[HTML][HTML] Feebly-interacting particles: FIPs 2022 workshop report

C Antel, M Battaglieri, J Beacham, C Boehm… - The European Physical …, 2023 - Springer
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 …

[HTML][HTML] Feebly-interacting particles: FIPs 2020 workshop report

P Agrawal, M Bauer, J Beacham, A Berlin… - The European Physical …, 2021 - Springer
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 …

The landscape of QCD axion models

L Di Luzio, M Giannotti, E Nardi, L Visinelli - Physics Reports, 2020 - Elsevier
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 …

Black hole superradiance of self-interacting scalar fields

M Baryakhtar, M Galanis, R Lasenby, O Simon - Physical Review D, 2021 - APS
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 …

New experimental approaches in the search for axion-like particles

IG Irastorza, J Redondo - Progress in Particle and Nuclear Physics, 2018 - Elsevier
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 …

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 …

Bosonic dark matter in neutron stars and its effect on gravitational wave signal

D Rafiei Karkevandi, S Shakeri, V Sagun, O Ivanytskyi - Physical Review D, 2022 - APS
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 …

[HTML][HTML] Causal limit of neutron star maximum mass in f (R) gravity in view of GW190814

AV Astashenok, S Capozziello, SD Odintsov… - Physics Letters B, 2021 - Elsevier
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 …

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 …

Stellar recipes for axion hunters

M Giannotti, IG Irastorza, J Redondo… - … of Cosmology and …, 2017 - iopscience.iop.org
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 …