scholarly journals Spin effects in gravitational radiation back reaction. II. Finite mass effects

1998 ◽  
Vol 57 (6) ◽  
pp. 3423-3432 ◽  
Author(s):  
L. Gergely ◽  
Z. Perjés ◽  
M. Vasúth
Keyword(s):  
Gravitational Radiation ◽  
Back Reaction ◽  
Finite Mass ◽  
Mass Effects ◽  
Spin Effects

scholarly journals Spin effects in gravitational radiation back reaction. I. The Lense-Thirring approximation

1998 ◽  
Vol 57 (2) ◽  
pp. 876-884 ◽  
Author(s):  
László Á. Gergely ◽  
Zoltán I. Perjés ◽  
Mátyás Vasúth
Keyword(s):  
Gravitational Radiation ◽  
Back Reaction ◽  
Spin Effects

scholarly journals GRAVITATIONAL WAVEFORMS FOR FINITE MASS BINARIES

2007 ◽  
Vol 22 (13) ◽  
pp. 2405-2414 ◽  
Author(s):  
MÁTYÁS VASÚTH ◽  
JÁNOS MAJÁR
Keyword(s):  
Binary System ◽  
Gravitational Wave ◽  
Gravitational Radiation ◽  
Compact Stars ◽  
Spin Orbit ◽  
Wave Polarization ◽  
Finite Mass ◽  
Compact Binaries ◽  
Eccentric Orbits ◽  
Comparable Mass

One of the promising sources of gravitational radiation is a binary system composed of compact stars. It is an important question of how the rotation of the bodies and the eccentricity of the orbit affect the detectable signal. Here we present a method to evaluate the gravitational wave polarization states for inspiralling compact binaries with comparable mass. We consider eccentric orbits and the spin-orbit contribution in the case of one spinning object up to 1.5 post-Newtonian order. For circular orbits our results are in agreement with existing calculations.

scholarly journals Finite-mass effects on inclusiveB-meson hadroproduction

2008 ◽  
Vol 77 (1) ◽  
Author(s):  
Bernd A. Kniehl ◽  
Gustav Kramer ◽  
Ingo Schienbein ◽  
Hubert Spiesberger
Keyword(s):  
Finite Mass ◽  
Mass Effects

scholarly journals Back reaction of the gravitational radiation on the metric of spacetime

2018 ◽  
Vol 27 (07) ◽  
pp. 1850071
Author(s):  
A. A. Grib ◽  
Yu. V. Pavlov
Keyword(s):  
Black Holes ◽  
Energy Density ◽  
Gravitational Waves ◽  
Gravitational Radiation ◽  
Accretion Disc ◽  
Large Energy ◽  
Back Reaction

The problem of back reaction of the gravitational radiation of the two merging black holes on the metric of the spacetime is investigated. It is shown for some models that large energy density of the gravitational waves close to the merger can lead to the disappearance of the visible accretion disc of the merged pair of black holes.

scholarly journals Deconfining phase transition in a finite volume with massive particles: finite size and finite mass effects

2016 ◽  
Vol 94 (2) ◽  
pp. 180-187 ◽  
Author(s):  
L. Ghenam ◽  
A. Ait El Djoudi ◽  
K. Mezouar
Keyword(s):  
Phase Transition ◽  
Finite Volume ◽  
Size Effects ◽  
Finite Size ◽  
Gluon Plasma ◽  
Finite Mass ◽  
Finite Size Effects ◽  
Strange Quarks ◽  
Mass Effects ◽  
Thermally Driven

We study the deconfining phase transition from a hadronic gas phase consisting of massive pions to a quark–gluon plasma (QGP) phase containing gluons, massless up and down quarks, and massive strange quarks. The two phases are supposed to coexist in a finite volume, and the finite size effects are studied, in the two cases of thermally driven and density driven deconfining phase transitions. Finite-mass effects are also examined, then the color-singletness condition for the QGP is taken into account and finite size effects are investigated in this case also.

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