English
Related papers

Related papers: Axion Dark Matter Detection with Cold Molecules

200 papers

Axions are a theoretically promising dark matter (DM) candidate. In the presence of radiation from bright astrophysical sources at radio frequencies, nonrelativistic DM axions can undergo stimulated decay to two nearly back-to-back photons,…

High Energy Physics - Phenomenology · Physics 2022-03-25 Yitian Sun , Katelin Schutz , Anjali Nambrath , Calvin Leung , Kiyoshi Masui

Quantum Chromodynamics (QCD) is the theory of the strong interactions within the Standard Model of particle physics, which explains more than 99% of the mass of the visible Universe. However, there is evidence that a substantial portion of…

High Energy Physics - Lattice · Physics 2026-04-01 Bastian B. Brandt , Gergely Endrődi , José Javier Hernández Hernández , Gergely Markó , Laurin Pannullo

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 Universe. They also appear in models of inflation, dark…

High Energy Physics - Phenomenology · Physics 2018-08-01 Igor G. Irastorza , Javier Redondo

We consider axionlike particles, as the most probable constituents of dark matter, the Yukawa-type corrections to Newton's gravitational law and constraints on their parameters following from astrophysics and different laboratory…

High Energy Physics - Phenomenology · Physics 2021-09-15 Galina L. Klimchitskaya , Vladimir M. Mostepanenko

The potential to detect axion dark matter through astrophysical processes has shown high promise in recent years. We therefore expand on previous work studying the axion-to-photon conversion efficacy of neutron stars and the interstellar…

High Energy Astrophysical Phenomena · Physics 2026-05-15 Felix Weber , Vikram Ravi

A dark matter axion with mass $m_a$ induces an oscillating electric field in a cylindrical sample placed under a magnetic field $B_0$ parallel to the cylinder axis. When the cylinder is made of a highly electrically conductive material, the…

High Energy Physics - Phenomenology · Physics 2026-04-10 Aiichi Iwazaki

The natural environment of the Earth can act as a sensitive detector for dark matter in ultralight axions. When axions with masses between $1\times10^{-15}\,{\rm eV}$ and $1\times10^{-13}\,{\rm eV}$ pass through the Earth, they interact…

High Energy Physics - Phenomenology · Physics 2025-04-23 Atsushi Nishizawa , Atsushi Taruya , Yoshiaki Himemoto

We investigate a novel technique for the astrophysical detection of axions or axion-like particles in the dark matter halo of the Milky Way based on stimulated decay of axions, which we call axion gegenschein emission. Photons from the…

Cosmology and Nongalactic Astrophysics · Physics 2020-08-07 Oindrila Ghosh , Jordi Salvado , Jordi Miralda-Escudé

Axions are hypothetical particles that may explain the observed dark matter (DM) density and the non-observation of a neutron electric dipole moment. An increasing number of axion laboratory searches are underway worldwide, but these…

High Energy Physics - Phenomenology · Physics 2022-03-23 Malte Buschmann , Joshua W. Foster , Anson Hook , Adam Peterson , Don E. Willcox , Weiqun Zhang , Benjamin R. Safdi

The ultralight boson represents a promising dark matter candidate exhibiting unique wave-like behaviors. These properties could transfer to the dark mediator, such as the kinetic mixing dark photon, which can be a link between the dark and…

High Energy Physics - Phenomenology · Physics 2023-08-29 Jinhui Guo , Yuxuan He , Jia Liu , Xiao-Ping Wang , Ke-Pan Xie

Ultra-low-mass axions are a viable dark matter candidate and may form a coherently oscillating classical field. Nuclear spins in experiments on Earth might couple to this oscillating axion dark-matter field, when propagating on Earth's…

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

We review the physics potential of a next generation search for solar axions: the International Axion Observatory (IAXO). Endowed with a sensitivity to discover axion-like particles (ALPs) with a coupling to photons as small as…

Dark matter remains one of the most compelling open problems in modern physics, motivating experimental searches for new light, weakly coupled particles beyond the Standard Model. Despite extensive efforts employing diverse detection…

Instrumentation and Detectors · Physics 2026-02-12 Sharada Sahoo , Jing-han Chen , Mahdi Mirzakhani , Harikrishnan Ramani , Rupak Mahapatra , Surjeet Rajendran

We propose a new table-top experimental configuration for the direct detection of dark matter axions with mass in the $(10^{-6} \rm eV - 10^{-2} \rm eV)$ range using non-perturbative effects in a system with non-trivial spatial topology.…

High Energy Physics - Phenomenology · Physics 2017-08-11 ChunJun Cao , Ariel Zhitnitsky

Hidden monopole is a plausible dark matter candidate due to its stability, but its direct experimental search is extremely difficult due to feeble interactions with the standard model particles in the minimal form. Then, we introduce an…

