Dark matter in compact stars
J Bramante, N Raj - Physics Reports, 2024 - Elsevier
WDs and neutron stars are far-reaching and multi-faceted laboratories in the hunt for dark
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …
matter. We review detection prospects of wave-like, particulate, macroscopic and black hole …
Dark matter effects on the properties of neutron stars: Compactness and tidal deformability
We systematically study the observable properties of dark-matter admixed neutron stars with
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …
arbitrary dark-matter fraction, employing a realistic nuclear equation of state in combination …
Bosonic dark matter in light of the NICER precise mass-radius measurements
S Shakeri, DR Karkevandi - Physical Review D, 2024 - APS
We explore the presence of self-interacting bosonic dark matter (DM) within neutron stars
(NSs) in light of the latest multimessenger observations of the Neutron Star Interior …
(NSs) in light of the latest multimessenger observations of the Neutron Star Interior …
Effects from dark matter halos on x-ray pulsar pulse profiles
Y Liu, HB Li, Y Gao, L Shao, Z Hu - Physical Review D, 2024 - APS
Neutron stars (NSs) can capture dark matter (DM) particles because of their deep
gravitational potential and high density. The accumulated DM can affect the properties of …
gravitational potential and high density. The accumulated DM can affect the properties of …
Indirect Searches for Dark Photon-Photon Tridents in Celestial Objects
T Linden, TTQ Nguyen, TMP Tait - arXiv preprint arXiv:2402.01839, 2024 - arxiv.org
We model and constrain the unique indirect detection signature produced by dark matter
particles that annihilate through a $ U (1) $ gauge symmetry into dark photons that …
particles that annihilate through a $ U (1) $ gauge symmetry into dark photons that …
Exploring the Distribution and Impact of Bosonic Dark Matter in Neutron Stars
D Rafiei Karkevandi, M Shahrbaf, S Shakeri, S Typel - Particles, 2024 - mdpi.com
The presence of dark matter (DM) within neutron stars (NSs) can be introduced by different
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …
Beyond Hawking evaporation of black holes formed by dark matter in compact stars
The memory burden effect is an explicit resolution to the information paradox by which an
evaporating black hole acquires quantum hair, which then suppresses its rate of mass loss …
evaporating black hole acquires quantum hair, which then suppresses its rate of mass loss …
Exploring the distribution and impact of bosonic dark matter in neutron stars
DR Karkevandi, M Shahrbaf, S Shakeri… - arXiv preprint arXiv …, 2024 - arxiv.org
The presence of dark matter (DM) within neutron stars (NSs) can be introduced by different
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …
[PDF][PDF] Exploring the Distribution and Impact of Bosonic Dark Matter in Neutron Stars. Particles 2024, 7, 201–213
D Rafiei Karkevandi, M Shahrbaf, S Shakeri, S Typel - 2024 - researchgate.net
The presence of dark matter (DM) within neutron stars (NSs) can be introduced by different
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …
accumulation scenarios in which DM and baryonic matter (BM) may interact only through the …