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We propose a thought experiment to detect low-energy Quantum Gravity phenomena using Quantum Optical Information Technologies. Gravitational field perturbations, such as gravitational waves and quantum gravity fluctuations, decohere the…

量子物理 · 物理学 2009-10-15 Fabrizio Tamburini

The Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) have recently provided new and precise measurements of the Cosmic Microwave Background anisotropy damping tail. This region of the CMB angular spectra, thanks to the…

宇宙学与河外天体物理 · 物理学 2013-05-08 Andrea Marchini , Alessandro Melchiorri , Valentina Salvatelli , Luca Pagano

Recent Pulsar Timing Array (PTA) collaborations show strong evidence for a stochastic gravitational wave background (SGWB) with the characteristic Hellings-Downs inter-pulsar correlations. The signal may stem from supermassive black hole…

广义相对论与量子宇宙学 · 物理学 2025-12-25 N. M. Jiménez Cruz , Ameek Malhotra , Gianmassimo Tasinato , Ivonne Zavala

We propose a novel method for testing isotropy of a three-dimensional distribution using Shannon entropy. We test the method on some Monte Carlo simulations of isotropic and anisotropic distributions and find that the method can effectively…

宇宙学与河外天体物理 · 物理学 2016-08-24 Biswajit Pandey

In the present work the detection, by means of a nondemolition measurement, of a Yukawa term, coexisting simultaneously with gravity, has been considered. In other words, a nondemolition variable for the case of a particle immersed in a…

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

A four mass torsion pendulum facility for testing of the LISA GRS is under development in Trento. With a LISA-like test mass suspended off-axis with respect to the pendulum fiber, the facility allows for a direct measurement of surface…

广义相对论与量子宇宙学 · 物理学 2009-11-11 L. Carbone , A. Cavalleri , G. Ciani , R. Dolesi , M. Hueller , D. Tombolato , S. Vitale , W. J. Weber

Pulsar-timing arrays (PTAs) are seeking gravitational waves from supermassive-black-hole binaries, and there are prospects to complement these searches with stellar-astrometry measurements. Theorists still disagree, however, as to whether…

宇宙学与河外天体物理 · 物理学 2020-06-19 Selim C. Hotinli , Marc Kamionkowski , Andrew H. Jaffe

In this paper, we investigate the influence of the spacetime curvature on the Yukawa potential, focusing on boson-boson interactions derived from the {\Phi^3} theory. Using the Bunch-Parker propagator expansion within Born's first…

广义相对论与量子宇宙学 · 物理学 2025-03-19 J. V. Zamperlini , C. C. Barros

We analyze the measurement of cosmological distances in the presence of torsion in both Einstein-Cartan and Poincare gauge theory of gravity. Using the modified cosmological distance measurements, we use the observed time delays in…

广义相对论与量子宇宙学 · 物理学 2023-09-15 Siamak Akhshabi , Saboura Zamani

The GRAAL experiment could constrain the variations of the speed of light. The anisotropy of the speed of light may imply that the spacetime is anisotropic. Finsler geometry is a reasonable candidate to deal with the spacetime anisotropy.…

高能物理 - 唯象学 · 物理学 2013-05-23 Zhe Chang , Sai Wang

The light scalar field with a coupling to standard model particles provide a possible source of the dark matter, long-range Yukawa forces or violation of the weak equivalence principle, which can be potentially explored by precision gravity…

广义相对论与量子宇宙学 · 物理学 2024-03-05 ChengGang Qin , XiaoYu Lu , BingChen Zhao , Jun Ke , AnBin Du , Jie Luo , YuJie Tan , ChengGang Shao

The nature of the gravitational interaction between ordinary and dark matter is still open. Any deviation from universality or the Newtonian law also modifies the standard assumption of collisionless dark matter. On the other hand,…

高能物理 - 理论 · 物理学 2010-12-14 Zurab Berezhiani , Fabrizio Nesti , Luigi Pilo , Nicola Rossi

This paper is a pedagogical introduction to models of gravity and how to constrain them through cosmological observations. We focus on the Horndeski scalar-tensor theory and on the quantities that can be measured with a minimum of…

宇宙学与河外天体物理 · 物理学 2020-01-27 Luca Amendola , Dario Bettoni , Ana Marta Pinho , Santiago Casas

Identifying the anisotropies in a cosmologically sourced stochastic gravitational wave background (SGWB) would be of significance in shedding light on the nature of primordial inhomogeneities. For example, if SGWB carries isocurvature…

宇宙学与河外天体物理 · 物理学 2023-12-18 Yanou Cui , Soubhik Kumar , Raman Sundrum , Yuhsin Tsai

Motivated by a variety of theories that predict new effects, we tested the gravitational 1/r^2 law at separations between 10.77 mm and 137 microns using two different 10-fold azimuthally symmetric torsion pendulums and rotating 10-fold…

高能物理 - 唯象学 · 物理学 2009-09-29 C. D. Hoyle , D. J. Kapner , B. R. Heckel , E. G. Adelberger , J. H. Gundlach , U. Schmidt , H. E. Swanson

In this work we investigate the anisotropic conformal structure of the gravitational field incorporating dark gravity in a generalized Lagrange geometric framework on the Lorentz tangent bundle and we present two applications; the…

广义相对论与量子宇宙学 · 物理学 2023-08-28 Christos Savvopoulos , Panayiotis Stavrinos

The low-frequency resolution of space-based gravitational wave observatories such as LISA (Laser Interferometry Space Antenna) hinges on the orbital purity of a free-falling reference test mass inside a satellite shield. We present here a…

广义相对论与量子宇宙学 · 物理学 2009-11-10 L. Carbone , A. Cavalleri , R. Dolesi , C. D. Hoyle , M. Hueller , S. Vitale , W. J. Weber

To simplify a number of considerations in the weak field approximation, including the determination of the response of interferometric gravitational wave detectors, the "transverse traceless" (TT) gauge is often used. While the…

广义相对论与量子宇宙学 · 物理学 2009-12-02 Istvan Racz

The two-point angular correlation function is a traditional method used to search for deviations from expectations of isotropy. In this paper we develop and explore a statistically descriptive three-point method with the intended…

天体物理仪器与方法 · 物理学 2009-10-02 J. D. Hague , B. R. Becker , M. S. Gold , J. A. J. Matthews

Motivated by higher-dimensional theories that predict new effects, we tested the gravitational 1/r^2 law at separations ranging down to 218 micrometers using a 10-fold symmetric torsion pendulum and a rotating 10-fold symmetric attractor.…

高能物理 - 唯象学 · 物理学 2008-11-26 C. D. Hoyle , U. Schmidt , B. R. Heckel , E. G. Adelberger , J. H. Gundlach , D. J. Kapner , H. E. Swanson