Title of article
Kaon-Nucleus Interaction Studied through the in-flight image Reactions Original Research Article
Author/Authors
T. Kishimoto، نويسنده , , T. Hayakawa، نويسنده , , S. Ajimura، نويسنده , , F. Khanam، نويسنده , , T. Itabashi، نويسنده , , K. Matsuoka، نويسنده , , S. Minami، نويسنده , , Y. Mitoma، نويسنده , , A. Sakaguchi، نويسنده , , Y. Shimizu، نويسنده , , K. Terai، نويسنده , , R.E. Chrien، نويسنده , , P. Pile، نويسنده , , H. Noumi، نويسنده , , M. Sekimoto، نويسنده , , H. Takahashi، نويسنده , , T. Fukuda، نويسنده , , W. Imoto، نويسنده , , Y. Mizoi، نويسنده ,
Issue Information
هفته نامه با شماره پیاپی سال 2009
Pages
3
From page
321
To page
323
Abstract
We studied the View the MathML source-nucleus interaction by the (K−,N) reactions on 12C and 16O. An appreciable strength observed in a bound region indicates that the View the MathML source-nuclear potential is strongly attractive. Potential depth was derived by comparing with the theoretical calculations. It is −190 MeV for the View the MathML source −160 MeV for the View the MathML source, and −180 MeV for the View the MathML source reaction and −160 MeV for the View the MathML source respectively. Our data suggest that the View the MathML source-nucleus potential is sufficiently deep to realize kaon condensation in the core of neutron stars.
Keywords
Kaon-nucleus interaction , Kaon condensation , Neutron stars
Journal title
Nuclear physics A
Serial Year
2009
Journal title
Nuclear physics A
Record number
1204858
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