- 1、本文档共8页,可阅读全部内容。
- 2、有哪些信誉好的足球投注网站(book118)网站文档一经付费(服务费),不意味着购买了该文档的版权,仅供个人/单位学习、研究之用,不得用于商业用途,未经授权,严禁复制、发行、汇编、翻译或者网络传播等,侵权必究。
- 3、本站所有内容均由合作方或网友上传,本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺!文档内容仅供研究参考,付费前请自行鉴别。如您付费,意味着您自己接受本站规则且自行承担风险,本站不退款、不进行额外附加服务;查看《如何避免下载的几个坑》。如果您已付费下载过本站文档,您可以点击 这里二次下载。
- 4、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等,请点击“版权申诉”(推荐),也可以打举报电话:400-050-0827(电话支持时间:9:00-18:30)。
查看更多
Metastable strange matter and compact quark stars
a
r
X
i
v
:
a
s
t
r
o
-
p
h
/
0
3
0
4
0
9
6
v
1
4
A
p
r
2
0
0
3
Metastable strange matter and compact quark stars
M. Malheiro? ?, M. Fiolhais§ and A. R. Taurines?
? Instituto de F??sica, Universidade Federal Fluminense, 24210-340 Nitero?i, Brazil
§ Departamento de F??sica and Centro de F??sica Computacional,
Universidade de Coimbra, P-3004-516 Coimbra, Portugal
? Instituto de F??sica, Universidade Federal do Rio Grande do Sul CP 15051,
91501-970 Porto Alegre, Brazil
Abstract. Strange quark matter in beta equilibrium at high densities is studied in
a quark confinement model. Two equations of state are dynamically generated for the
same set of model parameters used to describe the nucleon: one corresponds to a chiral
restored phase with almost massless quarks and the other to a chiral broken phase.
The chiral symmetric phase saturates at around five times the nuclear matter density.
Using the equation of state for this phase, compact bare quark stars are obtained with
radii and masses in the ranges R ~ 5 ? 8 km and M ~ M⊙. The energy per baryon
number decreases very slowly from the center of the star to the periphery, remaining
above the corresponding values for the iron or the nuclear matter, even at the edge.
Our results point out that strange quark matter at very high densities may not be
absolutely stable and the existence of an energy barrier between the two phases may
prevent the compact quarks stars to decay to hybrid stars.
Submitted to: J. Phys. G: Nucl. Phys.
? Email: mane@if.uff.br
Metastable strange matter and compact quark stars 2
1. Introduction
The recent discoveries of X-ray sources, whose origin may be attributed to strange
stars [1, 2, 3], is stimulating theoretical research on the structure, composition, dynamics
and evolution of such objects. It is believed that the innermost region of compact
stars, such as neutron stars, can be made out of hyperons, meson condensates or quark
matter [4, 5, 6, 7, 8], whose thermodynamical behavior can be expr
您可能关注的文档
- Killtest 分享JN0-100 题库.pdf
- KIMOS计算参数实例.pdf
- Kinematics of Vega-like stars lifetimes and temporal evolution of circumstellar dust disks.pdf
- Kinetic Sweep and Prune for Collision Detection.pdf
- Kinetic magnetoelectric effect in a 2D semiconductor strip due to boundary-confinement indu.pdf
- Kinetics of Particles in Relativistic Collisionless Shocks.pdf
- KLINGERSIL C-4400 MSDS.pdf
- KN-Q7 Manual.pdf
- KneeMeasurer. A Wearable Interface for Joint Angle Measurements.pdf
- Knowledge Discovery on Clinical Trials to Explore the Overall Safety of the Medicinal Produ.pdf
最近下载
- TBIE 004—2023通孔回流焊接技术规范团标.pdf
- 国开《MySQL数据库应用》形考1-4(试题及答案).pdf VIP
- 煤矿安全生产作业规程操作规程安全技术措施编制审批贯彻及执行管理制度.doc
- 2020年光学膜行业研究报告.pdf
- 采血管种类和应用ppt课件.pptx VIP
- 职业生涯报告六篇.pdf VIP
- Unit 4 Plants arounds us PartA Let's talk(课件)人教PEP版(2024)英语三年级上册.pptx
- 七年级上册生物:必考问答式知识点汇总(背诵+默写).docx
- 《青纱帐——甘蔗林》课件【中职专用】高教版 基础模块下册.pptx
- 国家开放大学学位英语历年真题试卷号1909.docx
文档评论(0)