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Related papers: Axion as a CDM component

200 papers

We present a detailed study of cosmological effects of homogeneous tachyon matter coexisting with non-relativistic matter and radiation, concentrating on the inverse square potential and the exponential potential for the tachyonic scalar…

Astrophysics · Physics 2011-05-05 J. S. Bagla , H. K. Jassal , T. Padmanabhan

The properties of axions that constitute 100% of cold dark matter (CDM) depend on the tensor-to-scalar ratio $r$ at the end of inflation. If $r=0.20^{+0.07}_{-0.05}$ as reported by the BICEP2 collaboration, then "half" of the CDM axion…

High Energy Physics - Phenomenology · Physics 2014-07-09 L. Visinelli , P. Gondolo

The axion particle is the outcome of the proposed Peccei-Quinn mechanism for solving the strong CP problem. Axion is also a popular dark matter candidate. Thus there is an increased interest in establishing its existence. Axions couple to…

High Energy Physics - Phenomenology · Physics 2022-04-06 A. Nicolaidis

Cosmology and particle physics are closer today than ever before, with several searches underway at the interface between cosmology, particle physics, and field theory. The mystery of dark matter (DM) is one of the greatest common unsolved…

High Energy Physics - Phenomenology · Physics 2022-03-14 Ahmed Ayad

We consider a dark matter (DM) model offering a very natural explanation of the observed relation, $\Omega_{\rm dark} \sim \Omega_{\rm visible}$. This generic consequence of the model is a result of the common origin of both types of matter…

High Energy Physics - Phenomenology · Physics 2017-09-20 Shuailiang Ge , Xunyu Liang , Ariel Zhitnitsky

We investigate the level-crossing phenomenon in two-axion systems, where the mass eigenvalues intersect as the mass of one axion increases with the cooling of the universe. This phenomenon can significantly alter the abundance of axions in…

High Energy Physics - Phenomenology · Physics 2024-12-16 Kai Murai , Yuma Narita , Fuminobu Takahashi , Wen Yin

A model is presented in the philosophy of the "String Axiverse" of Arvanitaki et al (arXiv:0905.4720v2 [hep-th]) that incorporates a coupling of ultralight axions to their corresponding moduli through the mass term. The light fields roll in…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-19 David J. E. Marsh

Axions and axion-like particles are ubiquitous in extensions of the Standard Model and offer a unifying framework for addressing open problems in cosmology. Depending on their mass and interactions, axions can act as dark matter, drive…

High Energy Physics - Phenomenology · Physics 2026-05-01 Luca Visinelli

Contents: 1. The strong CP problem 2. Dark matter axions 3. The cavity detector of galactic halo axions 4. The phase space structure of cold dark matter halos

High Energy Physics - Phenomenology · Physics 2007-05-23 Pierre Sikivie

The identification of dark matter in our particle physics model is still a very open question. Here we will argue that axinos can be successful dark matter candidates in models with supersymmetry and the axion solution of the strong CP…

Cosmology and Nongalactic Astrophysics · Physics 2009-10-22 Laura Covi , Jihn E. Kim

QCD axions can be a substantial part of dark matter if their mass $m_a\sim10^{-5}$eV. Since the axions were created by the misalignment mechanism, their local energy spectrum density is large. Consequently, the axion-induced atomic…

High Energy Physics - Phenomenology · Physics 2023-06-21 Qiaoli Yang , Shiqin Dong

The exact QCD is one of the cornerstones of particle physics. Hence it would appear that there should exist no physical situation where a broken version of QCD may have any relevance. However, here I shall show that a spontaneously broken…

High Energy Physics - Phenomenology · Physics 2007-05-23 Afsar Abbas

In this talk, I present a pedagogical and historical review related to the CP symmetry. It includes the weak CP violation, the strong CP problem, "invisible" axions and cosmology, and Type-II leptogenesis.

High Energy Physics - Phenomenology · Physics 2017-03-22 Jihn E. Kim

The existence of light QCD axions, whose mass depends on an additional free parameter, can lead to a new ground state of matter, where the sourced axion field reduces the nucleon effective mass. The presence of the axion field has…

High Energy Physics - Phenomenology · Physics 2024-12-20 Antonio Gómez-Bañón , Kai Bartnick , Konstantin Springmann , José A. Pons

We propose to use the nuclear spin excitation in the ferromagnetic A1 phase of the superfluid $^3$He for the axion dark matter detection. This approach is striking in that it is sensitive to the axion-nucleon coupling, one of the most…

High Energy Physics - Phenomenology · Physics 2024-11-04 So Chigusa , Dan Kondo , Hitoshi Murayama , Risshin Okabe , Hiroyuki Sudo

We evaluate the efficiency of axion production from spatially random initial conditions in the axion field, so a network of axionic strings is present. For the first time, we perform numerical simulations which fully account for the large…

High Energy Physics - Phenomenology · Physics 2017-12-13 Vincent B. Klaer , Guy D. Moore

Consistent frameworks of quantum gravity often predict the existence of large numbers of ultralight pseudoscalar degrees of freedom, forming the phenomenological landscape of the String Axiverse. The complexity of the extra-dimensional…

High Energy Physics - Theory · Physics 2018-11-15 Matthew J. Stott

The smallness of neutrino mass, the strong CP problem, and the existence of dark matter are explained in an economical way. The neutrino mass is generated by the colored version of a radiative seesaw mechanism by using color adjoint…

High Energy Physics - Phenomenology · Physics 2017-11-01 Ernest Ma , Takahiro Ohata , Koji Tsumura

As cosmology has entered a phase of precision experiments, the content of the universe has been established to contain interesting and not yet fully understood components, namely dark energy and dark matter. While the cause and exact nature…

High Energy Physics - Phenomenology · Physics 2015-06-25 Lars Bergstrom

Axions have for some time been considered a plausible candidate for dark matter. They can be produced through misalignment, but it has been argued that when inflation occurs before a Peccei-Quinn transition, appreciable production can…

High Energy Physics - Phenomenology · Physics 2021-11-22 Michael Dine , Nicolas Fernandez , Akshay Ghalsasi , Hiren H. Patel
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