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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

The ISLAND (Inverse Square Law And Newtonian Dynamics) Space Explorer is a new concept to test the gravitational Inverse Square Law at: (1) submillimeter scale and (2) at the largest Solar System scales (dozens of Astronomical Units --AU).…

广义相对论与量子宇宙学 · 物理学 2018-09-05 Joel Bergé

Starting from a static spherically symmetric solution of the Einstein's field equations in the second approximation in the perfect fluid scheme, in the exterior of the source, the corresponding metrics depend on a dimensionless parameter…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Nicholas Ionescu-Pallas , Marius I. Piso , Silvia Onofrei

The field equations of a generalized $f(R)$ type gravity model, in which there is an arbitrary coupling between matter and geometry, are obtained. The equations of motion for test particles are derived from a variational principle in the…

广义相对论与量子宇宙学 · 物理学 2009-05-26 T. Harko

Searches for anisotropies due to Earth's motion relative to a preferred frame -- modern versions of the Michelson-Morley experiment -- provide precise verifications of special relativity. We describe other tests, independent of this motion,…

高能物理 - 唯象学 · 物理学 2008-11-26 Sidney Coleman , Sheldon L. Glashow

A new, field-theory-based framework for discussing and interpreting tests of gravity, notably at the second post-Newtonian (2PN) level, is introduced. Contrary to previous frameworks which attempted at parametrizing any conceivable…

广义相对论与量子宇宙学 · 物理学 2011-09-09 Thibault Damour , Gilles Esposito-Farese

An experimental formula, sometimes named as Newton-collision-formula, (v1-v2) = - e.(u1-u2) relating relative-velocities before & after impact of two bodies under linear-collision, is commonly used successfully for study of…

综合物理 · 物理学 2007-05-23 R. C. Gupta , Ruchi Gupta , Sanjay Gupta

We examine the entropic picture of Newton's second law for the case of circular motion. It is shown that one must make modifications to the derivation of F=ma due to a change in the effective Unruh temperature for circular motion. These…

广义相对论与量子宇宙学 · 物理学 2011-09-12 Michael Duncan , Ratbay Myrzakulov , Douglas Singleton

Based on recent data about the history of the Hubble factor, it is argued that the second law of thermodynamics holds at the largest scales accessible to observation. This is consistent with previous studies of the same question.

宇宙学与河外天体物理 · 物理学 2025-12-02 Narayan Banerjee , Purba Mukherjee , Diego Pavón

Constancy of the speed of light together with the Hubble law lead in a doctrine of expanding universe to a conclusion that universe evolution is not only an expansion of space but also a deceleration of the course of physical time (Taganov,…

综合物理 · 物理学 2008-07-28 Igor N. Taganov

Following two dictums roadmap of Einstein (one, for incorporation of maximum of empirical facts, and the other, on long continued experimental verifications for perfecting a scientific theory) for future generations to make his General…

综合物理 · 物理学 2016-06-15 Abhijit Biswas , Krishnan RS Mani

Stellar kinematics in the external regions of globular clusters can be used to probe the validity of Newton's law in the low acceleration regimes without the complication of non-baryonic dark matter. Indeed, in contrast with what happens…

星系天体物理 · 物理学 2015-05-19 Riccardo Scarpa , Renato Falomo

Chameleon and similar (symmetron and dilation) theories of gravity can exhibit new and interesting features on cosmological scales whilst screening the modifications on small scales thereby satisfying solar system tests of general…

宇宙学与河外天体物理 · 物理学 2015-02-17 Jeremy Sakstein

We analyse the acceleration of a mass with a simple structure taking into account Thermodynamics. Two situations are analysed. The first one for the application of a localized force to a point of the mass. The second one for the application…

综合物理 · 物理学 2007-05-23 Rodrigo de Abreu

One of the outstanding problems of classical celestial mechanics was the restricted 3-body prob- lem, in which a planetoid of small mass is subject to the Newtonian attraction of two celestial bodies of large mass, as it occurs, for…

广义相对论与量子宇宙学 · 物理学 2015-06-18 Emmanuele Battista , Giampiero Esposito

When a small, uncharged, compact object is immersed in an external background spacetime, at zeroth order in its mass it moves as a test particle in the background. At linear order, its own gravitational field alters the geometry around it,…

广义相对论与量子宇宙学 · 物理学 2017-06-07 Adam Pound

We review the experimental evidence for Einstein's special and general relativity. A variety of high precision null experiments verify the weak equivalence principle and local Lorentz invariance, while gravitational redshift and other clock…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Clifford M. Will

A scheme for creating NOON-states of the quasi-momentum of ultra-cold atoms has recently been proposed [New J. Phys. 8, 180 (2006)]. This was achieved by trapping the atoms in an optical lattice in a ring configuration and rotating the…

量子物理 · 物理学 2015-05-13 David W. Hallwood , Adam Stokes , Jessica J. Cooper , Jacob Dunningham

Newton's third law states that any action is countered by a reaction of equal magnitude but opposite direction. The total force in a system not affected by external forces is thus zero. However, according to the principles of relativity, a…

综合物理 · 物理学 2021-05-13 Shailendra Rajput , Asher Yahalom

A spherically symmetric and static metric that describes physical coordinates is introduced. It is defined to be a metric that gives coordinate independent results for physically observable quantities without a further coordinate…

天体物理学 · 物理学 2007-05-23 Yukio Tomozawa