Spherical mechanics for a particle near the horizon of extremal black hole
| Parent link: | Physics of Particles and Nuclei Letters.— , 2004- Vol. 11, iss. 7.— 2014.— [P. 890-893] |
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| Muut tekijät: | , |
| Yhteenveto: | Title screen We describe canonical transformation, which links the Hamiltonian of a massive relativistic particle moving near the horizon of an extremal black hole to the conventional form of the conformal mechanics. Thus, like the non-relativistic conformal mechanics, the investigation of the particle dynamics reduces to analyzing its “spherical sector” defined by the Casimir element of the conformal algebra. We present a detailed list of such systems originating from various types of black hole configurations. Режим доступа: по договору с организацией-держателем ресурса |
| Kieli: | englanti |
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2014
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| Linkit: | http://dx.doi.org/10.1134/S154747711407019X |
| Aineistotyyppi: | Elektroninen Kirjan osa |
| KOHA link: | https://koha.lib.tpu.ru/cgi-bin/koha/opac-detail.pl?biblionumber=641519 |
| Yhteenveto: | Title screen We describe canonical transformation, which links the Hamiltonian of a massive relativistic particle moving near the horizon of an extremal black hole to the conventional form of the conformal mechanics. Thus, like the non-relativistic conformal mechanics, the investigation of the particle dynamics reduces to analyzing its “spherical sector” defined by the Casimir element of the conformal algebra. We present a detailed list of such systems originating from various types of black hole configurations. Режим доступа: по договору с организацией-держателем ресурса |
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| DOI: | 10.1134/S154747711407019X |