Kaonic nuclei probed by the in-flight (K-, n) reaction

被引：64

作者：

Kishimoto, T ^{[1
]}

Hayakawa, T

Ajimura, S

Minami, S

Sakaguchi, A

Shimizu, Y

Chrien, RE

May, M

Pile, P

Rusek, A

Sutter, R

Noumi, H

Tamura, H

Ukai, M

Miura, Y

Tanida, K

机构：

[1] Osaka Univ, Dept Phys, Toyonaka, Osaka 5600043, Japan

[2] Brookhaven Natl Lab, Upton, NY 11973 USA

[3] KEK, High Energy Accelerator Res Org, Tsukuba, Ibaraki 3050801, Japan

[4] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan

[5] RIKEN, Inst Phys & Chem Res, Wako, Saitama 3510198, Japan

来源：

NUCLEAR PHYSICS A | 2005年 / 754卷

基金：

日本学术振兴会;

关键词：

D O I：

10.1016/j.nuclphysa.2005.03.019

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Kaonic nuclei are observed by the (K-, n) reaction. The spectra indicate that the kaon nuclear potential is strongly attractive which seems to contradict many theoretical predictions. It suggests that kaon condensation is taking place in the core of neutron stars. (c) 2005 Elsevier B.V. All rights reserved.

引用

页码：383C / 390C

页数：8

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