scholarly journals Quantum Gravitational Applications of Nuclear, Atomic and Astrophysical Phenomena

Author(s):  
U. V. S. SESHAVATHARAM ◽  
S. LAKSHMINARAYANA
2018 ◽  
Vol 189 (08) ◽  
pp. 785-802 ◽  
Author(s):  
Rafail L. Aptekar ◽  
Andrei M. Bykov ◽  
Sergei V. Golenetskii ◽  
Dmitrii D. Frederiks ◽  
Dmitry S. Svinkin ◽  
...  

In this review, we consider some of the effects which might occur in astrophysical phenomena as a result of possible electromagnetic interactions of neutrinos, and of the hypothetical electron-neutrino interaction.


1998 ◽  
Vol 188 ◽  
pp. 402-403
Author(s):  
Y. Tajima ◽  
J. Fukue

The accretion disks are now supposed to be the main driving source of the active astrophysical phenomena. Even the electron-positron pair plasma will be created at the surface of the sufficiently luminous disk. While the effect of radiation drag which causes in the intense radiation fields around the accretion disk is examined recently. Then, we numerically consider the radiative accelerated pair-winds, which blow off from central luminous accretion disk surrounding a black hole, taking into account radiation drag of the order of v/c.


2004 ◽  
Author(s):  
Anton S. Konkin ◽  
Vadim V. Zhmailo ◽  
Rostislav A. Orlov ◽  
Alexander E. Lakhtikov ◽  
Alexander P. Morovov

2017 ◽  
Vol 95 (1) ◽  
pp. 68-71 ◽  
Author(s):  
B. N. Chetverushkin ◽  
N. D’Ascenzo ◽  
A. V. Saveliev ◽  
V. I. Saveliev

2011 ◽  
Vol 7 (S285) ◽  
pp. 29-34 ◽  
Author(s):  
Jonathan Grindlay ◽  
Sumin Tang ◽  
Edward Los ◽  
Mathieu Servillat

AbstractThe large-scale surveys such as PTF, CRTS and Pan-STARRS-1 that have emerged within the past 5 years or so employ digital databases and modern analysis tools to accentuate research into Time Domain Astronomy (TDA). Preparations are underway for LSST which, in another 6 years, will usher in the second decade of modern TDA. By that time the Digital Access to a Sky Century @ Harvard (DASCH) project will have made available to the community the full sky Historical TDA database and digitized images for a century (1890–1990) of coverage. We describe the current DASCH development and some initial results, and outline plans for the “production scanning” phase and data distribution which is to begin in 2012. That will open a 100-year window into temporal astrophysics, revealing rare transients and (especially) astrophysical phenomena that vary on time-scales of a decade. It will also provide context and archival comparisons for the deeper modern surveys.


2008 ◽  
Author(s):  
Ding-Xiong Wang ◽  
Yong-Chun Ye ◽  
Chang-Yin Huang ◽  
Zhao-Ming Gan ◽  
Ye-Fei Yuan ◽  
...  

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