W 2019

RAGtime 21: 16-20 September, 2019 - Workshop on Black Holes and Neutron Stars

ABRAMOWICZ, Marek, Stanislav HLEDÍK, Jiří KOVÁŘ, John MILLER, Petr SLANÝ et. al.

Základní údaje

Originální název

RAGtime 21: 16-20 September, 2019 - Workshop on Black Holes and Neutron Stars

Autoři

ABRAMOWICZ, Marek (616 Polsko, domácí), Stanislav HLEDÍK (203 Česká republika, domácí), Jiří KOVÁŘ (203 Česká republika, domácí), John MILLER (826 Velká Británie a Severní Irsko), Petr SLANÝ (203 Česká republika, domácí), Jan SCHEE (203 Česká republika, domácí), Zdeněk STUCHLÍK (203 Česká republika, domácí), Eva ŠRÁMKOVÁ (203 Česká republika, domácí), Gabriel TÖRÖK (203 Česká republika, garant, domácí) a Martin URBANEC (203 Česká republika, domácí)

Vydání

2019

Další údaje

Jazyk

angličtina

Typ výsledku

Uspořádání workshopu

Obor

10308 Astronomy

Stát vydavatele

Česká republika

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Kód RIV

RIV/47813059:19240/19:A0000584

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

Klíčová slova anglicky

black holes; neutron stars; relativistic astrophysics; compact objects; accretion discs; strong gravity; cosmology; X-ray cosmic missions

Příznaky

Mezinárodní význam
Změněno: 22. 3. 2020 22:30, RNDr. Jan Hladík, Ph.D.

Anotace

V originále

RAGtime - the series of the Relativistic Astrophysics Group workshops and proceedings – started in 1999 at Institute of Physics, the Faculty of Philosophy and Science of the Silesian University in Opava, Czech Republic. The 21th RAGtime workshop took place at the Silesian University in Opava, Czech Republic on September 16-20, 2019. The scientific focus of the workshop was traditionally devoted mainly to problems of relativistic physics of black holes and neutron or quark stars. Large attention was given to confronting theoretical models with up-to-date observations available through both electromagnetic and gravitational wave window to the Universe; to the modelling of astrophysical effects in the combined strong gravity and relevant external magnetic fields; and to current issues in accretion theory. Problems related to cosmology, mathematical aspects of the theory of relativity, and alternative theories of gravity was addressed also. In addition, new methods of generating complex general relativistic solutions containing a black hole was exposed. Last but not least, special focus was putted on national and international collaboration regarding the present and future cosmic X-ray missions. The invited speakers included: Hackmann, Eva (ZARM, University of Bremen); Kluźniak, Włodek (Nicolaus Copernicas Astronimcal Center, Warsaw, Poland); Karas, Vladimír (Astronomical Institute, Academy of Sciences of the Czech Republic, Prague, Czech Republic); Rueda, Jorge A. (ICRANet, Pescara, Italy; ICRA, Dipartimento di Fisica, Universita di Roma Sapienza, Rome, Italy and INAF, Istituto de Astrofisica e Planetologia Spaziali, Rome, Italy); Ruffini, Remo (ICRANet, Pescara, Italy; ICRA, Dipartimento di Fisica, Universita di Roma Sapienza, Rome, Italy and INAF, Rome, Italy); Wielgus, Maciek (Center for Astrophysics at Harvard & Smithsonian, Cambridge, Massachusetts, USA and Black Hole Initiative at Harvard University, Cambridge, Massachusetts, USA)