Action-angle variables for the particle near extreme Kerr throat

Détails bibliographiques
Parent link:Modern Physics Letters A: Scientific Journal
Vol. 27, iss. 32.— 2012.— [1250191 р. 11]
Auteur principal: Bellucci S. Stefano
Autres auteurs: Nersessian A. P. Armen Petrosovich, Yeghikyan V. Vahagn
Résumé:Title screen
We construct the action-angle variables for the spherical part of conformal mechanics describing the motion of a particle near extreme Kerr throat. We indicate the existence of the critical point |pφ|=mcRSch (with m being the mass of the particle, c denoting the speed of light, RSch=2γM/c2 being the Schwarzschild radius of a black hole with mass M, and γ denoting the gravitational constant), where these variables are expressed in terms of elementary functions. Away from this point the action-angle variables are defined by elliptic integrals. The proposed formulation allows one to easily reconstruct the whole dynamics of the particle both in initial coordinates, as well as in the so-called conformal basis, where the Hamiltonian takes the form of conventional non-relativistic conformal mechanics. The related issues, such as semiclassical quantization and supersymmetrization are also discussed.
Режим доступа: по договору с организацией-держателем ресурса
Langue:anglais
Publié: 2012
Sujets:
Accès en ligne:http://dx.doi.org/10.1142/S021773231250191X
http://arxiv.org/abs/1112.4713
Format: Électronique Chapitre de livre
KOHA link:https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=641458

MARC

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200 1 |a Action-angle variables for the particle near extreme Kerr throat  |f S. Bellucci , A. P. Nersessian, V. Yeghikyan 
203 |a Text  |c electronic 
300 |a Title screen 
320 |a [References: 24 tit.] 
330 |a We construct the action-angle variables for the spherical part of conformal mechanics describing the motion of a particle near extreme Kerr throat. We indicate the existence of the critical point |pφ|=mcRSch (with m being the mass of the particle, c denoting the speed of light, RSch=2γM/c2 being the Schwarzschild radius of a black hole with mass M, and γ denoting the gravitational constant), where these variables are expressed in terms of elementary functions. Away from this point the action-angle variables are defined by elliptic integrals. The proposed formulation allows one to easily reconstruct the whole dynamics of the particle both in initial coordinates, as well as in the so-called conformal basis, where the Hamiltonian takes the form of conventional non-relativistic conformal mechanics. The related issues, such as semiclassical quantization and supersymmetrization are also discussed. 
333 |a Режим доступа: по договору с организацией-держателем ресурса 
461 |t Modern Physics Letters A  |o Scientific Journal 
463 |t Vol. 27, iss. 32  |v [1250191 р. 11]  |d 2012 
610 1 |a электронный ресурс 
610 1 |a труды учёных ТПУ 
700 1 |a Bellucci  |b S.  |g Stefano 
701 1 |a Nersessian  |b A. P.  |c physicist  |c Professor of Tomsk Polytechnic University  |f 1964-  |g Armen Petrosovich  |3 (RuTPU)RU\TPU\pers\34605  |9 17967 
701 1 |a Yeghikyan  |b V.  |g Vahagn 
801 2 |a RU  |b 63413507  |c 20150520  |g RCR 
856 4 |u http://dx.doi.org/10.1142/S021773231250191X 
856 4 |u http://arxiv.org/abs/1112.4713 
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