Expansion of Accreting Main-sequence Stars during Rapid Mass Transfer
Accreting main-sequence stars expand significantly when the mass accretion timescale is much shorter than their thermal timescales. This occurs during mass transfer from an evolved giant star onto a main-sequence companion in a binary system and is an ...
Mike Y. M. Lau +3 more
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Choosing Suitable Noise Models for Nanohertz Gravitational-wave Astrophysics
Accurately estimating the parameters of the nanohertz gravitational-wave background is essential for understanding its origin. The background is typically modeled with a power-law spectrum, parameterized with an amplitude A , which describes its ...
Valentina Di Marco +4 more
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The promises of gravitational-wave astronomy. [PDF]
Martin IW +3 more
europepmc +1 more source
Gravitational-wave astronomy: delivering on the promises. [PDF]
Schutz BF.
europepmc +1 more source
`Bridging Gravitational Wave Astronomy and Observational Astrophysics', Proceedings of the 13th Gravitational Wave Data Analysis Workshop (GWDAW13) (San Juan, Puerto Rico, 19–22 January 2009), sponsored by the Center for Gravitational Wave Astronomy, The University of Texas at Brownsville and The National Astronomy and Ionosphere Center [PDF]
M. C. Díaz +2 more
openalex +1 more source
Axisymmetric deformations of neutron stars and gravitational-wave astronomy [PDF]
Guilherme Raposo, Paolo Pani
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Special Lecture “KAGRA and Gravitational-wave Astronomy”
Hiroshi Daimon
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Solar Plasma Noise in TianQin Laser Propagation: An Extreme Case and Statistical Analysis
TianQin (TQ) proposes to detect gravitational-wave signals by using laser interferometry. However, the laser propagation effect introduces a potential noise factor for TQ.
Yanan Liu +4 more
doaj +1 more source
Gauged Q-ball dark matter through a cosmological first-order phase transition
As a new type of dynamical dark matter mechanism, we discuss the stability of the gauged Q-ball dark matter and its production mechanism through a cosmological first-order phase transition.
Siyu Jiang, Fa Peng Huang, Pyungwon Ko
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