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The axion arises in well-motivated extensions of the Standard Model of particle physics and is regarded as an alternative to the weakly interacting massive particle paradigm to explain the nature of dark matter. In this contribution, we…

High Energy Physics - Phenomenology · Physics 2018-01-30 Ken'ichi Saikawa

Measurements of 21cm intensity mapping (IM) during the dark ages can potentially provide us with an unprecedented window on high redshifts and small scales. One of the main advantages this can bring involves the possibility to probe the…

Cosmology and Nongalactic Astrophysics · Physics 2024-03-06 Eleonora Vanzan , Alvise Raccanelli , Nicola Bartolo

The quantum chromodynamics axion with a decay constant near the Grand Unification (GUT) scale has an ultralight mass near a neV. We show, however, that axion-like particles with masses near the keV - PeV range with GUT-scale decay constants…

High Energy Physics - Phenomenology · Physics 2023-01-18 Joshua W. Foster , Soubhik Kumar , Benjamin R. Safdi , Yotam Soreq

We derive new constraints on the coupling of heavy pseudoscalar (axion-like) particles to photons, based on the gamma ray flux expected from the decay of these particles into photons. After being produced in the supernova core, these heavy…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Maurizio Giannotti , Leanne D. Duffy , Rafaela Nita

Growing amount of observations indicate presence of intrinsically faint quasar subgroup (a few % of known quasars) with noncosmological quantized redshift. Here we find an analytical solution of Einstein equations describing bubbles made…

Astrophysics · Physics 2007-05-23 Anatoly A. Svidzinsky

Light feebly-coupled bosonic particles can efficiently extract the rotational energy of rapidly spinning black holes on sub-astrophysical timescales via a phenomenon known as black hole superradiance. In the case of light axions, the feeble…

High Energy Physics - Phenomenology · Physics 2025-04-08 Samuel J. Witte , Andrew Mummery

We investigate the degeneracy between the effects of ultra-light axion dark matter and baryonic feedback in suppressing the matter power spectrum. We forecast that galaxy shear data from the Rubin Observatory's Legacy Survey of Space and…

Cosmology and Nongalactic Astrophysics · Physics 2025-10-09 Calvin Preston , Keir K. Rogers , Alexandra Amon , George Efstathiou

A number of proposed and ongoing experiments search for axion dark matter with a mass nearing the limit set by small scale structure (${\cal O} ( 10 ^{ - 21 } {\rm eV} ) $). We consider the late universe cosmology of these models, showing…

High Energy Physics - Phenomenology · Physics 2021-01-11 Jeff A. Dror , Jacob M. Leedom

In the past decade, gamma-ray observations and radio observations put strong constraints on the parameters of dark matter annihilation. In this article, we suggest another robust way to constrain the parameters of dark matter annihilation.…

High Energy Astrophysical Phenomena · Physics 2017-08-09 Man Ho Chan

We report on a search for ultra-low-mass axion-like dark matter by analysing the ratio of the spin-precession frequencies of stored ultracold neutrons and $^{199}$Hg atoms for an axion-induced oscillating electric dipole moment of the…

High Energy Physics - Experiment · Physics 2018-05-28 N. J. Ayres

We consider the production of axion dark matter through the misalignment mechanism in the context of a nonstandard cosmological history involving early matter domination by a scalar field with a time-dependent decay rate. In cases where the…

High Energy Physics - Phenomenology · Physics 2023-05-24 Paola Arias , Nicolás Bernal , Jacek K. Osiński , Leszek Roszkowski

We study the growth of density perturbations in a universe with unstable dark matter particles. The mass (m_\nu) range 30 eV < m_\nu < 10 keV with lifetimes ($t_d$) in the range 10^7 sec < t_d < 10^16 sec are considered. We calculate the…

Astrophysics · Physics 2009-10-30 Somnath Bharadwaj , Shiv K. Sethi

The amount of decaying dark matter, accumulated in the central regions in neutron stars together with the energy deposition rate from decays, may set a limit on the neutron star survival rate against transitions to more compact objects…

Solar and Stellar Astrophysics · Physics 2015-04-09 M. Angeles Perez-Garcia , J. Silk

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

High Energy Physics - Phenomenology · Physics 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya

We investigate the interplay between early universe cosmology and dark matter direct detection, considering axion models with naturally suppressed couplings to photons. In the context of the cosmological relaxation of the electroweak scale,…

High Energy Physics - Phenomenology · Physics 2021-01-26 Nayara Fonseca , Enrico Morgante

We show that a Majorana heavy neutrino with a mass O(100TeV) is a good candidate particle for cold dark matter. It can be responsible for the majority of the cosmological diffuse photon background owing to lifetime of the order of…

High Energy Physics - Phenomenology · Physics 2007-05-23 D. Palle

Constraints on the indirect detection of dark matter are usually obtained from observations of astrophysical objects -- the Galactic Center, dwarf galaxies, M31, etc. Here we propose instead to look for the annihilation or decay of dark…

High Energy Physics - Phenomenology · Physics 2021-10-27 Teresa Marrodán Undagoitia , Werner Rodejohann , Tim Wolf , Carlos E. Yaguna

The subjects of this thesis are the invisible axion and the more general family of axion-like particles. The invisible axion is a hypothetical elementary particle and a cold dark matter candidate. I present an improved computation of the…

Cosmology and Nongalactic Astrophysics · Physics 2011-11-23 Luca Visinelli

We derive a constraint on the cosmic density of string moduli fields in gauge-mediated supersymmetry-breaking theories by requiring that photons emitted from the unstable moduli fields should not exceed the observed X-ray backgrounds. Since…

High Energy Physics - Phenomenology · Physics 2015-06-25 M. Kawasaki , T. Yanagida

Axions currently provide the most compelling solution to the strong CP problem. These particles may be copiously produced in the early universe, including via thermal processes. Therefore, relic axions constitute a hot dark matter component…

Cosmology and Nongalactic Astrophysics · Physics 2015-11-18 Eleonora Di Valentino , Elena Giusarma , Massimiliano Lattanzi , Olga Mena , Alessandro Melchiorri , Joseph Silk
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