Dilatonic dyon black hole solutions

Dilatonic black hole dyon solutions with an arbitrary dilatonic coupling constant λ ≠ 0 and canonical sign ε = +1 for the scalar field kynetic term are considered. These solutions are defined up to solutions of two master equations for moduli functions. For λ ≠ 1/2 the solutions are extended to ε = ±1, where ε = -1 corresponds to a ghost (phantom) scalar field. Some physical parameters of the solutions: gravitational mass, scalar charge, Hawking temperature, black hole area entropy and parametrized post-Newtonian (PPN) parameters β and γ are obtained. It is shown that PPN parameters do not depend on scalar field coupling λ and ε. Two groups of bounds on gravitational mass and scalar charge (for a fixed and arbitrary extremality parameter μ > 0) are found by using a certain conjecture on parameters of solutions when1 + 2λ2ε > 0. These bounds are verified numerically for certain examples. Using the product we are led to the well-known lower bound on mass which was obtained earlier by Gibbons, Kastor, London, Townsend and Traschen by using spinor techniques. © 2015 IOP Publishing Ltd.

Авторы
Abishev M.E. 1, 2 , Boshkayev K.A.1, 2 , Dzhunushaliev V.D.1, 2 , Ivashchuk V.D. 3, 4
Номер выпуска
16
Язык
Английский
Статус
Опубликовано
Номер
165010
Том
32
Год
2015
Организации
  • 1 IETP, Al-Farabi KazNU, Almaty, 050040, Kazakhstan
  • 2 Physical and Technical Faculty, Al-Farabi Kazakh National University, al'-Farabi St. 71, Almaty, 050040, Kazakhstan
  • 3 Center for Gravitation and Fundamental Metrology, VNIIMS, Ozyornaya St. 46, Moscow, 119361, Russian Federation
  • 4 Institute of Gravitation and Cosmology, Peoples' Friendship University of Russia, Miklukho-Maklaya St. 6, Moscow, 117198, Russian Federation
Ключевые слова
black holes; dyon; mass bounds
Дата создания
19.10.2018
Дата изменения
19.10.2018
Постоянная ссылка
https://repository.rudn.ru/ru/records/article/record/4527/