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Dark matter (DM) refers to a new type of matter that may explain observed rotation curves of galaxies and the composite structure of the Universe. It may couple to the Standard Model particles via portals, which include the possibility of…

High Energy Physics - Experiment · Physics 2023-11-30 Vindhyawasini Prasad

An appealing framework for dark matter is provided by light hidden sectors, below the electroweak scale, feebly coupled to the Standard Model via light mediators. We consider a minimal, predictive model where both the dark matter and the…

High Energy Physics - Phenomenology · Physics 2025-10-31 Ana Luisa Foguel , Renata Zukanovich Funchal , Michele Frigerio

Long-standing efforts to detect axions are driven by two compelling prospects, naturally accounting for the absence of charge-conjugation and parity symmetry breaking in quantum chromodynamics, and for the elusive dark matter at ultralight…

High Energy Physics - Phenomenology · Physics 2023-07-19 Georg Engelhardt , Amit Bhoonah , W. Vincent Liu

The Standard Model Lagrangian has an approximate scale symmetry in the high-energy limit. This observation can be included in the fundamental principle of the ultimate theory of Nature as the requirement of the exact quantum scale…

High Energy Physics - Phenomenology · Physics 2023-06-21 Aleksandr I. Belokon , Anna Tokareva

While, to ensure successful cosmology, dark matter (DM) must kinematically decouple from the standard model plasma very early in the history of the Universe, it can remain coupled to a bath of "dark radiation" until a relatively late epoch.…

Cosmology and Nongalactic Astrophysics · Physics 2013-06-05 Francis-Yan Cyr-Racine , Kris Sigurdson

We study phenomenological implications of an axion that arises as a pseudo Nambu-Goldstone boson due to the spontaneous breaking of anomaly-free global flavor symmetry. One interesting possibility for such anomaly-free axion to explain dark…

High Energy Physics - Phenomenology · Physics 2022-08-10 Kodai Sakurai , Fuminobu Takahashi

The QCD axion was originally predicted as a dynamical solution to the strong CP problem. Axion like particles (ALPs) are also a generic prediction of many high energy physics models including string theory. Theoretical models for axions are…

High Energy Physics - Phenomenology · Physics 2017-12-11 David J. E. Marsh

The asymmetric dark matter (ADM) scenario solves the baryon-dark matter coincidence problem when the dark matter (DM) mass is of $\mathcal{O}(1)$GeV. Composite ADM models based on QCD-like strong dynamics are particularly motivated since…

High Energy Physics - Phenomenology · Physics 2021-08-18 Masahiro Ibe , Shin Kobayashi , Keiichi Watanabe

We study the thermal freeze-out of a dark photon dark matter in the so-called dark-axion portal - a triple coupling among a dark photon, an axion-like particle and the SM $\gamma$ or $Z$ boson. We analyze in detail the thermal production…

High Energy Physics - Phenomenology · Physics 2025-02-18 Bastián Díaz Sáez

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

The recent detection of B-modes by BICEP2 has non-trivial implications for axion dark matter implied by combining the tensor interpretation with isocurvature constraints from Planck. In this paper the measurement is taken as fact, and its…

Cosmology and Nongalactic Astrophysics · Physics 2014-07-09 David J. E. Marsh , Daniel Grin , Renee Hlozek , Pedro G. Ferreira

We study QCD axion or cosmological axion-like particles (ALPs) in a model inspired by the recent interest in 4-dimensional clockwork models, with the global symmetry being accidentally enforced by a gauge abelian quiver with scalar…

High Energy Physics - Phenomenology · Physics 2019-01-21 Quentin Bonnefoy , Emilian Dudas , Stefan Pokorski

A kinetic mixing between the axion and the inflaton allows for a production of axion dark matter even if the inflationary Hubble scale is smaller than the zero-temperature axion mass. We analyze the axion dynamics in this recently…

High Energy Physics - Phenomenology · Physics 2020-09-10 Takeshi Kobayashi , Lorenzo Ubaldi

In this master's thesis we study the production of axion dark matter through the so-called misalignment mechanism by considering that during that time, the universe was dominated by a new kind of fluid, different than radiation. We perform…

High Energy Physics - Phenomenology · Physics 2021-06-16 Moira Venegas

The cold dark matter (CDM) paradigm provides a remarkably good description of the Universe's large-scale structure. However, some discrepancies exist between its predictions and observations at very small sub-galactic scales. To address…

Cosmology and Nongalactic Astrophysics · Physics 2024-01-04 Atrideb Chatterjee , Sourav Mitra , Amrita Banerjee

The eXciting Dark Matter (XDM) model was proposed as a mechanism to efficiently convert the kinetic energy (in sufficiently hot environments) of dark matter into e+e- pairs. The standard scenario invokes a doublet of nearly degenerate DM…

High Energy Physics - Phenomenology · Physics 2016-10-12 Douglas P. Finkbeiner , Neal Weiner

We investigate a cosmological model in which a fraction of the dark matter is atomic dark matter (ADM). This ADM consists of dark versions of the electron and of the proton, interacting with each other and with dark photons just as their…

Cosmology and Nongalactic Astrophysics · Physics 2024-05-14 Ellie Hughes , Fei Ge , Francis-Yan Cyr-Racine , Lloyd Knox , Srinivasan Raghunathan

The search for axions has gained ground in recent years, with laboratory searches for cold dark matter (CDM) axions, relativistic solar axions and ultra-light axions the subject of extensive literature. In particular, the interest in axions…

Cosmology and Nongalactic Astrophysics · Physics 2017-08-07 Katharine Kelley , P. J. Quinn

The QCD axion is a good dark matter candidate. The observed dark matter abundance can arise from misalignment or defect mechanisms, which generically require an axion decay constant $f_a \sim \mathcal{O}(10^{11})$ GeV (or higher). We…

High Energy Physics - Phenomenology · Physics 2018-07-27 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

In an axiverse with numerous axions, the cosmological moduli problem poses a significant challenge because the abundance of axions can easily exceed that of dark matter. The well-established stochastic axion scenario offers a simple…

High Energy Physics - Phenomenology · Physics 2023-09-06 Kai Murai , Fuminobu Takahashi , Wen Yin
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