Results 21 to 30 of about 688,478 (251)

Systematic treatment of displacements, strains, and electric fields in density-functional perturbation theory [PDF]

open access: yes, 2005
The methods of density-functional perturbation theory may be used to calculate various physical response properties of insulating crystals including elastic, dielectric, Born charge, and piezoelectric tensors.
Xifan Wu   +7 more
semanticscholar   +1 more source

Radiative and chiral corrections to elastic lepton-proton scattering in chiral perturbation theory [PDF]

open access: yesPhysical Review D, 2020
Pulak Talukdar, 2, ∗ Vanamali C. Shastry, 4, † Udit Raha, ‡ and Fred Myhrer § Department of Physics, Indian Institute of Technology Guwahati, Guwahati 781039, Assam, India. Department of Physics, S. B. Deorah College, Guwahati, Assam 781007.
P. Talukdar   +3 more
semanticscholar   +1 more source

Primordial black holes generated by the non-minimal spectator field [PDF]

open access: yesScience China Physics Mechanics and Astronomy, 2022
We improve and generalize the non-minimal curvaton model originally proposed in arXiv: 2112.12680 to a model in which a spectator field non-minimally couples to an inflaton field and the power spectrum of the perturbation of spectator field at small ...
De-Shuang Meng, Chengchao Yuan, Q. Huang
semanticscholar   +1 more source

No evidence for synchronization of the solar cycle by a "clock" [PDF]

open access: yesAstronomy & Astrophysics, 2023
The length of the solar activity cycle fluctuates considerably. The temporal evolution of the corresponding cycle phase, that is, the deviation of the epochs of activity minima or maxima from strict periodicity, provides relevant information concerning ...
E. Weisshaar, R. Cameron, M. Schussler
semanticscholar   +1 more source

Fragmentation of a dynamically condensing radiative layer [PDF]

open access: yes, 2009
In this paper, the stability of a dynamically condensing radiative gas layer is investigated by linear analysis. Our own time-dependent, self-similar solutions describing a dynamical condensing radiative gas layer are used as an unperturbed state.
Iwasaki, Kazunari, Tsuribe, Toru
core   +1 more source

Tensor perturbations from bounce inflation scenario in f(Q) gravity [PDF]

open access: yesScience China Physics, Mechanics & Astronomy, 2023
In this paper, we construct a bounce inflation cosmological scenario in the framework of the modified symmetric teleparallel gravity, namely f(Q) theory, and investigate the tensor perturbations therein.
K. Hu, Tanmoy Paul, Taotao Qiu
semanticscholar   +1 more source

OGLE-2009-BLG-092/MOA-2009-BLG-137: A Dramatic Repeating Event With the Second Perturbation Predicted by Real-Time Analysis [PDF]

open access: yes, 2010
We report the result of the analysis of a dramatic repeating gravitational microlensing event OGLE-2009-BLG-092/MOA-2009-BLG-137, for which the light curve is characterized by two distinct peaks with perturbations near both peaks.
A. Allan   +129 more
core   +3 more sources

Quasi-radial modes of pulsating neutron stars: numerical results for general-relativistic rigidly rotating polytropic models [PDF]

open access: yes, 2014
In this paper we compute general-relativistic polytropic models simulating rigidly rotating, pulsating neutron stars. These relativistic compact objects, with a radius of $\sim 10 \, \mathrm{km}$ and mass between $\sim 1.4$ and $3.2$ solar masses, are ...
Geroyannis, Vassilis   +1 more
core   +1 more source

Gauge invariant perturbations of general spherically symmetric spacetimes [PDF]

open access: yesScience China Physics Mechanics and Astronomy, 2022
In this paper, the gauge choices in general spherically symmetric spacetimes are explored. In particular, we construct the gauge invariant variables and the master equations for both the Detweiler easy gauge and the Regge-Wheeler gauge, respectively. The
Wentao Liu   +3 more
semanticscholar   +1 more source

Euclid preparation. XLI. Galaxy power spectrum modelling in real space [PDF]

open access: yesAstronomy & Astrophysics, 2023
We investigate the accuracy of the perturbative galaxy bias expansion in view of the forthcoming analysis of the spectroscopic galaxy samples. We compare the performance of a Eulerian galaxy bias expansion using state-of-the-art prescriptions from the ...
Euclid Collaboration A. Pezzotta   +499 more
semanticscholar   +1 more source

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