搜索结果: 1-13 共查到“星系与宇宙学 Neutron”相关记录13条 . 查询时间(0.139 秒)
Scientists map gusty winds in a far-off neutron star system(图)
中子星系统 阵风图 星系形成
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2023/6/9
LIGO and Virgo detect neutron star smash-ups(图)
LIGO Virgo neutron star smash-ups
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2019/10/30
On April 25, NSF's Laser Interferometer Gravitational-Wave Observatory (LIGO) and the European-based Virgo detector registered gravitational waves from what appears to be a crash between two neutron s...
Measuring a cosmological distance-redshift relationship using only gravitational wave observations of binary neutron star coalescences
neutron stars gravitational waves cosmology
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2011/10/14
Detection of gravitational waves from the inspiral phase of binary neutron star coalescence will allow us to measure the effects of the tidal coupling in such systems. These effects will be measurable...
Initial data for binary neutron stars with arbitrary spins
Initial data binary neutron stars arbitrary spins
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2011/10/18
In general neutron stars in binaries are spinning. Due to the existence of millisecond pulsars we know that these spins can be substantial. We argue that spins with periods on the order a few dozen mi...
Towards Quark Deconfinement in Neutron Stars via Spindown: Gravitational Waves or Magnetic Braking?
Quark Deconfinement Neutron Stars Gravitational Waves Magnetic Braking
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2011/9/28
A phase of interacting quark matter can arise inside the dense core of isolated neutron stars when they have been sufficiently spun down from their initial rapidly rotating configuration. In this work...
Tidal deformations of neutron stars: The role of stratification and elasticity
Tidal deformations stars:stratification elasticity
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2011/9/27
We discuss the response of neutron stars to the tidal interaction in a compact binary system, as encoded in the Love number associated with the induced deformation. This problem is of interest for gra...
Rapid Neutron Capture Process in Supernovae and Chemical Element Formation
Supernova—nucleosynthesis—abundance—r-process
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2010/9/15
The rapid neutron capture process (r-process) is one of the major nucleosynthesis processes responsible for the synthesis of heavy nuclei beyond iron. Isotopes beyond Fe are most exclusively formed in...
The Twin Peak QPOs in Neutron Star and Black Hole Sources:What is explained, and What is not
The Twin Peak QPOs Black Hole Sources Neutron Star
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2009/7/1
The Twin Peak QPOs in Neutron Star and Black Hole Sources:What is explained, and What is not。
The crust cooling curve of the neutron star in mxb 1659{29
crust cooling curve neutron star mxb 1659{29
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2009/6/17
The crust cooling curve of the neutron star in mxb 1659{29。
The complex relations between Supernova Remnants and Neutron Stars
Supernova Remnants Neutron Stars
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2009/6/10
The complex relations between Supernova Remnants and Neutron Stars。
Black hole-neutron star mergers
neutron star mergers Black hole
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2009/6/8
Black hole-neutron star mergers。
Neutron diffusion and nucleosynthesis in an inhomogeneous big bang model
Neutron diffusion big bang model
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2009/6/8
Neutron diffusion and nucleosynthesis in an inhomogeneous big bang model。
Evolution of Neutron Star Magnetic Fields
Neutron stars Magnetic field
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2009/5/19
This paper reviews the current status of the theoretical models
of the evolution of the magnetic fields of neutron stars other than magnetars.
It appears that the magnetic fields of neutron stars de...