Zobrazeno 1 - 10
of 33
pro vyhledávání: '"K. Yugindro Singh"'
Publikováno v:
Chinese Journal of Physics. 83:579-598
Autor:
Sapam Gayatri Devi, I. Ablu Meitei, T. Ibungochouba Singh, Aheibam Keshwarjit Singh, K. Yugindro Singh
Publikováno v:
International Journal of Modern Physics A.
Quantum gravity effects on tunneling of fermions across the event horizon of rotating BTZ black hole
Publikováno v:
International Journal of Modern Physics A. 37
In this paper, the tunneling of fermions across the event horizon of rotating BTZ black hole is investigated by using Dirac equation in the presence of quantum gravity effects, WKB approximation and Feynman prescription. The tunneling probability and
Publikováno v:
International Journal of Theoretical Physics. 56:2640-2650
The correction of Hawking temperature of Schwarzschild-de Sitter (SdS) black hole is investigated using the generalized Klein-Gordon equation and the generalized Dirac equation by taking the quantum gravity effects into account. We derive the correct
Publikováno v:
International Journal of Astronomy and Astrophysics. :247-253
A study of the optical luminosity function of Quasi Stellar Objects (QSOs) and its evolution with redshift is carried out using the data from the Sloan Digital Sky Survey Data Release Seven (SDSS DR7). It is shown that the observed QSO luminosity fun
Autor:
K. Yugindro Singh, H. Shanjit
Publikováno v:
Advances in Astrophysics. 2
Autor:
A. Senorita Devi, K. Yugindro Singh
Publikováno v:
Astrophysics and Space Science. 354:535-540
The present paper aims to study the previously unstudied Chandra observed X-ray point sources of NGC 3384. While most of the point sources in NGC 3384 are hard X-ray binaries, we report here the discovery of a candidate Ultra-luminous X-ray source (U
Publikováno v:
Astrophysics and Space Science. 352:737-741
The entropy correction of Kerr-Newman black hole is investigated using the Hamilton-Jacobi method beyond semiclassical approximation. To get entropy correction, the inverse of the sum of square of event horizon (r+) and the square of rotational param
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Publikováno v:
Publications of The Korean Astronomical Society. 30:741-743
We have designed and built three cost eective observatories, in distinct models, which can house Schmidt { Cassegrain type small telescopes having aperture sizes up to 16 inches. Using the available small telescopes, we provided the people of Manipur