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Strong Gravity News & Events

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New class of rotating charged black holes in the external Bertotti-Robinson (electro)magnetic field

GGD - Gr@V Seminar
Speaker
Hryhorii Ovcharenko (Charles University, Faculty of Mathematics and Physics, Institute of Theoretical Physics)
Event date
Venue
Hybrid: Sala Sousa Pinto and Teams
Event Website
Event type

We present a large family of twisting and expanding solutions to the Einstein-Maxwell equations of algebraic type D, for which the two double principal null directions (PNDs) of the Weyl tensor are not aligned with the null eigendirections of the Faraday tensor. In addition to systematically deriving this new class, we present its various metric forms and convenient parameterizations.

On the Thermodynamics of Deformed Black Holes

GGD - Gr@V Seminar
Speaker
Maryem Jemri (Mohammed V University of Rabat, Morocco)
Event date
Venue
Hybrid: Sala 11.2.21 and Teams
Event Website
Event type

Inspired by noncommutative geometry in string theory, we introduce extended derivatives in black hole physics by incorporating a real antisymmetric rank-2 tensor, exhibiting similarities with certain string-theoretic fields.

O(3) boson stars and hairy black holes

GGD - Gr@V Seminar
Speaker
Yasha Shnir (Dubna)
Event date
Venue
Hybrid: Sala Sousa Pinto and Teams
Event Website
Event type

We present and study new nontopological soliton solutions in the U(1) gauged nonlinear O(3) sigma-model with a symmetry breaking potential in 3+1 dimensional space-time. The configurations are endowed with an electric and magnetic field and also carry a nonvanishing angular momentum density.

Squeezing solution generating techniques: A road to enlarge the spectrum of exact vacuum solutions in GR and to construct dynamical primordial objects.

GGD - Gr@V Seminar
Speaker
Adolfo Cisterna (Institute of Theoretical Physics, Charles University)
Event date
Venue
Hybrid: Sala Sousa Pinto and Teams
Event Website
Event type

This talk presents two distinct problems in gravitational physics that are connected through the use of solution-generating techniques within Einstein–Maxwell–scalar theory. First, we construct new vacuum solutions of Einstein’s equations starting from electrovacuum configurations embedded in external electromagnetic backgrounds.