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Gyroscopes play a crucial role in many and diverse applications associated with navigation, positioning, and inertial sensing [1]. In general, most optical gyroscopes rely on the Sagnac effect -- a relativistically induced phase shift that…

According to the cosmological principle, the Universe should appear isotropic, without any preferred directions, to an observer whom we may consider to be fixed in the co-moving co-ordinate system of the expanding Universe. Such an observer…

宇宙学与河外天体物理 · 物理学 2013-06-11 Ashok K. Singal

Our proper acceleration with respect to the Cosmic Microwave Background results in a real-time change of the angular position of distant extragalactic sources. The cosmological component of this aberration drift signal, the non-inertial…

宇宙学与河外天体物理 · 物理学 2018-07-18 Julien Bel , Christian Marinoni

We generalize tensor-scalar theories of gravitation by the introduction of an abnormally weighting type of energy. This theory of tensor-scalar anomalous gravity is based on a relaxation of the weak equivalence principle that is now…

天体物理学 · 物理学 2009-01-14 J. -M. Alimi , A. Füzfa

Collapse calculations indicate that the hot newly born protoneutron stars (PNS) rotate differentially so that strong toroidal magnetic field components should exist in the outer crust where also the Hall effect appears to be important when…

天体物理学 · 物理学 2015-05-13 Guenther Ruediger , Manfred Schultz , Michael Mond , Dmitry A. Shalybkov

Chiral symmetries in field theory are typically affected by an anomaly in the quantum theory. This anomaly emerges when one introduces an interaction with a Yang-Mills or gravitational background. Physical applications of this quantum…

广义相对论与量子宇宙学 · 物理学 2021-09-22 Adrian del Rio

The trajectories of test particles moving in the gravitational field of a non-spherically symmetric mass distribution become affected by the presence of multipole moments. In the case of hyperbolic trajectories, the quadrupole moment of an…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Hernando Quevedo

A uniformly accelerated charged particle feels the vacuum as thermally excited and fluctuates around the classical trajectory. Then we may expect additional radiation besides the Larmor radiation. It is called Unruh radiation. In this…

高能物理 - 唯象学 · 物理学 2011-02-24 Satoshi Iso , Yasuhiro Yamamoto , Sen Zhang

Peculiar motion of the solar system, determined from the dipole anisotropy in the Cosmic Microwave Background Radiation (CMBR), has given a velocity $370$ km s$^{-1}$ along RA$=168^{\circ}$, Dec$=-7^{\circ}$. Subsequent peculiar motion…

宇宙学与河外天体物理 · 物理学 2023-01-04 Ashok K. Singal

An object moving with the acceleration will change the temperature of environment around it, because of the presence of the Unruh thermal effect. In this work, we investigate the impact of Unruh thermal noise on the quantum-memory-assisted…

广义相对论与量子宇宙学 · 物理学 2024-11-26 Yu-Kun Zhang , Li-Juan Li , Xue-Ke Song , Liu Ye , Dong Wang

In the context of a parametric theory (with the time being a dynamical variable) we consider the coupling between the quantum vacuum and the background gravitation that pervades the universe (unavoidable because of the universality of…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Antonio F. Ranada , Alfredo Tiemblo

The variation in the intensity of cosmic rays at small angular scales is attributed to the interstellar turbulence in the vicinity of the Solar system. We show that {a turbulent origin of the small-scale structures implies that} the…

高能天体物理现象 · 物理学 2018-12-12 Rahul Kumar , Noemie Globus , David Eichler , Martin Pohl

The observed radii of M dwarfs in eclipsing binaries exceed predicted radii by ~ 5%. To investigate this anomaly, the structure of low-mass stars irradiated by a close companion is considered. Irradiation modifies the surface boundary…

太阳与恒星天体物理 · 物理学 2017-05-24 L. B. Lucy

The radial acceleration relation (RAR) of late-type galaxies relates their dynamical acceleration, $g_\text{obs}$, to that sourced by baryons alone, $g_\text{bar}$, across their rotation curves. Literature fits to the RAR have fixed the…

星系天体物理 · 物理学 2024-02-27 Harry Desmond

Radiation-pressure instability was identified soon after the seminal classical accretion disk models of Shakura-Sunyaev and Novikov-Thorne, yet its full implications remain an active area of investigation. These models form the backbone of…

高能天体物理现象 · 物理学 2025-12-10 Agnieszka Janiuk , Bozena Czerny , Pulkit Ojha , Yuri Cavecchi , Federico Vincentelli

In analyzing the nature of thermal radiance experienced by an accelerated observer (Unruh effect), an eternal black hole (Hawking effect) and in certain types of cosmological expansion, one of us proposed a unifying viewpoint that these can…

广义相对论与量子宇宙学 · 物理学 2008-11-26 Alpan Raval , B. L. Hu , Don Koks

Both the recently reported anomalous secular increase of the astronomical unit, of the order of a few cm yr^-1, and of the eccentricity of the lunar orbit e_ = (9+/-3) 10^-12 yr^-1 can be phenomenologically explained by postulating that the…

广义相对论与量子宇宙学 · 物理学 2011-07-26 Lorenzo Iorio

Whenever an experiment can be described classically, quantum physics must predict the same outcome. Intuitively, there is nothing quantum about an accelerating observer travelling through a vacuum. It is therefore not surprising that many…

量子物理 · 物理学 2026-03-24 Sara Kanzi , Daniel Hodgson , Almut Beige

The Unruh effect remains a central topic in quantum field theory, although its direct experimental verification continues to be challenging. Recent efforts have therefore focused on indirect detection strategies in which the Unruh effect…

广义相对论与量子宇宙学 · 物理学 2026-01-01 Manuel de Atocha Rodríguez Fernández , Alexander I. Nesterov , Gennady P. Berman , C. Moreno-González

We present high precision radial velocity observations of HD17156 during a transit of its eccentric Jovian planet. In these data, we detect the Rossiter-McLaughlin effect, which is an apparent perturbation in the velocity of the star due to…

天体物理学 · 物理学 2009-11-13 William D. Cochran , Seth Redfield , Michael Endl , Anita L. Cochran