Dr. Rajesh S.R. is Assistant Professor and Research Supervisor at the Post Graduate Department of Physics and Research Centre, Sanatana Dharma College. He has over 10 years of experience teaching at the undergraduate and postgraduate levels. A Post-Graduate from the Indian Institute of Technology, Roorkee, he was awarded Junior and Senior Research Fellowships by UGC-CSIR. Dr. Rajesh S.R. earned his Doctoral Degree from Indian Institute of Science (IISc), Bangalore (2011), pursuing research in Astrophysical Thermodynamics. He has been a Visiting Associate at IUCAA, Pune, since 2014.
Astrophysical Hydrodynamics
(1) “Transition of accretion flow from Keplerian phase to advective phase as a dynamical system ”, S. R. Rajesh & S. B. Rakesh Chandran , MNRAS 452, 3346–3356 , 2015.
(2) “SEP events and wake region lunar dust charging with grain radii”, S.B. Rakesh Chandran, S.R. Rajesh, A. Abraham, G. Renuka, Chandu Venugopal, Advances in Space Research 59 (2017) 483–489
(3)“Time varaibility of viscosity parameter in differentially rotating disc” Rajesh,S. R & Nishant K. Singh, 2014, NewAstronomy, 30, 38-45.
(4)“Weakly non-linear stability of hydrodynamic accretion disc” Rajesh, S. R., 2011, MNRAS, 414, 691-701.
(5) “Two-temperature accretion around rotating black holes: a description of the general advective flow paradigm in the presence of various cooling processes to explain low to high luminous sources”, Rajesh, S. R. & Mukhopadhyay, Banibrat 2010, MNRAS, 402..961R.
(6)“Two temperature viscous accretion flows around rotating black holes: Description of underfed systems to ultra-luminous X-ray sources”,Rajesh, S. R. & Mukhopadhyay, Banibrat, 2010, NewAstronomy,15..283R.
(7)“Transition from radiatively inefficient to cooling dominated phase in two temperatur eaccretion disks around black holes” Sinha, Monika; Rajesh, S. R. & Mukhopadhyay, Banibrat, 2009, RAA,9.1331S.