, Anupam; Laha, Ranjan; Dasgupta, Basudeb

Primordial black holes can have substantial spin—a fundamental property that has a strong effect on its evaporation rate. We conduct a comprehensive study of the detectability of primordial black holes with non-negligible spin, via the searches for the neutrinos and positrons in the MeV energy range. Diffuse supernova neutrino background searches …

2020 Physical Review Letters
INTEGRAL 190
Sign of Hard-X-Ray Pulsation from the γ -Ray Binary System LS 5039
DOI: 10.1103/PhysRevLett.125.111103 Bibcode: 2020PhRvL.125k1103Y

Takahashi, T.; Enoto, T.; Makishima, K. +3 more

To understand the nature of the brightest γ -ray binary system LS 5039, hard x-ray data of the object, taken with the Suzaku and NuSTAR observatories in 2007 and 2016, respectively, were analyzed. The two data sets jointly gave tentative evidence for a hard x-ray periodicity, with a period of ∼9 s and a period increase rate by ∼3 ×10-10

2020 Physical Review Letters
Suzaku 41
First Results on Dark Matter Substructure from Astrometric Weak Lensing
DOI: 10.1103/PhysRevLett.125.111101 Bibcode: 2020PhRvL.125k1101M

Van Tilburg, Ken; Weiner, Neal; Taki, Anna-Maria +1 more

Low-mass structures of dark matter (DM) are expected to be entirely devoid of light-emitting regions and baryons. Precisely because of this lack of baryonic feedback, small-scale substructures of the Milky Way are a relatively pristine testing ground for discovering aspects of DM microphysics and primordial fluctuations on subgalactic scales. In t…

2020 Physical Review Letters
Gaia 33
Joining Bits and Pieces of Reionization History
DOI: 10.1103/PhysRevLett.125.071301 Bibcode: 2020PhRvL.125g1301H

Finelli, Fabio; Paoletti, Daniela; Hazra, Dhiraj Kumar +1 more

Cosmic microwave background (CMB) temperature and polarization anisotropies from Planck have estimated a lower value of the optical depth to reionization (τ ) compared to WMAP. A significant period in the reionization history would then fall within 6 <redshift(z )<10 , where detection of galaxies with Hubble frontier fields program and indep…

2020 Physical Review Letters
eHST 17