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Research Groups and Staff
Research Groups Staff
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International Physics Course
General-relativistic astrophysics
Research Interests
1.
Numerical simulations in General Relativity.
2.
Equation of state of compact stellar objects.
3.
Central engines of gamma-ray bursts:
accretion discs around black holes, magnetic instabilities, jet formation.
4.
Sources of gravitational waves:
binary compact objects (neutron stars, black holes), deformed compact stars.
Introduction to the research interests

The study of compact objects, like (binary) black holes, (binary) neutron stars, their mergers and subsequent formation of a single compact object surrounded by an accretion disk are very important for contemporary astrophysics (and physics) for several reasons. Binary neutron-star systems are particularly interesting, because they are the best candidate source for explaining a class of gamma-ray bursts, which are in general the most energetic explosions in the Universe. Gamma-ray bursts are observed daily by satellites and telescopes, but their origin and mechanism is not known in detail.
Binary neutron-star and/or black-hole systems are also powerful sources of gravitational radiation. Gravitational waves are a fundamental prediction of General Relativity and, after huge experimental efforts worldwide especially with laser interferometric detectors, have been measured for the first time only recently: the first binary black-hole merger in September 2015 and the first binary neutron-star merger in August 2017. The measurement of gravitational waves has opened a completely new observational window on the Universe, through which we will get to know things that are completely or partially inaccessible to electromagnetic observations, like black-hole dynamics, the internal structure of compact stars, the equation of state of ultra-high density matter, and so on, in addition to the internal engine of gamma-ray bursts, as mentioned above.
These measurements were performed by interferometers in the US (LIGO) and Italy (Virgo), while in Japan the KAGRA detector is currently being built.
In order to physically interpret the measurements, accurate knowledge of gravitational waveforms is of crucial importance and hence numerical simulations of the sources are necessary. Given the high nonlinearity of the Einstein equations for General Relativity, numerical solutions are in fact often the only means to study the internal structure and the most violent dynamics of such objects in detail.

Luca Baiotti is currently part of the OUTAP group (Osaka University Theoretical AstroPhysics group) in the Department of Earth and Space Science. Prospective students, in particular, are invited to look at the web pages of the OUTAP group.

Rest-mass density and magnetic-field lines of a black hole surrounded by a disc, a system produced by the merger of binary neutron stars.

Gravitational waveforms of binary neutron-star coalescence, merger, and post-merger.