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Equations of motion of a spinning relativistic particle in external fields. / Pomeranskiǐ, A. A.; Khriplovich, I. B.

In: Journal of Experimental and Theoretical Physics, Vol. 86, No. 5, 01.01.1998, p. 839-849.

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Harvard

Pomeranskiǐ, AA & Khriplovich, IB 1998, 'Equations of motion of a spinning relativistic particle in external fields', Journal of Experimental and Theoretical Physics, vol. 86, no. 5, pp. 839-849. https://doi.org/10.1134/1.558554

APA

Pomeranskiǐ, A. A., & Khriplovich, I. B. (1998). Equations of motion of a spinning relativistic particle in external fields. Journal of Experimental and Theoretical Physics, 86(5), 839-849. https://doi.org/10.1134/1.558554

Vancouver

Pomeranskiǐ AA, Khriplovich IB. Equations of motion of a spinning relativistic particle in external fields. Journal of Experimental and Theoretical Physics. 1998 Jan 1;86(5):839-849. https://doi.org/10.1134/1.558554

Author

Pomeranskiǐ, A. A. ; Khriplovich, I. B. / Equations of motion of a spinning relativistic particle in external fields. In: Journal of Experimental and Theoretical Physics. 1998 ; Vol. 86, No. 5. pp. 839-849.

BibTeX

@article{63972011d0a34adfa9a6749560e21029,
title = "Equations of motion of a spinning relativistic particle in external fields",
abstract = "We consider the motion of a spinning relativistic particle in external electromagnetic and gravitational fields to first order in the external field but to arbitrary order in the spin. The influence of the spin on the particle trajectory is properly accounted for by describing the spin noncovariantly. Specific calculations are performed through second order in the spin. A simple derivation is presented for the gravitational spin-orbit and spin-spin interactions of a relativistic particle. We discuss the gravimagnetic moment (GM), a particular spin effect in general relativity. We show that for a Kerr black hole the gravimagnetic ratio, i.e., the coefficient of the GM, equals unity (just as the gyromagnetic ratio equals 2 for a charged Kerr hole). The equations of motion obtained for a spinning relativistic particle in an external gravitational field differ substantially from the Papapetrou equations.",
author = "Pomeranskiǐ, {A. A.} and Khriplovich, {I. B.}",
year = "1998",
month = jan,
day = "1",
doi = "10.1134/1.558554",
language = "English",
volume = "86",
pages = "839--849",
journal = "Journal of Experimental and Theoretical Physics",
issn = "1063-7761",
publisher = "МАИК {"}Наука/Интерпериодика{"}",
number = "5",

}

RIS

TY - JOUR

T1 - Equations of motion of a spinning relativistic particle in external fields

AU - Pomeranskiǐ, A. A.

AU - Khriplovich, I. B.

PY - 1998/1/1

Y1 - 1998/1/1

N2 - We consider the motion of a spinning relativistic particle in external electromagnetic and gravitational fields to first order in the external field but to arbitrary order in the spin. The influence of the spin on the particle trajectory is properly accounted for by describing the spin noncovariantly. Specific calculations are performed through second order in the spin. A simple derivation is presented for the gravitational spin-orbit and spin-spin interactions of a relativistic particle. We discuss the gravimagnetic moment (GM), a particular spin effect in general relativity. We show that for a Kerr black hole the gravimagnetic ratio, i.e., the coefficient of the GM, equals unity (just as the gyromagnetic ratio equals 2 for a charged Kerr hole). The equations of motion obtained for a spinning relativistic particle in an external gravitational field differ substantially from the Papapetrou equations.

AB - We consider the motion of a spinning relativistic particle in external electromagnetic and gravitational fields to first order in the external field but to arbitrary order in the spin. The influence of the spin on the particle trajectory is properly accounted for by describing the spin noncovariantly. Specific calculations are performed through second order in the spin. A simple derivation is presented for the gravitational spin-orbit and spin-spin interactions of a relativistic particle. We discuss the gravimagnetic moment (GM), a particular spin effect in general relativity. We show that for a Kerr black hole the gravimagnetic ratio, i.e., the coefficient of the GM, equals unity (just as the gyromagnetic ratio equals 2 for a charged Kerr hole). The equations of motion obtained for a spinning relativistic particle in an external gravitational field differ substantially from the Papapetrou equations.

UR - http://www.scopus.com/inward/record.url?scp=33744673821&partnerID=8YFLogxK

U2 - 10.1134/1.558554

DO - 10.1134/1.558554

M3 - Article

AN - SCOPUS:33744673821

VL - 86

SP - 839

EP - 849

JO - Journal of Experimental and Theoretical Physics

JF - Journal of Experimental and Theoretical Physics

SN - 1063-7761

IS - 5

ER -

ID: 36646021