The Effect of the Triple-α Reaction Rate on Stellar Evolution at Low-Metallicity

Details The Effect of the Triple-α Reaction Rate on Stellar Evolution at Low-Metallicity The Effect of the Triple-α Reaction Rate on Stellar Evolution at Low-Metallicity

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1238..122s&link_type=abstract

TOURS SYMPOSIUM ON NUCLEAR PHYSICS AND ASTROPHYSICS-VII. AIP Conference Proceedings, Volume 1238, pp. 122-125 (2010).

Physics

Nuclear Physics

Star Formation, Brightness, Stars, Stellar Mass, Star Formation, Luminosity And Mass Functions, Population Ii Stars, Masses

Scientific paper

We investigate the effect of the triple-α reaction rates on the evolution of low-mass stars and massive stars. The former is compared with the observations of metal-poor stars known to date. For the latter, we discuss the impact of recent calculation of triple-α reaction rate by Ogata et al. (2009, PTP, 122, 1055) on the evolution until carbon burning.

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