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035 _a(RuTPU)RU\TPU\network\32994
090 _a661911
100 _a20200320a2019 k y0engy50 ba
101 0 _aeng
102 _aUS
135 _adrcn ---uucaa
181 0 _ai
182 0 _ab
200 1 _aComment on “Generalized near horizon extreme binary black hole geometry”
_fA. V. Galajinsky
203 _aText
_celectronic
300 _aTitle screen
320 _a[References: 12 tit.]
330 _aIt is demonstrated that the near–horizon geometry of two extreme Kerr black holes of equal mass, which are held finite distance apart by a massless strut, introduced recently in [Phys. Rev. D 100, 044033 (2019)], is a particular member of the near horizon Kerr–Bolt class.
461 _tPhysical Review D
_ocovering particles, fields, gravitation, and cosmology
463 _tVol. 100, iss. 12
_v[128501, 2 p.]
_d2019
610 1 _aэлектронный ресурс
610 1 _aтруды учёных ТПУ
610 1 _aчерные дыры
610 1 _aгоризонты
700 1 _aGalajinsky
_bA. V.
_cDoctor of Physical and Mathematical Sciences, Tomsk Polytechnic University (TPU), Department of Higher Mathematics and Mathematical Physics of the Institute of Physics and Technology (HMMPD IPT)
_cProfessor of the TPU
_f1971-
_gAnton Vladimirovich
_2stltpush
_3(RuTPU)RU\TPU\pers\27878
712 0 2 _aНациональный исследовательский Томский политехнический университет
_bИсследовательская школа физики высокоэнергетических процессов
_c(2017- )
_h8118
_2stltpush
_3(RuTPU)RU\TPU\col\23551
801 2 _aRU
_b63413507
_c20210316
_gRCR
856 4 _uhttp://earchive.tpu.ru/handle/11683/64791
856 4 _uhttps://doi.org/10.1103/PhysRevD.100.128501
942 _cCF