| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9827442 | Astroparticle Physics | 2005 | 7 Pages |
Abstract
The photo-coulomb neutrino process (Z+γâZ+ν+ν¯) has been considered in the electro-weak theory and the influence of this process to the evolution of stars has been outlined. The scattering cross-section of this process is calculated in both low and high energy limit. The neutrino mass has been taken into account in this calculation. In the low-energy limit the neutrino luminosity is computed in the temperature range 108-109 K and is also compared to the previous result obtained according to the current-current coupling theory. The process may be significant for the evolution of stars in the later phases.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Indranath Bhattacharyya,