Possible gravitational radiation detection using the geometric phase of a light beam

Mitskievich, Nikolai V.; Nesterov, Alexander I.

doi:10.1007/bf02107934

Cited by 7 publications

(10 citation statements)

References 11 publications

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“…Mitskievich et al [37] investigated Berry's phase shift of a monochromatic EM wave beam in a plane monochromatic GW field, and it is shown that (a) For parallel the propagating GW and EM wave, the phase shift is absent. (b) When the both waves are mutually orthogonal, the nonvanishing phase shift will be produced, and the phase shift is proportional to the distance propagated by the EM wave (see, Eq.…”

Section: Geometrical Phase Shift Produced By the High-frequency Relic...mentioning

confidence: 99%

Electromagnetic response of a Gaussian beam to high-frequency relic gravitational waves in quintessential inflationary models

2003

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Maximal signal and peak of high-frequency relic gravitational waves (GW's), recently expected by quintessential inflationary models, may be firmly localized in the GHz region, the energy density of the relic gravitons in critical units (i.e., h 2 0 Ω GW ) is of the order 10 −6 , roughly eight orders of magnitude larger than in ordinary inflationary models. This is just right best frequency band of the electromagnetic (EM) response to the high-frequency GW's in smaller EM detecting systems. We consider the EM response of a Gaussian beam passing through a static magnetic field to a high-frequency relic GW. It is found that under the synchroresonance condition, the first-order perturbative EM power fluxes will contain "left circular wave" and "right circular wave" around the symmetrical axis of the Gaussian beam, but the perturbative effects produced by the states of + polarization and × polarization of the relic GW have different properties, and the perturbations on behavior are obviously different from that of the background EM fields in the local regions. For the high-frequency relic GW with the typical parameters ν g = 10 10 Hz, h = 10 −30 in the quintessential inflationary models, the corresponding perturbative photon flux passing through the region 10 −2 m 2 would be expected to be 10 3 s −1 . This is largest perturbative photon flux we recently analyzed and estimated using the typical laboratory parameters. In addition, we also discuss geometrical phase shift generated by the high-frequency relic GW in the Gaussian beam and estimate possible physical effects.

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Section: Geometrical Phase Shift Produced By the High-frequency Relic...mentioning

confidence: 99%

Electromagnetic response of a Gaussian beam to high-frequency relic gravitational waves in quintessential inflationary models

2003

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“…The thermal motion of plasma of stars, the interaction of the EM waves with interstellar plasma and magnetic fields, the evaporation of primordial black holes [8], even ultra-high-intensity lasers [9] and other highenergy laboratory schemes [10,11,12] are possible means to generate the HFGWs in the GHz band and higher frequencies. Interaction of the HFGWs with the EM fields and the EM detection of the HFGWs have been theoretically and experimentally studied by many authors [13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28,29,30,31,32,33,34,35,36,37,38].These works include the gravitation-EM conversion in the static EM fields(e.g., the Gertsenshtein effect and its inverse effect), the cavity classical-and cavity quantum-electrodynamical response to the HFGWs, resonant photon-graviton conversion, Barry's phase in the EM detection of the HFGWs, resonant interaction of the HFGWs with the EM wave beams, the rotation of the polarization vector of EM wave caused by the HFGWs in the toroidal waveguide, the difference frequency resonant response of coupled spherical cavities, etc.…”

Section: Introductionmentioning

confidence: 99%

Perturbative photon fluxes generated by high-frequency gravitational waves and their physical effects

Baker²,

Fang

et al. 2008

Eur. Phys. J. C

115

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We consider the electromagnetic (EM) perturbative effects produced by the high-frequency gravitational waves (HFGWs) in the GHz band in a special EM resonance system, which consists of fractal membranes, a Gaussian beam (GB) passing through a static magnetic field.It is predicted, under the synchroresonance condition, coherence modulation of the HFGWs to the preexisting transverse components of the GB produces the transverse perturbative photon flux (PPF),which has three novel and important properties: (1)The PPF has maximum at a longitudinal symmetrical surface of the GB where the transverse background photon flux (BPF) vanishes; (2) the resonant effect will be high sensitive to the propagating directions of the HFGWs; (3) the PPF reflected or transmitted by the fractal membrane exhibits a very small decay compared with very large decay of the much stronger BPF. Such properties might provide a new way to distinguish and display the perturbative effects produced by the HFGWs. We also discuss the high-frequency asymptotic behavior of the relic GWs in the microwave band and the positive definite issues of their energy-momentum pseudo-tensor .

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“…As a comoving reference frame we choose the reference frame of a single observer [15]. This reference frame is determined by the motion of a single mass point.…”

Section: Comoving Reference Framementioning

confidence: 99%

“…For a nonrotating frame (i.e. when the vectors h (n) i are displaced along the basis line (2) according to the Fermi-Walker transport) the quantities {X (α) , cτ} correspond to the Fermi normal coordinates (see for instance [14,15,16]). Analogous quantities…”

Section: Comoving Reference Framementioning

confidence: 99%

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The Equations of Motion of Compact Binaries in the Neighborhood of Supermassive Black Hole

Gorbatsievich

Bobrik

Ruffini³

et al. 2010

AIP Conference Proceedings

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Abstract. By the use of Einstein-Infeld-Hoffmann method, the equations of motion of a binary star system in the field of a supermassive black hole are derived. In spite of the fact that the motion of a binary system as a whole can be relativistic or even ultra-relativistic with respect to the supermassive black hole, it is shown, that under the assumption of non-relativistic relative motion of the stars in binary system, the motion of the binary system as a whole satisfies the Mathisson-Papapetrou equations with additional terms depending on quadrupole moments. Exemplary case of ultrarelativistic motion of a binary neutron star in the vicinity of non-rotating black hole is considered. It it shown that the motion of binary's center of mass may considerably differ from geodesic motion.

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Possible gravitational radiation detection using the geometric phase of a light beam

Cited by 7 publications

References 11 publications

Electromagnetic response of a Gaussian beam to high-frequency relic gravitational waves in quintessential inflationary models

Electromagnetic response of a Gaussian beam to high-frequency relic gravitational waves in quintessential inflationary models

Perturbative photon fluxes generated by high-frequency gravitational waves and their physical effects

The Equations of Motion of Compact Binaries in the Neighborhood of Supermassive Black Hole

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