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相关论文: The CPT-violating effects on neutron's gravitation…

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The build up of the stress whose relaxation is presumed to account for pulsar frequency glitches can be attributed to various mechanisms, of which the most efficient involve differential rotation of the neutron superfluid in the inner…

天体物理学 · 物理学 2009-11-10 Nicolas Chamel , Brandon Carter

The precise knowledge of the gravitational phase evolution of compact binaries is crucial to the data analysis for gravitational waves. Until recently, it was known analytically (for non-spinning systems) up to the 3.5 post-Newtonian (PN)…

广义相对论与量子宇宙学 · 物理学 2024-01-23 L. Blanchet , G. Faye , Q. Henry , F. Larrouturou , D. Trestini

We argue that a cosmic neutrino background that carries non-zero lepton charge develops gravitational instabilities. Fundamentally, these instabilities are related to the mixed gravity-lepton number anomaly. We have explicitly computed the…

高能物理 - 唯象学 · 物理学 2020-01-27 Neil D. Barrie , Archil Kobakhidze

Quantum states in the Earth's gravitational field can be observed, when ultra-cold neutrons fall under gravity. In an experiment at the Institut Laue-Langevin in Grenoble, neutrons are reflected and trapped in a gravitational cavity above a…

高能物理 - 唯象学 · 物理学 2015-06-25 Hartmut Abele , Stefan Baessler , Alexander Westphal

Extracting the properties of a binary system emitting gravitational waves relies on models describing the last stages of the compact binary coalescence. In this article, we study potential biases inherent to current tidal waveform…

广义相对论与量子宇宙学 · 物理学 2019-07-31 Anuradha Samajdar , Tim Dietrich

Classic tests of CPT symmetry have been done in the neutral-meson system. These have been continued with new results in the framework of the Standard-Model Extension, where the coefficient for CPT violation is both boost and direction…

高能物理 - 唯象学 · 物理学 2016-11-24 Ágnes Roberts

Motion of many comets is affected by non-gravitational forces caused by outgassing from their surfaces. Outgassing also produces reactive torques resulting in cometary spin evolution. We propose that the two processes are correlated and…

地球与行星天体物理 · 物理学 2018-09-17 Roman R. Rafikov

We discuss the possibility that CPT violation may appear as a consequence of microscopic decoherence due to quantum-gravity effects, that we describe using a density-matrix formalism motivated by our studies of non-critical string theory.…

高能物理 - 唯象学 · 物理学 2007-05-23 John Ellis , N. E. Mavromatos , D. V. Nanopoulos

Neutrino oscillations in the presence of Lorentz violation can present novel observable signals in both long- and short-baseline experiments. In this talk we describe the theory and its different regimes depending on properties of the…

高能物理 - 唯象学 · 物理学 2017-08-23 Jorge S. Diaz

Lorentz- and CPT-violating models of electrodynamics with Chern-Simons terms are typically plagued by various sorts of instabilities. However, when the Chern-Simons term arises from a slow time variation in a pseudoscalar field with an…

高能物理 - 理论 · 物理学 2020-08-11 Sapan Karki , Brett Altschul

In this paper, we carry out a systematic analysis of the theoretical and observational constraints on the dimensionless coupling constants $c_i$ ($i=1,2,3,4$) of the Einstein-aether theory, taking into account the events GW170817 and GRB…

广义相对论与量子宇宙学 · 物理学 2018-06-20 Jacob Oost , Shinji Mukohyama , Anzhong Wang

In some quantum theories of gravity, deviations from the laws of relativity could be comparatively large while escaping detection to date. In the neutrino sector, precision experiments with beta decay yield new and improved constraints on…

高能物理 - 唯象学 · 物理学 2013-12-10 Jorge S. Diaz , Alan Kostelecky , Ralf Lehnert

Gravitational waves are tiny disturbances in space-time and are a fundamental, although not yet directly confirmed, prediction of General Relativity. Rapidly rotating neutron stars are one of the possible sources of gravitational radiation…

天体物理学 · 物理学 2008-12-03 Aaron Worley , Plamen G. Krastev , Bao-An Li

Neutron stars are known to show accelerated spin-up of their rotational frequency called a glitch. Highly magnetized rotating neutron stars (pulsars) are frequently observed by radio telescopes (and in other frequencies), where the glitch…

高能天体物理现象 · 物理学 2022-11-30 Dixeena Lopez , Shubhanshu Tiwari , Marco Drago , David Keitel , Claudia Lazzaro , Giovanni Andrea Prodi

It was recently reported that there exists a population of "glitch candidates" and "anti-glitch candidates" which are effectively small spin-ups and spin-downs of a neutron star with magnitudes smaller than those seen in typical glitches.…

高能天体物理现象 · 物理学 2022-12-07 Garvin Yim , D. I. Jones

We experimentally demonstrate an alternative method for the dynamic generation of atomic spin squeezing, building on the interplay between linear coupling and nonlinear phase evolution. Since the resulting quantum dynamics can be seen as…

量子物理 · 物理学 2015-07-13 W. Muessel , H. Strobel , D. Linnemann , T. Zibold , B. Juliá-Díaz , M. K. Oberthaler

We revisit the decay of the orbital period in binary systems that occurs due to the emission of gravitational waves in the context of modified gravity models where the coupling $G_{gw}$ between matter and on-shell gravitons is allowed to…

广义相对论与量子宇宙学 · 物理学 2022-11-22 Diego Santos de Jesus , Hermano Velten , Federico Piazza

Experimental searches for new, "fifth" forces are attracting a lot of attention because they allow to test theoretical extensions to the standard model. Here, we report a new experimental search for possible fifth forces, specifically…

原子物理 · 物理学 2022-12-13 Kai Wei , Wei Ji , Changbo Fu , Arne Wickenbrock , Jiancheng Fang , Victor Flambaum , Dmitry Budker

A time-reversal-violating spin-correlation coefficient in the total cross section for polarized neutrons incident on a tensor rank-2 polarized target is calculated by assuming a time-reversal-noninvariant, parity-conserving ``five-fold"…

核理论 · 物理学 2009-09-25 V. Hnizdo , C. R. Gould

Recent theoretical work has made it plausible for neutron stars (NSs) to lose angular momentum via gravitational radiation on long timescales (around Myrs) while actively accreting. The gravitational waves (GWs) can either be emitted via…

天体物理学 · 物理学 2007-05-23 Lars Bildsten