Generalizations of the Kerr-Newman solution Print E-mail

We search for approximate and exact solutions of the Einstein-Maxwell field equations that can be used to describe the interior and exterior gravitational and electromagnetic fields of relativistic compact objects such as white dwarfs, neutron stars and black holes. In particular, we are interested in generalizations of the Kerr-Newman solution that include higher-order multipole moments.

• Quadrupolar solutions

• Matching conditions

• Physical properties
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Group leader: Prof. Hernando Quevedo

In collaboration with:
M. Abishev (KazNU), E. Bayona (UNAM), N. Beisen (KazNU), F. Belissarova (KazNU), K. Boshkayev (KazNU), F. Frutos-Alfaro (UCR), A.C. Gutíerrez-Piñeres (UIS), R. Kerr (ICRANet), C. Lämmerzahl (UB), O. Luongo (INFN), A. Mansurova (KazNU), A. Muratkhan (KazNU), V. Perlick (UB), D. Phillip (UB), D. Pugliese (SU), W. Pulido (UNC), R. Ruffini (ICRANet), A. Sánchez (UNAM), P. Sánchez (UNAM), S. Toktarbay (KazNU), S. Vargas-Serdio (UNAM).

INFN: Istituto Nazionale di Fisica Nucleare
KazNU: Kazakh National University
SU: Slezská univerzita v OpavÄ›
UB: Universität Bremen
UCR: Universidad de Costa Rica
UIS: Universidad Industrial de Santander
UNAM: Universidad Nacional Autónoma de México
UNC: Universidad Nacional de Colombia
 
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