Explosive alpha capturing reactions at high temperature conditions in Astrophysics

dc.contributor.author	Bhattcharyya, A. B
dc.contributor.author	Duorah, K
dc.contributor.author	Duorah, H. L
dc.date.accessioned	2007-09-28T10:18:53Z
dc.date.available	2007-09-28T10:18:53Z
dc.date.issued	1996
dc.identifier.citation	BASI, Vol.24 No. 4 pp. 705-709	en
dc.identifier.uri	http://hdl.handle.net/2248/1842
dc.description.abstract	It has been recognized that C to the power 12 (alpha, gamma) O to the power 16 and O to the power 16 (alpha, gamma) Ne to the power 20 may proceed explosively at some stellar situation; more particularly at the outer layers of pre-supernova stage of stellar evolution. The effect of temperature on the mass of nuclei involved in these reactions are studied. Corrections for finite number size and nuclear surface energy are considered. There is a considerable change in the mass along with the temperature in the region considered. With these new mass, Q values for the reactions are calculated. With these new values, it is expected that reaction may proceed through some new levels. Reaction rate for capturing reactions are modified accordingly.	en
dc.format.extent	262630 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996BASI...24..705B	en
dc.subject	Pre-supernova	en
dc.subject	Explosive nucleosynthesis	en
dc.title	Explosive alpha capturing reactions at high temperature conditions in Astrophysics	en
dc.type	Article	en