Thermonuclear reactions in stars

Stars as thermonuclear reactors: their fuels and ashes -- A. Ray, Lecture Notes on Nuclear Astrophysics at the Fifth SERC School on Nuclear Physics at Panjab University, Chandigarh Feb-Mar, 2002 to be published (2003).

Neutrinos from stellar collapse and explosion

Neutrino Spectroscopy of the Early Phase of Nearby Supernovae - F.K. Sutaria \& A. Ray, Phys. Rev. Letters, 79, 1599, (1997).

Oscillation effects on Neutrinos from the early phase of a nearby Supernova - D. Majumdar, A. Raychaudhury, K. Kar, A. Ray, F.K. Sutaria, Int. J. Mod. Phys. A15, 2105 (2000).

Discussion on a possible neutrino detector located in India -- M.V.N. Murthy,..., N. K. Mondal, J. Learned, A. Ray and 23 others, in Procs of Workshop on High Energy Particle Physics - Pramana 54, 347 (2000).

Neutrino inelastic scattering and prompt shocks in core bounce supernovae - A. Ray, in ``Supernovae", ed S. E. Woosley, p362 (Springer Verlag, 1991).

Beta decay, electron capture and weak reactions in presupernova and core collapse

Centroids of Gamow-Teller transitions at finite temperature in fp-shell neutron-rich nuclei - O. Civitarese and A. Ray, Physica Scripta 59, 352 (1999).

Half-lives and pre-supernova weak interaction rate for nuclei far away from the stability line - K.Kar, S.Chakravarti, A.Ray and S.Sarkar, Jour. Phys. G, 24, 1641 (1998) (nucl-th/9806082).

Weak interaction rates for nuclei in presupernova stars - A. Ray, K. Kar, S. Sarkar and S. Chakravarti in Proc. of the IAU Colloquium No 145 on Supernovae and Supernova Remnants, Xian, China (ed. R. McCray and Z. Wang, 1996).

Beta decay rates of fp shell nuclei with A $>$ 60 in massive stars at presupernova stage - K. Kar, A. Ray and S. Sarkar Ap. J. 434, 662, (1994).

Beta decay rates of fp shell nuclei in advanced evolutionary stages of presuepernova stars - K. Kar, S. Sarkar and A. Ray, Physics Letters B261, 217 (1991); erratum: Phys Lett B277, 528 (1992).

Electron capture supernovae: One zone collapse calculation for stars with masses 10 M$_{\odot}$ and 15 M$_{\odot}$ - A. Ray, S.M. Chitre and K. Kar, Astrophys. J. 285 , 766 (1984).