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相关论文: Axion Homeopathy: Screening Dilaton Interactions

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Axion-like fields are naturally generated by a mechanism of anomaly cancellation of one or more anomalous gauge abelian symmetries at the Planck scale, emerging as duals of a two-form from the massless bosonic sector of string theory. This…

高能物理 - 唯象学 · 物理学 2018-07-04 Claudio Coriano , Paul H. Frampton

Coupled dark sector models have gained significant attention, motivated by recent advances in cosmology and the pressing need to address unresolved puzzles. In this work, we study coupled scalar dark sector models inspired by…

高能物理 - 理论 · 物理学 2025-09-05 Saba Rahimy , Elsa M. Teixeira , Ivonne Zavala

A global O$(2,2)$ symmetry is found in the Brans-Dicke theory of gravity when the dilaton is coupled to axion and moduli fields. The symmetry is broken if a cosmological constant is introduced. Within the class of spatially homogeneous…

广义相对论与量子宇宙学 · 物理学 2016-08-31 James E. Lidsey

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…

高能物理 - 唯象学 · 物理学 2025-04-23 Atsushi Nishizawa , Atsushi Taruya , Yoshiaki Himemoto

The axion dark matter echo technique, proposed in Ref. [1], aims to search for axion dark matter by detecting the electromagnetic echo coming from stimulated decay of ambient axion dark matter interacting with a radio-microwave outgoing…

高能物理 - 唯象学 · 物理学 2023-01-11 Ariel Arza , Abaz Kryemadhi , Konstantin Zioutas

We discuss the two-dimensional dilaton gravity with a scalar field as the source matter. The coupling between the gravity and the scalar, massless, field is presented in an unusual form. We work out two examples of these couplings, and…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Marcelo Alves

Most matter in the Universe is invisible and unknown, which is called dark matter. A candidate of dark matter is axion, which is an ultra-light particle motivated as a solution for the CP problem. Axions form clouds in a galactic halo,…

广义相对论与量子宇宙学 · 物理学 2022-10-14 Takuya Tsutsui , Atsushi Nishizawa

In this work, we propose to employ the concept of photon self-interaction for axion detection. In particular, we derive the interaction Hamiltonian for photons via axions in a ring cavity. We show that when the incoming photons are…

高能物理 - 唯象学 · 物理学 2025-04-15 Ahmad Hoseinpour , Moslem Zarei , Mehdi Abdi

We study fermions derivatively coupled to axion-like or pseudoscalar fields, and show that the axial vector current of the fermions is not conserved in the limit where the fermion is massless. This apparent violation of the classical chiral…

高能物理 - 理论 · 物理学 2022-08-24 Peter Adshead , Kaloian D. Lozanov

We investigate the structure of gravitational self-interactions of coherently oscillating axions in the general relativistic framework. A generic action for a massive scalar field in the Friedmann-Robertson-Walker background is first…

高能物理 - 唯象学 · 物理学 2014-03-18 Toshifumi Noumi , Ken'ichi Saikawa , Ryosuke Sato , Masahide Yamaguchi

We propose an alternative scenario for the axion misalignment mechanism based on the nontrivial interplay between the axion and a light dilaton in the early universe. Dark matter abundance is still sourced by the initial misalignment of the…

高能物理 - 唯象学 · 物理学 2023-05-31 Ling-Xiao Xu , Seokhoon Yun

Standard axion electrodynamics has two closely related features. First, the coupling of a massless axion field to photons is quantized, in units proportional to the electric gauge coupling squared. Second, the equations of motion tell us…

高能物理 - 唯象学 · 物理学 2023-12-27 Ben Heidenreich , Jacob McNamara , Matthew Reece

We introduce the concept of impedance matching to axion dark matter by posing the question of why axion detection is difficult, even though there is enough power in each square meter of incident dark-matter flux to energize a LED light…

高能物理 - 唯象学 · 物理学 2021-12-22 Saptarshi Chaudhuri

Ultralight axion-like particles can contribute to the dark matter near the Sun, leading to a distinct, stochastic signature in terrestrial experiments. We search for such particles through their neutron-spin coupling by re-analyzing…

高能物理 - 唯象学 · 物理学 2023-04-05 Junyi Lee , Mariangela Lisanti , William A. Terrano , Michael Romalis

We revisit the theory and constraints on axion-like particles (ALPs) interacting with leptons. We clarify some subtleties in the constraints on ALP parameter space and find several new opportunities for ALP detection. We identify a…

高能物理 - 唯象学 · 物理学 2023-06-23 Wolfgang Altmannshofer , Jeff A. Dror , Stefania Gori

Light scalar particles with couplings of sub-gravitational strength, which can generically be called 'dilatons', can produce violations of the equivalence principle. However, in order to understand experimental sensitivities one must know…

广义相对论与量子宇宙学 · 物理学 2011-03-28 Thibault Damour , John F. Donoghue

We study axion-dilaton cosmologies derived from the low-energy string effective action. We present the classical homogeneous Friedmann-Robertson-Walker solutions and derive the semi-classical perturbation spectra in the dilaton, axion and…

高能物理 - 理论 · 物理学 2009-10-30 E. J. Copeland , Richard Easther , David Wands

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…

高能物理 - 实验 · 物理学 2023-11-30 Vindhyawasini Prasad

In this contribution an entirely different way compared to conventional approaches for axion, hidden photon and dark matter (DM) detection is proposed for discussion. The idea is to use living plants which are known to be very sensitive to…

高能物理 - 实验 · 物理学 2015-09-29 Fritz Caspers

Axion is a light pseudoscalar particle of much interest for physics of elementary particles and for astrophysics. We review the recently obtained constraints on axion to nucleon coupling constants following from different experiments on…

高能物理 - 唯象学 · 物理学 2015-02-27 G. L. Klimchitskaya , V. M. Mostepanenko