Guffaw
发表于 2025-3-21 17:54:17
书目名称Saturation of the f-mode Instability in Neutron Stars影响因子(影响力)<br> http://figure.impactfactor.cn/if/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars影响因子(影响力)学科排名<br> http://figure.impactfactor.cn/ifr/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars网络公开度<br> http://figure.impactfactor.cn/at/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars网络公开度学科排名<br> http://figure.impactfactor.cn/atr/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars被引频次<br> http://figure.impactfactor.cn/tc/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars被引频次学科排名<br> http://figure.impactfactor.cn/tcr/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars年度引用<br> http://figure.impactfactor.cn/ii/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars年度引用学科排名<br> http://figure.impactfactor.cn/iir/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars读者反馈<br> http://figure.impactfactor.cn/5y/?ISSN=BK0860962<br><br> <br><br>书目名称Saturation of the f-mode Instability in Neutron Stars读者反馈学科排名<br> http://figure.impactfactor.cn/5yr/?ISSN=BK0860962<br><br> <br><br>
Ligneous
发表于 2025-3-21 21:26:01
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cleaver
发表于 2025-3-22 00:27:54
Final Remarks,Summary, conclusions, and final remarks.
ANTI
发表于 2025-3-22 05:10:29
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maintenance
发表于 2025-3-22 09:40:44
978-3-030-07474-6Springer Nature Switzerland AG 2018
Retrieval
发表于 2025-3-22 14:57:07
Saturation of the f-mode Instability in Neutron Stars978-3-319-98258-8Series ISSN 2190-5053 Series E-ISSN 2190-5061
Popcorn
发表于 2025-3-22 19:56:38
Introduction,n be applied in neutron stars, so that the equation of state of dense nuclear matter is determined. Then, we discuss neutron stars as gravitational-wave sources, focusing on the presence of unstable oscillation modes and reviewing their significance both for gravitational-wave asteroseismology and neutron star evolution.
fender
发表于 2025-3-23 01:12:06
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贪婪性
发表于 2025-3-23 02:17:20
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世俗
发表于 2025-3-23 08:35:59
The Oscillation Modes: Linear Perturbation Scheme,ghout this study. Finally, we consider the general case of a rotating star (Sect. .), making use of the slow-rotation approximation, i.e., introducing (up to second-order) rotational corrections to the eigenfrequencies.