[HTML][HTML] Feebly-interacting particles: FIPs 2022 workshop report
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
of matter over anti-matter in the Universe, the origin of the neutrino masses, the apparent …
[HTML][HTML] Feebly-interacting particles: FIPs 2020 workshop report
With the establishment and maturation of the experimental programs searching for new
physics with sizeable couplings at the LHC, there is an increasing interest in the broader …
physics with sizeable couplings at the LHC, there is an increasing interest in the broader …
The landscape of QCD axion models
We review the landscape of QCD axion models. Theoretical constructions that extend the
window for the axion mass and couplings beyond conventional regions are highlighted and …
window for the axion mass and couplings beyond conventional regions are highlighted and …
Black hole superradiance of self-interacting scalar fields
Black hole superradiance is a powerful probe of light, weakly coupled hidden sector
particles. Many candidate particles, such as axions, generically have self-interactions that …
particles. Many candidate particles, such as axions, generically have self-interactions that …
New experimental approaches in the search for axion-like particles
Axions and other very light axion-like particles appear in many extensions of the Standard
Model, and are leading candidates to compose part or all of the missing matter of the …
Model, and are leading candidates to compose part or all of the missing matter of the …
Upper limit on the QCD axion mass from isolated neutron star cooling
M Buschmann, C Dessert, JW Foster, AJ Long… - Physical review …, 2022 - APS
The quantum chromodynamics (QCD) axion may modify the cooling rates of neutron stars
(NSs). The axions are produced within the NS cores from nucleon bremsstrahlung and …
(NSs). The axions are produced within the NS cores from nucleon bremsstrahlung and …
Bosonic dark matter in neutron stars and its effect on gravitational wave signal
We study an impact of self-interacting bosonic dark matter (DM) on various observable
properties of neutron stars (NSs). The analysis is performed for asymmetric DM with masses …
properties of neutron stars (NSs). The analysis is performed for asymmetric DM with masses …
[HTML][HTML] Causal limit of neutron star maximum mass in f (R) gravity in view of GW190814
We investigate the causal limit of maximum mass for stars in the framework of f (R) gravity.
We choose a causal equation of state, with variable speed of sound, and with the transition …
We choose a causal equation of state, with variable speed of sound, and with the transition …
Rp attractors static neutron star phenomenology
VK Oikonomou - Monthly Notices of the Royal Astronomical …, 2023 - academic.oup.com
In this work, we study the neutron star phenomenology of R p attractor theories in the
Einstein frame. The Einstein frame R p attractor theories have the attractor property that they …
Einstein frame. The Einstein frame R p attractor theories have the attractor property that they …
Stellar recipes for axion hunters
There are a number of observational hints from astrophysics which point to the existence of
stellar energy losses beyond the ones accounted for by neutrino emission. These excessive …
stellar energy losses beyond the ones accounted for by neutrino emission. These excessive …