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Detection schemes for the quantum chromodynamics axions and other axion-like particles in light-shining-through-a-wall (LSW) experiments are based on the conversion of these particles into photons in a magnetic field. An alternative scheme…

高能物理 - 唯象学 · 物理学 2019-02-13 H. B. Tran Tan , V. V. Flambaum , I. B. Samsonov , Y. V. Stadnik , D. Budker

We advocate an idea that the presence of the daily and annual modulations of the axion flux on the Earth surface may dramatically change the strategy of the axion searches. Our computations are based on the so-called Axion Quark Nugget…

高能物理 - 唯象学 · 物理学 2020-02-19 Dmitry Budker , Victor V. Flambaum , Xunyu Liang , Ariel Zhitnitsky

The axion, as a leading dark matter candidate, is the target of many ongoing and proposed experimental searches based on its coupling to photons. Ultralight axions that couple to photons can also cause polarization rotation of light, which…

高能物理 - 唯象学 · 物理学 2024-10-08 Xucheng Gan , Lian-Tao Wang , Huangyu Xiao

Axions are some of the best motivated particles beyond the Standard Model. We show how the attractive self-interactions of dark matter (DM) axions over a broad range of masses, from $10^{-22}$ eV to $10^7$ GeV, can lead to nongravitational…

宇宙学与河外天体物理 · 物理学 2020-04-15 Asimina Arvanitaki , Savas Dimopoulos , Marios Galanis , Luis Lehner , Jedidiah O. Thompson , Ken Van Tilburg

We study the impact of axion emission in simulations of massive star explosions, as an additional source of energy loss complementary to the standard neutrino emission. The inclusion of this channel shortens the cooling time of the nascent…

高能天体物理现象 · 物理学 2016-10-26 Tobias Fischer , Sovan Chakraborty , Maurizio Giannotti , Alessandro Mirizzi , Alexandre Payez , Andreas Ringwald

Dark matter axions may cause transitions between atomic states that differ in energy by an amount equal to the axion mass. Such energy differences are conveniently tuned using the Zeeman effect. It is proposed to search for dark matter…

高能物理 - 唯象学 · 物理学 2020-06-02 P. Sikivie

We introduce a new experimental method for solar hadronic axions search. It is suggested that these axions are created in the Sun during M1 transition between the first thermally excited level at 9.4 keV and the ground state in $^{83}Kr$.…

核实验 · 物理学 2009-12-08 K. Jakovcic , Z. Krecak , M. Krcmar , A. Ljubicic

Electromagnetic radiation with angular frequency equal to half the axion mass stimulates the decay of cold dark matter axions and produces an echo, i.e. faint electromagnetic radiation traveling in the opposite direction. We propose to…

高能物理 - 唯象学 · 物理学 2019-10-02 Ariel Arza , Pierre Sikivie

We study the interaction between axions and nuclei by combining the Peccei-Quinn mechanism with results from quantum chromo-dynamics (QCD) which imply that the QCD condensates are reduced within nuclear matter. Thus, the effective axion…

高能物理 - 唯象学 · 物理学 2024-05-17 Stefan Evans , Ralf Schützhold

Nuclear Magnetic Resonance (NMR) spans diverse fields from biology to quantum science. Employing NMR on a floating object could unveil novel possibilities beyond conventional operational paradigms. Here, we observe Nuclear Magnetic…

量子物理 · 物理学 2024-07-30 J. Voisin , A. Durand , T. Copie , M. Perdriat , G. Hétet

We study the new mechanism of the axion production suggested recently in [1,2]. This mechanism is based on the so-called Axion Quark Nugget (AQN) dark matter model, which was originally invented to explain the similarity of the dark and…

宇宙学与河外天体物理 · 物理学 2020-02-19 Xunyu Liang , Alexander Mead , Md Shahriar Rahim Siddiqui , Ludovic Van Waerbeke , Ariel Zhitnitsky

We report on recent result according to which the fermion-fermion interaction mediated by axions and axion-like particles can be revealed by means of neutron interferometry. We assume that the initial neutron beam is split in two beams…

高能物理 - 唯象学 · 物理学 2024-03-06 Antonio Capolupo , Salvatore Marco Giampaolo , Aniello Quaranta

Axions may be produced in abundance inside stellar cores and then convert into observable X-rays in the Galactic magnetic fields. We focus on the Quintuplet and Westerlund 1 super star clusters, which host large numbers of hot, young stars…

高能物理 - 唯象学 · 物理学 2021-03-03 Christopher Dessert , Joshua W. Foster , Benjamin R. Safdi

We consider a possibility to observe the axion emission from a nearby supernova (SN) in the future, which can be known in advance by the pre-SN alert system, by collider detectors like the LHC detectors (i.e., the ATLAS and the CMS) and the…

高能物理 - 唯象学 · 物理学 2022-05-04 Shoji Asai , Yoshiki Kanazawa , Takeo Moroi , Thanaporn Sichanugrist

We consider a scenario with axions/axion-like particles Chern-Simons gravity coupling, such that gravitational waves can be produced directly from axion wave parametric resonance in the early universe after inflation. This axion gravity…

高能物理 - 唯象学 · 物理学 2024-04-09 Mingqiu Li , Sichun Sun , Qi-Shu Yan , Zhijie Zhao

Current techniques cannot detect axion dark matter over much of its parameter space, particularly in the theoretically well-motivated region where the axion decay constant f_a lies near the GUT and Planck scales. We suggest a novel…

高能物理 - 唯象学 · 物理学 2011-10-03 Peter W. Graham , Surjeet Rajendran

The generation and control of neutron orbital angular momentum (OAM) states and spin correlated OAM (spin-orbit) states provides a powerful probe of materials with unique penetrating abilities and magnetic sensitivity. We describe…

量子物理 · 物理学 2018-11-14 D. Sarenac , J. Nsofini , I. Hincks , M. Arif , Charles W. Clark , D. G. Cory , M. G. Huber , D. A. Pushin

The penetrating ability of cosmic ray muons makes them an attractive probe for imaging dense materials. Here, we describe experimental results from a new technique that uses neutrons generated by cosmic-ray muons to identify the presence of…

Axions are hypothetical particles that were postulated to solve one of the puzzles arising in the standard model of particle physics, namely the strong CP (Charge conjugation and Parity) problem. The new International AXion Observatory…

仪器与探测器 · 物理学 2014-03-05 I. Shilon , A. Dudarev , H. Silva , U. Wagner , H. H. J. ten Kate
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