找回密码
 To register

QQ登录

只需一步,快速开始

扫一扫,访问微社区

Titlebook: Saturation of the f-mode Instability in Neutron Stars; Pantelis Pnigouras Book 2018 Springer Nature Switzerland AG 2018 Gravitational Wave

[复制链接]
楼主: Guffaw
发表于 2025-3-23 10:21:40 | 显示全部楼层
发表于 2025-3-23 15:41:21 | 显示全部楼层
The Oscillation Modes: Linear Perturbation Scheme,e oscillation modes of a star. We will first consider the simple case of a nonrotating star (Sect. .), in which the various classes of modes are defined (Sect. .), namely . and . modes. The former class contains the (fundamental) .-modes, the (pressure) .-modes, and the (buoyancy) .-modes, and the l
发表于 2025-3-23 21:36:53 | 显示全部楼层
The ,-mode Instability, not necessarily deformed by rotation into an oblate spheroid, but may also be shaped like a triaxial ellipsoid, should it rotate sufficiently fast. Depending on the assumed density profile, there is an upper limit on the maximum rotation that a star can support (Sect. 3.2), which determines whether
发表于 2025-3-24 01:57:31 | 显示全部楼层
Mode Coupling: Quadratic Perturbation Scheme, perturbations (Sect. .). We will show that, in the quadratic-perturbation approximation, modes couple in triplets, which satisfy a resonance condition (Sect. .). Coupling of an unstable mode to other (stable) modes of the star can lead to the saturation of the unstable mode’s amplitude, through a m
发表于 2025-3-24 03:16:10 | 显示全部楼层
Results,later during the discussion of the results. We will present results both for typical (Sect. .) and supramassive (Sect. .) neutron stars, for various polytropic and adiabatic exponents. In each section, we review the evolution of the instability and discuss the results. We also present estimations ab
发表于 2025-3-24 07:05:09 | 显示全部楼层
发表于 2025-3-24 10:53:44 | 显示全部楼层
发表于 2025-3-24 18:22:22 | 显示全部楼层
2190-5053 and make it saturate via a mechanism called parametric resonance instability. Further, it calculates the saturation amplitude of the most unstable f-mode multipoles throughout their so-called instability windows..978-3-030-07474-6978-3-319-98258-8Series ISSN 2190-5053 Series E-ISSN 2190-5061
发表于 2025-3-24 21:08:27 | 显示全部楼层
on about reasons for specific decision. The proposed models were created on Mt. Kopaonik, Serbia ski resort and it is shown that ski injury in the following hour on specific ski slope can be predicted with AUC ~0.76, which is better up to ~15% compared to classical approaches such as logistic regres
发表于 2025-3-25 02:25:24 | 显示全部楼层
 关于派博传思  派博传思旗下网站  友情链接
派博传思介绍 公司地理位置 论文服务流程 影响因子官网 SITEMAP 大讲堂 北京大学 Oxford Uni. Harvard Uni.
发展历史沿革 期刊点评 投稿经验总结 SCIENCEGARD IMPACTFACTOR 派博系数 清华大学 Yale Uni. Stanford Uni.
|Archiver|手机版|小黑屋| 派博传思国际 ( 京公网安备110108008328) GMT+8, 2025-5-19 13:36
Copyright © 2001-2015 派博传思   京公网安备110108008328 版权所有 All rights reserved
快速回复 返回顶部 返回列表