BAKALA, Pavel, Stanislav HLEDÍK a Zdeněk STUCHLÍK. Extreme gravitational lensing in vicinity of Schwarzschild-de Sitter black holes. CENTRAL EUROPEAN JOURNAL OF PHYSICS. DE - Spolková republika Německo, roč. 5, č. 4, s. 599-610. ISSN 1895-1082. doi:10.2478/s11534-007-0033-6. 2007.
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Základní údaje
Originální název Extreme gravitational lensing in vicinity of Schwarzschild-de Sitter black holes
Název anglicky Extreme gravitational lensing in vicinity of Schwarzschild-de Sitter black holes
Autoři BAKALA, Pavel, Stanislav HLEDÍK a Zdeněk STUCHLÍK.
Vydání CENTRAL EUROPEAN JOURNAL OF PHYSICS, DE - Spolková republika Německo, 2007, 1895-1082.
Další údaje
Typ výsledku Článek v odborném periodiku
Obor 10308 Astronomy
Utajení není předmětem státního či obchodního tajemství
Organizační jednotka Filozoficko-přírodovědecká fakulta v Opavě
Doi http://dx.doi.org/10.2478/s11534-007-0033-6
UT WoS 000251320600014
Klíčová slova anglicky black holes, cosmological constant, gravitational lensing, visualization, numerical relativity
Štítky UF
Příznaky Mezinárodní význam, Recenzováno
Návaznosti LC06014, projekt VaV. MSM4781305903, záměr.
Změnil Změnila: Mgr. Pavlína Jalůvková, učo 25213. Změněno: 8. 12. 2020 14:00.
Anotace
We have developed a realistic, fully general relativistic computer code to simulate optical projection in a strong, spherically symmetric gravitational field. The standard theoretical analysis of optical projection for an observer in the vicinity of a Schwarzschild black hole is extended to black hole spacetimes with a repulsive cosmological constant, i.e, Schwarzschild de Sitterspacetimes. Influence of the cosmological constant is investigated for static observers and observers radially free-falling from the static radius. Simulations include efects of the gravitational lensing, multiple images, Doppler and gravitational frequency shift, as well as the intensity amplification. The code generates images of the sky for the static observer and a movie simulations of the changing sky for the radially free-falling observer.
Anotace anglicky
We have developed a realistic, fully general relativistic computer code to simulate optical projection in a strong, spherically symmetric gravitational field. The standard theoretical analysis of optical projection for an observer in the vicinity of a Schwarzschild black hole is extended to black hole spacetimes with a repulsive cosmological constant, i.e, Schwarzschild de Sitterspacetimes. Influence of the cosmological constant is investigated for static observers and observers radially free-falling from the static radius. Simulations include efects of the gravitational lensing, multiple images, Doppler and gravitational frequency shift, as well as the intensity amplification. The code generates images of the sky for the static observer and a movie simulations of the changing sky for the radially free-falling observer.
VytisknoutZobrazeno: 20. 4. 2024 07:33