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Recently, BICEP2 collaboration has released their results on the measurements of the CMB polarizations. In the framework of the $\Lambda$CDM with a power law form of the scalar primordial power spectrum, this new measurement on the B-mode…

宇宙学与河外天体物理 · 物理学 2014-05-08 Hong Li , Jun-Qing Xia , Xinmin Zhang

We present a nonlinear post-Friedmann framework for structure formation, generalizing to cosmology the weak-field (post-Minkowskian) approximation, unifying the treatment of small and large scales. We consider a universe filled with a…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Irene Milillo , Daniele Bertacca , Marco Bruni , Andrea Maselli

We reconsider four-dimensional scalar field theory in presence of Robin boundary conditions on two parallel plates. These boundary conditions are directly imposed in the path integral definition of the theory via auxiliary fields living on…

高能物理 - 理论 · 物理学 2024-09-12 David Dudal , Aaron Gobeyn , Bruno W. Mintz , Thomas Oosthuyse , Sebbe Stouten

It is difficult to discover pulsars via their gamma-ray emission because current instruments typically detect fewer than one photon per million rotations. This creates a significant computing challenge for isolated pulsars, where the…

高能天体物理现象 · 物理学 2020-10-23 L. Nieder , B. Allen , C. J. Clark , H. J. Pletsch

We consider a recently proposed class of extended teleparallel theories of gravity, which entail a scalar field which is non-minimally coupled to the torsion of a flat, metric-compatible connection. This class of scalar-torsion theories of…

广义相对论与量子宇宙学 · 物理学 2020-01-24 Elena D. Emtsova , Manuel Hohmann

Starting from the global parametrized post-Newtonian (PPN) reference system with two PPN parameters $\gamma$ and $\beta$ we consider a space-bounded subsystem of matter and construct a local reference system for that subsystem in which the…

广义相对论与量子宇宙学 · 物理学 2011-07-19 Sergei A. Klioner , Michael H. Soffel

Primordial magnetic fields (PMFs), which were generated in the early Universe before recombination, affect the motion of plasma and then the cosmic microwave background and the matter power spectrum. We consider constraints on PMFs with a…

宇宙学与河外天体物理 · 物理学 2013-12-03 Dai G. Yamazaki , Kiyotomo Ichiki , Keitaro Takahashi

Power-law inflation with $a(t) \propto t^m$ is conceptually simple and predicts a scalar tilt $n_s = 1 - 2/m$ compatible with CMB data, but in four-dimensional Einstein gravity it typically yields a tensor-to-scalar ratio $r = 16/m$ that is…

广义相对论与量子宇宙学 · 物理学 2026-02-19 Daniel Oliveira , Seyed Rasouli , Joao Marto , Paulo Moniz

Pulsar Timing constraints on scalar-tensor theories with conformal and disformal couplings to matter are discussed. Reducing the dynamics to the motion in the centre of mass frame and using the mean anomaly parametrisation, we find the…

广义相对论与量子宇宙学 · 物理学 2023-03-24 David Benisty , Philippe Brax , Anne-Christine Davis

Using a formulation of the post-Newtonian expansion in terms of Feynman graphs, we discuss how various tests of General Relativity (GR) can be translated into measurement of the three- and four-graviton vertices. In problems involving only…

广义相对论与量子宇宙学 · 物理学 2015-05-13 Umberto Cannella , Stefano Foffa , Michele Maggiore , Hillary Sanctuary , Riccardo Sturani

An asymptotic framework is defined for the small parameter eta which quantifies a good separation between the extended bodies that make a weakly gravitating system. This is introduced within an alternative scalar theory of gravitation,…

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

This work systematically investigates the post-Newtonian behavior of general quadratic gravity in the weak-field regime. By extending the Einstein-Hilbert action to include quadratic curvature terms as $\mathcal{L}\propto R-\lambda C^2+\mu…

广义相对论与量子宇宙学 · 物理学 2026-04-28 Jie Zhu , Hao Li

Spatial and temporal variations in the electron-to-proton mass ratio, mu, and in the fine-structure constant, alpha, are predicted in non-Standard models aimed to explain the nature of dark energy. Among them the so-called chameleon-like…

宇宙学与河外天体物理 · 物理学 2009-11-20 S. A. Levshakov , I. I. Agafonova , P. Molaro , D. Reimers

We present a general method for determining the masses and orbital parameters of binary millisecond pulsars with long orbital periods (P_orb >> 1 yr), using timing data in the form of pulse frequency derivatives. We apply our method to…

天体物理学 · 物理学 2009-10-28 K. J. Joshi , F. A. Rasio

In the framework of teleparallel gravity, the Friedman-Robertson-Walker cosmological model with scalar tensor theory where scalar field is non-minimally coupled to both the torsion scalar and boundary term is studied. Utilizing the Noether…

广义相对论与量子宇宙学 · 物理学 2018-08-29 Ganim Gecim , Yusuf Kucukakca

In this followup analysis, we update previous constraints on the Transitional Planck Mass (TPM) modified gravity model using the latest version of EFTCAMB and provide new constraints using SPT and Planck anisotropy data along with Planck…

宇宙学与河外天体物理 · 物理学 2023-07-25 Joshua A Kable , Giampaolo Benevento , Graeme E Addison , Charles L Bennett

New tests are proposed to constrain possible deviations from local Lorentz invariance and local position invariance in the gravity sector. By using precise timing results of two binary pulsars, i.e., PSRs J1012+5307 and J1738+0333, we are…

广义相对论与量子宇宙学 · 物理学 2016-12-28 Lijing Shao , Norbert Wex , Michael Kramer

Analytical expressions for the orbital precessions affecting the relative motion of the components of a local binary system induced by Lorentz-violating Preferred Frame Effects (PFE) are explicitly computed in terms of the PPN parameters…

广义相对论与量子宇宙学 · 物理学 2014-01-06 Lorenzo Iorio

The violation of the weak equivalence principle (EP) in the gravitational field of the Earth, described by the E\"otv\"os parameter $\eta_\oplus$, was recently constrained to the level $\left|\eta_\oplus\right| \lesssim 10^{-14}$ by the…

广义相对论与量子宇宙学 · 物理学 2018-06-15 Lijing Shao , Norbert Wex , Michael Kramer

We formulate a theory combining the principles of a scalar-tensor gravity and Rastall's proposal of a violation of the usual conservation laws. We obtain a scalar-tensor theory with two parameters $\omega$ and $\lambda$, the latter…