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相关论文: Modulation and diurnal variation in axionic dark m…

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The dynamics of spin in external electromagnetic, gravitational, and axion fields is analysed in the framework of the gravitoelectromagnetism approach in Einstein's general relativity theory. We consistently extend the recent studies from…

广义相对论与量子宇宙学 · 物理学 2023-07-07 Yuri N. Obukhov

Due to the accuracy now reached by space geodetic techniques, and also considering some modelisations, the temporal variations of some Earth Gravity Field coefficients can be determined. They are due to Earth oceanic and solid tides, as…

天体物理学 · 物理学 2007-11-29 G. Bourda , N. Capitaine

It is widely believed that axions are ubiquitous in string theory and could be the dark matter. The peculiar features of the axion dark matter are coherent oscillations and a coupling to the electromagnetic field through the Chern-Simons…

高能物理 - 理论 · 物理学 2018-04-24 Daiske Yoshida , Jiro Soda

We propose to search for scalar dark matter via its effects on the electromagnetic fine-structure constant and particle masses. Scalar dark matter that forms an oscillating classical field produces `slow' linear-in-time drifts and…

高能物理 - 唯象学 · 物理学 2015-11-16 Yevgeny V. Stadnik , Benjamin M. Roberts , Victor V. Flambaum , Vladimir A. Dzuba

Stellar variability due to magnetic activity and flows at different spatial scales strongly impacts radial velocities. This variability is seen as oscillations, granulation, supergranulation, and meridional flows. The effect of this latter…

太阳与恒星天体物理 · 物理学 2020-06-17 Nadège Meunier , Anne-Marie Lagrange

We study the presence of resonances in the region of space around the Earth. We consider a massless body (e.g, a dust particle or a small space debris) subject to different forces: the gravitational attraction of the geopotential, the…

地球与行星天体物理 · 物理学 2020-02-19 Alessandra Celletti , Catalin Gales , Christoph Lhotka

Due to non-homogeneous mass distribution and non-uniform velocity rate inside the Sun, the solar outer shape is distorted in latitude. In this paper, we analyze the consequences of a temporal change in this figure on the luminosity. To do…

太阳与恒星天体物理 · 物理学 2011-08-31 Z. Fazel , J. P. Rozelot , S. Lefebvre , A. Ajabshirizadeh , S. Pireaux

Implications of supersymmetrizing the clockwork axions are studied. Supersymmetry ensures that the saxions and axinos have the same pattern of the coupling hierarchy as the clockwork axions. If we assume supersymmetry breaking is universal…

高能物理 - 唯象学 · 物理学 2020-07-21 Kyu Jung Bae , Sang Hui Im

We present a pedagogical introduction to the direct search of axions as dark matter, as well as to searches for solar axions. The plethora of experimental searches exploit the axion's coupling to two photons: They attempt to convert the…

高能物理 - 唯象学 · 物理学 2025-07-10 Babette Döbrich , Igor G. Irastorza

We show that Earth's natural environment can serve as a powerful probe for ultralight axion dark matter. In the presence of global geomagnetic fields, the axions with masses ranging from $10^{-15}\,{\rm eV}-10^{-13}\,{\rm eV}$ induce…

高能物理 - 唯象学 · 物理学 2025-09-19 Atsushi Taruya , Atsushi Nishizawa , Yoshiaki Himemoto

The DAMA collaboration reported an annually modulated rate with a phase compatible with a Dark Matter induced signal. We point out that a slowly varying rate can bias or even simulate an annual modulation if data are analyzed in terms of…

高能物理 - 实验 · 物理学 2020-05-20 Dario Buttazzo , Paolo Panci , Nicola Rossi , Alessandro Strumia

We present an overview of recent developments in the detection of light bosonic dark matter, including axion, pseudoscalar axion-like and scalar dark matter, which form either a coherently oscillating classical field or topological defects…

原子物理 · 物理学 2015-09-04 Y. V. Stadnik , V. V. Flambaum

We propose a novel method to detect axion dark matter based on a topological phenomenon known as the shift current. We exploit the second-order nonlinearity of the shift current by applying a strong oscillating electric field. This field…

高能物理 - 唯象学 · 物理学 2025-05-23 Dan Kondo , Takahiro Morimoto , Genta Osaki , Thanaporn Sichanugrist

The search for dark matter (DM) is one of the most active and challenging areas of current research. Possible DM candidates are ultralight fields such as axions and weak interacting massive particles (WIMPs). Axions piled up in the center…

太阳与恒星天体物理 · 物理学 2017-09-13 Fabrizio Tamburini , Ignazio Licata

We search for transient variations of the fine structure constant using data from a European network of fiber-linked optical atomic clocks. By searching for coherent variations in the recorded clock frequency comparisons across the network,…

Axion dark matter is interesting as it allows a natural coupling to the gravitational Chern-Simons term. In the presence of an axion background, the gravitational Chern-Simons term produces parity violating effects in the gravitational…

广义相对论与量子宇宙学 · 物理学 2020-02-13 Chong-Sun Chu , Jiro Soda , Daiske Yoshida

We report on a search for ultra-low-mass axion-like dark matter by analysing the ratio of the spin-precession frequencies of stored ultracold neutrons and $^{199}$Hg atoms for an axion-induced oscillating electric dipole moment of the…

高能物理 - 实验 · 物理学 2018-05-28 N. J. Ayres

Axion dark matter differentiates the phase velocities of the circular-polarized photons. In Phys.Rev.Lett. 123 (2019) no.11, 111301, we have proposed a scheme to measure the phase difference by using a linear optical cavity. If the scheme…

高能物理 - 唯象学 · 物理学 2019-12-20 Koji Nagano , Ippei Obata , Tomohiro Fujita , Yuta Michimura

Recently, a discussion about the effects of the anisotropy in the spatial density of Dark Matter in the Solar neighbourhood due to the motion of the Sun through the Galactic halo on the orbital motion of the solar system's planets and their…

广义相对论与量子宇宙学 · 物理学 2019-09-11 Lorenzo Iorio

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