Effect of Finite Quark Masses on the Superdense Quarkion Configurations
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概要
- 論文の詳細を見る
Phase transition between neutron matter and quark matter is considered by taking account of the finite masses of the constituent quarks. The transition pressures and densities obtained are compared with those for the case of massless quarks. However, the transition densities so obtained are still much higher than the maxium stable certral density limits of neutron stars.
- 理論物理学刊行会の論文
- 1980-06-25
著者
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Bhattacharjee Pijushpani
Department Of Physics And Astrophysics University Of Delhi
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Anand J.d.
Department Of Physics And Astrophysics University Of Delhi
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BHATTACHARJEE Pijushpani
Department of Physics and Astrophysics, University of Delhi