Strong Gravity News & Events

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VII Black Holes Workshop

Conference poster
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Venue
Physics Amphitheatre
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From astrophysics to high-energy physics, from information theory to quantum gravity, black holes have acquired an ever increasing role in fundamental physics, and are now part of the terminology of many important branches of observational, theoretical and mathematical physics. This workshop aims at bringing together experts about black holes in all their aspects. The fourth edition of the Black Holes Workshop will be held at the University of Aveiro in 18-19 December 2014.

Searching for the first super-massive black holes

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Speaker
Hugo Messias(Centro de Astronomia e Astrofísica da Universidade de Lisboa)
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GAP room
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Abstract: With the numerous pieces of evidence for the close evolution of super-massive black holes (SMBHs) and their host galaxies throughout the cosmic history, there has been a great effort to understand what drives such fact. One key point which could help achieve that goal is to observe the very first SMBHs in the early Universe and explore the initial conditions and what sets such co-evolution. This talk will guide you through the observational perspectives of this cosmic dance between SMBHs and their hosts, and the some alternative strategies to study them.

Simulating Accreting Binary Black Holes

Miguel Zilhão (Rochester Institute of Technology)
Speaker
Miguel Zilhão (Rochester Institute of Technology)
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GAP room
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Abstract: In this talk, we introduce the field of General Relativistic Magnetohydrodynamics (GRMHD) and give an overview on recent effort toward simulating and visualizing astrophysically realistic gas dynamics around compact binaries. In particular we motivate our group's approach, where a post-Newtonian expansion is used to construct an analytic spacetime, and we show preliminary results of circumbinary disks surrounding an equal-mass non-spinning black hole binary.

Warped AdS3 black holes: classical mode stability

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Hugo Ferreira (Nottingham U.)
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GAP room
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Abstract: (2+1)-dimensional gravity allows us to study aspects of classical and quantum gravity in a simpler technical setting which retains much of the conceptual complexity of the standard (3+1)-dimensional gravity. However, pure Einstein gravity lacks propagating degrees of freedom in 2+1 dimensions.