Chirally motivated <mml:math altimg="si1.gif" overflow="scroll" xmlns:xocs="http://www.elsevier.com/xml/xocs/dtd" xmlns:xs="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://www.elsevier.com/xml/ja/dtd" xmlns:ja="http://www.elsevier.com/xml/ja/dtd" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:tb="http://www.elsevier.com/xml/common/table/dtd" xmlns:sb="http://www.elsevier.com/xml/common/struct-bib/dtd" xmlns:ce="http://www.elsevier.com/xml/common/dtd" xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:cals="http://www.elsevier.com/xml/common/cals/dtd"><mml:msup><mml:mi>K</mml:mi><mml:mo>−</mml:mo></mml:msup></mml:math> nuclear potentials-Reference-Cited by-同舟云学术

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Chirally motivated K− nuclear potentials

Published:2011-08 Issue:5 Volume:702 Page:402-407
ISSN:0370-2693
Container-title:Physics Letters B
language:en
Short-container-title:Physics Letters B

Author:

Cieplý A.,Friedman E.,Gal A.,Gazda D.,Mareš J.

Funder

GACR

HadronPhysics2

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics

Reference34 articles.

1. Antikaon Interactions with Nucleons and Nuclei

2. T. Hyodo, D. Jido, Prog. Part. Nucl. Phys., submitted for publication, arXiv:1104.4474 [nucl-th].

3. Proc. Int. School of Physics “Enrico Fermi”, Course CLXVII;Schaffner-Bielich,2008

4. Astrophysical measurement of the equation of state of neutron star matter

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