Results 31 to 40 of about 1,645,326 (221)
Soft scattering evaporation of dark matter subhalos by inner galactic gases
The large gap between a galactic dark matter subhalo’s velocity and its own gravitational binding velocity creates the situation that small subhalos can be evaporated before dark matter thermalize with baryons due to the low binding velocity.
Xiao-jun Bi+4 more
doaj +1 more source
PLE$\nu$M: A global and distributed monitoring system of high-energy astrophysical neutrinos [PDF]
High-energy astrophysical neutrinos, discovered by IceCube, are now regularly observed, albeit at a low rate due to their low flux. As a result, open questions about high-energy neutrino astrophysics and particle physics remain limited by statistics at ...
L. Schumacher+5 more
semanticscholar +1 more source
Phase transitions and geothermodynamics of black holes in dRGT massive gravity
In this paper, we study the thermodynamics and geothermodynamics of spherical black hole solutions in dRGT massive gravity in a new extended phase space. Inspire by the work of Kastor et al.
M. Chabab+3 more
doaj +1 more source
Trinity: an imaging air Cherenkov telescope to search for Ultra-High-Energy neutrinos. [PDF]
Centre for Advanced Instrumentation, Durham University, South Road, Durham, DH1 3LE, UK Georgia Institute of Technology, School of Physics & Center for Relativistic Astrophysics, 837 State Street NW, Atlanta, Georgia 30332-0430, USA Università di Padova (
Anthony M. Brown+9 more
semanticscholar +1 more source
High-energy astrophysics and cosmology [PDF]
12 pages, 16 eps figures, uses espcrc2.sty. Talk presented at the XIIth International Symposium on Very-High-Energy Cosmic-Ray Interactions, CERN, July ...
openaire +4 more sources
Supergalactic Structure of Multiplets with the Telescope Array Surface Detector [PDF]
Evidence of supergalactic structure of multiplets has been found for ultra-high energy cosmic rays (UHECR) with energies above 1019 eV using 7 years of data from the Telescope Array (TA) surface detector.
Lundquist Jon Paul, Sokolsky Pierre V.
doaj +1 more source
DAMA/LIBRA-phase1 results and perspectives of the phase2
The results obtained with the total exposure of 1.04 ton × yr collected by DAMA/LIBRA–phase1 deep underground at the Gran Sasso National Laboratory (LNGS) of the I.N.F.N. during 7 annual cycles are summarized.
Bernabei R.+16 more
doaj +2 more sources
NUCLEAR AND HIGH-ENERGY ASTROPHYSICS [PDF]
52 pages, 43 figures; to appear in the Proceedings of the VIII International Workshop on Hadron Physics, April 14-19, 2002, Rio Grande do Sul ...
openaire +4 more sources
Viscous attenuation of gravitational waves propagating through an inhomogeneous background
We consider the propagation of gravitational waves in the late-time Universe in the presence of matter distribution inhomogeneities, and we also consider the cosmic fluid to be viscous.
Shashank Shekhar Pandey+3 more
doaj +1 more source
High energy neutrino astrophysics [PDF]
Astroparticle physics is a field rich of perspectives in investigating the ultra-high energy region which will never be accessible to man made machines. Many efforts are underway in order to detect the first cosmic neutrinos, messengers of the unobserved universe.
openaire +3 more sources