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Related papers: Axion as a cold dark matter candidate: Proof to fu…

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We investigate aspects of axion as a coherently oscillating massive classical scalar field by analyzing third order perturbations in Einstein's gravity in the axion-comoving gauge. The axion fluid has its characteristic pressure term…

General Relativity and Quantum Cosmology · Physics 2015-12-16 Hyerim Noh , Jai-chan Hwang , Chan-Gyung Park

Here we generally prove that the axion as a coherently oscillating scalar field acts as a cold dark matter in nearly all cosmologically relevant scales. The proof is made in the linear perturbation order. Compared with our previous proof…

Cosmology and Nongalactic Astrophysics · Physics 2009-09-28 Jai-chan Hwang , Hyerim Noh

We prove that the axion as a coherently oscillating scalar field acts as a cold dark matter (CDM) to the second-order perturbations in all cosmological scales including the super-horizon scale. The proof is made in the axion-comoving gauge.…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-17 Hyerim Noh , Chan-Gyung Park , Jai-chan Hwang

Axion as a coherently oscillating massive scalar field is known to behave as a zero-pressure irrotational fluid with characteristic quantum stress on a small scale. In relativistic perturbation theory, the case was proved in the…

Cosmology and Nongalactic Astrophysics · Physics 2022-03-09 Jai-chan Hwang , Hyerim Noh

Axion as a coherently oscillating scalar field is known to behave as a cold dark matter in all cosmologically relevant scales. For conventional axion mass with 10^{-5} eV, the axion reveals a characteristic damping behavior in the evolution…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-05 Chan-Gyung Park , Jai-chan Hwang , Hyerim Noh

We derive oscillating gravitational potential caused by an ultralight axion as the cosmic dark matter, assuming the Compton wavelength smaller than the horizon scale. A new oscillatory term is found which dominates the previously known one…

Cosmology and Nongalactic Astrophysics · Physics 2021-12-08 Jai-chan Hwang , Hyerim Noh

We present first-order post-Newtonian (1PN) approximations of a general imperfect fluid and of an axion as a coherently oscillating massive scalar field, both in the cosmological context. For the axion, using the Klein transformation and…

High Energy Physics - Theory · Physics 2023-04-26 Jai-chan Hwang , Hyerim Noh

Axion-like particles (ALPs) are promising dark matter candidates. They are typically described by a classical field, motivated by large phase space occupation numbers. Here we show that such a description is accompanied by a quantum effect:…

Cosmology and Nongalactic Astrophysics · Physics 2022-08-12 Michael Kopp , Vasileios Fragkos , Igor Pikovski

The axion is arguably one of the best motivated candidates for dark matter. For a decay constant greater than about 10^9 GeV, axions are dominantly produced non-thermally in the early universe and hence are "cold", their velocity dispersion…

High Energy Physics - Phenomenology · Physics 2016-12-30 Andreas Ringwald

The axion is a light pseudoscalar particle postulated to solve issues with the Standard Model, including the strong CP problem and the origin of dark matter. In recent years, there has been remarkable progress in the physics of axions in…

High Energy Physics - Phenomenology · Physics 2021-11-03 Kiwoon Choi , Sang Hui Im , Chang Sub Shin

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

The manuscript deals with an interacting scalar field that mimics the evolution of the so-called Axion Scalar Dark Matter or Axion like particles with ultra-light masses. It is discussed that such a scalar alongwith an ordinary fluid…

General Relativity and Quantum Cosmology · Physics 2020-04-02 Soumya Chakrabarti

Recently, two of the present authors showed that even when the axion momentum is much smaller than its mass, the axion can still behave like radiation if its energy density greatly exceeds the maximum potential energy set by the cosine-type…

High Energy Physics - Phenomenology · Physics 2025-09-17 Max Miyazaki , Yuma Narita , Deheng Song , Nemin Yaginuma , Wen Yin

Axions, and axion-like particles, have come back into fashion in the last decades as a possible solution to the galactic-scale crisis suffered by the cold dark matter model. In the framework of the wave Dark Matter model, we have carried…

Astrophysics of Galaxies · Physics 2023-12-13 Ivan De Martino

The axion is a motivated dark matter candidate, so it would be interesting to find features in Large Scale Structures specific to axion dark matter. Such features were proposed for a Bose Einstein condensate of axions, leading to confusion…

High Energy Physics - Phenomenology · Physics 2015-06-19 Sacha Davidson

The axion has emerged in recent years as a leading particle candidate to provide the mysterious dark matter in the cosmos, as we review here for a general scientific audience. We describe first the historical roots of the axion in the…

High Energy Physics - Phenomenology · Physics 2022-10-18 Francesca Chadha-Day , John Ellis , David J. E. Marsh

Axion-like particles are a well-motivated dark matter candidate that can form a condensate with low momentum and high occupation number. In the presence of dark radiation, this condensate loses energy, naturally increasing the energy…

High Energy Physics - Phenomenology · Physics 2024-09-24 Daniel Aloni , Hengameh Bagherian , Rashmish K. Mishra

Axions are among the most sought-after candidates for dark matter. In the ultralight regime, they could help alleviate puzzles in small scale cosmology. Searches for a halo of axion dark matter rely on the electromagnetic response to a…

High Energy Physics - Phenomenology · Physics 2023-12-08 Joshua Berger , Amit Bhoonah

We study cosmological solutions of (pseudo)scalar theories with periodic potentials, in the presence of arbitrary cosmological fluids -- including a cosmological constant of either sign. Independently of the initial misalignment angle and…

Cosmology and Nongalactic Astrophysics · Physics 2026-04-13 Gary Shiu , Flavio Tonioni , Hung V. Tran

The non-linear hydrodynamic equations for axion/scalar field dark matter (DM) in the non-relativistic Madelung-Shcr\"{o}dinger form are derived in a simple manner, including the effects of universal expansion and Hubble drag. The…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-18 David J. E. Marsh
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