Mass and spin constraint on black holes in long GRBs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F20%3A00562243" target="_blank" >RIV/67985815:_____/20:00562243 - isvavai.cz</a>
Result on the web
<a href="https://www.pta.edu.pl/pliki/proc/vol10/v10p55.pdf" target="_blank" >https://www.pta.edu.pl/pliki/proc/vol10/v10p55.pdf</a>
DOI - Digital Object Identifier
—
Alternative languages
Result language
angličtina
Original language name
Mass and spin constraint on black holes in long GRBs
Original language description
We compute the evolution of a quasi-spherical, slowly rotating accretion flownaround a black hole, whose mass and spin evolve adequately to the mass-energyntransfer through the horizon. Our model is relevant for the central engine drivingna long gamma ray burst, that originates from the collapse of a massive star. Ournresults show how much mass and spin a newly formed black hole should possessnduring collapsar to launch long GRB.
Czech name
—
Czech description
—
Classification
Type
D - Article in proceedings
CEP classification
—
OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
<a href="/en/project/GJ17-06962Y" target="_blank" >GJ17-06962Y: Non-linear phenomena in a multi-channel astronomy of black holes</a><br>
Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2020
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Polish Astronomical Society Meeting /39./
ISBN
978-83-950430-8-6
ISSN
2545-1022
e-ISSN
—
Number of pages
3
Pages from-to
55-57
Publisher name
Polskie Towarzystwo Astronomiczne
Place of publication
Warszawa
Event location
Olsztyn
Event date
Sep 9, 2019
Type of event by nationality
EUR - Evropská akce
UT code for WoS article
—