High Energy Physics - Phenomenology · Physics 2020-02-19 Ryuji Daido , Shu-Yu Ho , Fuminobu Takahashi

Axion as one of the promising dark matter candidates can be detected through narrow radio lines emitted from the magnetic white dwarf stars. Due to the existence of the strong magnetic field, the axion may resonantly convert into the radio…

High Energy Physics - Phenomenology · Physics 2021-06-23 Jin-Wei Wang , Xiao-Jun Bi , Run-Min Yao , Peng-Fei Yin

Axions are well-motivated dark matter candidates with simple cosmological production mechanisms. They were originally introduced to solve the strong CP problem, but also arise in a wide range of extensions to the Standard Model. This…

High Energy Physics - Experiment · Physics 2023-03-31 C. B. Adams , N. Aggarwal , A. Agrawal , R. Balafendiev , C. Bartram , M. Baryakhtar , H. Bekker , P. Belov , K. K. Berggren , A. Berlin , C. Boutan , D. Bowring , D. Budker , A. Caldwell , P. Carenza , G. Carosi , R. Cervantes , S. S. Chakrabarty , S. Chaudhuri , T. Y. Chen , S. Cheong , A. Chou , R. T. Co , J. Conrad , D. Croon , R. T. D'Agnolo , M. Demarteau , N. DePorzio , M. Descalle , K. Desch , L. Di Luzio , A. Diaz-Morcillo , K. Dona , I. S. Drachnev , A. Droster , N. Du , K. Dunne , B. Döbrich , S. A. R. Ellis , R. Essig , J. Fan , J. W. Foster , J. T. Fry , A. Gallo Rosso , J. M. García Barceló , I. G. Irastorza , S. Gardner , A. A. Geraci , S. Ghosh , B. Giaccone , M. Giannotti , B. Gimeno , D. Grin , H. Grote , M. Guzzetti , M. H. Awida , R. Henning , S. Hoof , G. Hoshino , V. Irsic , K. D. Irwin , H. Jackson , D. F. Jackson Kimball , J. Jaeckel , K. Jakovcic , M. J. Jewell , M. Kagan , Y. Kahn , R. Khatiwada , S. Knirck , T. Kovachy , P. Krueger , S. E. Kuenstner , N. A. Kurinsky , R. K. Leane , A. F. Leder , C. Lee , K. W. Lehnert , E. W. Lentz , S. M. Lewis , J. Liu , M. Lynn , B. Majorovits , D. J. E. Marsh , R. H. Maruyama , B. T. McAllister , A. J. Millar , D. W. Miller , J. Mitchell , S. Morampudi , G. Mueller , S. Nagaitsev , E. Nardi , O. Noroozian , C. A. J. O'Hare , N. S. Oblath , J. L. Ouellet , K. M. W. Pappas , H. V. Peiris , K. Perez , A. Phipps , M. J. Pivovaroff , P. Quílez , N. M. Rapidis , V. H. Robles , K. K. Rogers , J. Rudolph , J. Ruz , G. Rybka , M. Safdari , B. R. Safdi , M. S. Safronova , C. P. Salemi , P. Schuster , A. Schwartzman , J. Shu , M. Simanovskaia , J. Singh , S. Singh , K. Sinha , J. T. Sinnis , M. Siodlaczek , M. S. Smith , W. M. Snow , A. V. Sokolov , A. Sonnenschein , D. H. Speller , Y. V. Stadnik , C. Sun , A. O. Sushkov , T. M. P. Tait , V. Takhistov , D. B. Tanner , F. Tavecchio , D. J. Temples , J. H. Thomas , M. E. Tobar , N. Toro , Y. -D. Tsai , E. C. van Assendelft , K. van Bibber , M. Vandegar , L. Visinelli , E. Vitagliano , J. K. Vogel , Z. Wang , A. Wickenbrock , L. Winslow , S. Withington , M. Wooten , J. Yang , B. A. Young , F. Yu , K. Zhou , T. Zhou

New one- and two-loop contributions to the lepton's and nucleon's EDM, which are induced by an axion-like particle dark matter background, are examined. These contributions include effects from CP-violating ALP interactions with photons,…

High Energy Physics - Phenomenology · Physics 2025-09-17 Jason L. Evans , Nan Li , Junyuan Lyu

We show that dark matter can be accounted for by an axion that solves the strong CP problem, but is much lighter than usual due to a $Z_\mathcal{N}$ symmetry. The whole mass range from the canonical QCD axion down to the ultra-light regime…

High Energy Physics - Phenomenology · Physics 2023-02-16 Luca Di Luzio , Belen Gavela , Pablo Quilez , Andreas Ringwald