Context: Ogata et al. (2009; hereafter OKK) presented a theoretical determination of the triple-alpha nuclear reaction rate. Their rate differs from the NACRE rate by many orders of magnitude at temperatures relevant for low mass stars. Aims: We explore the evolutionary implications of adopting the OKK triple-alpha reaction rate in low mass stars and compare the results with those obtained using the NACRE rate. Methods: The triple-alpha reaction rates are compared by following the evolution of stellar models at 1 and 1.5 Msol with Z=0.0002 and Z=0.02. Results: Results show that the OKK rate has severe consequences for the late stages of stellar evolution in low mass stars. Most notable is the shortening--or disappearance--of the red giant phase. Conclusions: The OKK triple-alpha reaction rate is incompatible with observations of extended red giant branches and He burning stars in old stellar systems.
@article{arxiv.0905.2397,
title = {Evolutionary implications of the new triple-alpha nuclear reaction rate for low mass stars},
author = {Aaron Dotter and Bill Paxton},
journal= {arXiv preprint arXiv:0905.2397},
year = {2015}
}
Comments
Prepared as an A&A Research Note but not yet submitted. Comments are welcome