Upper Limit on the Mass of RX J1856.5-3754 as a Possible Quark Star
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概要
- 論文の詳細を見る
Recent deep Chandra LETG+HRC-S observations suggest the possibility that RX J1856.5-3754 is a compact star whose radiation radius is 3.8-8.2 km. In this paper, we systematically calculate the mass-radius relations of quark stars within the bag model. Assuming that RX J1856.5-3754 is a pure quark star, we derive an upper limit on its mass for various sets of bag-model parameters.
- 理論物理学刊行会の論文
- 2003-05-25
著者
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SATO Katsuhiko
Research Institute for Fundamental Physics Kyoto University
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Iida K
Inst. Physical And Chemical Res. (riken) Wako Jpn
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Iida Kei
The Institute Of Physical And Chemical Research (riken)
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Kohri K
Research Center For The Early Universe (resceu) School Of Science University Of Tokyo
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Kohri Kazunori
Research Center For The Early Universe (resceu) School Of Science University Of Tokyo
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Sato Katsuhiko
Research Center For The Early Universe University Of Tokyo
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Sato Katsuhiko
Research Center For The Early Universe School Of Science The University Of Tokyo
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SATO Katsuhiko
Research Center for the Early Universe (RESCEU), School of Science, University of Tokyo:Department of Physics, School of Science, University of Tokyo
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KOHRI Kazunori
Research Center for the Early Universe (RESCEU), School of Science, University of Tokyo
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Koi SATO
Department of Physics, Nagoya University
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IIDA Kei
Department of Physics,University of Tokyo
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SATO Katsuhiko
Research Center for the Early Universe (RESCEU), School of Science, University of Tokyo:Departrment of Physics, Scool of Science, University of Tokyo
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