Compact Objects in close orbits as Gravitational Wave Sources: Formation Scenarios and Properties

Abstract

Gravitational Waves (GWs) provide a unique way to explore our Universe. The ongoing ground-based detectors, e.g., LIGO, Virgo, and KAGRA, and the upcoming next-generation detectors, e.g., Cosmic Explorer and Einstein Telescope, as well as the future space-borne GW antennas, e.g., LISA, TianQin, and TaiJi, cover a wide range of GW frequencies {from $\sim 10^{-4}\mathrm{Hz}$ to $\sim 10^3\mathrm{Hz}$} and almost all types of compact objects in close orbits serve as the potential target sources for these GW detectors. The synergistic multi-band GW and EM observations would allow us to study fundamental physics from stars to cosmology. {The formation of stellar GW sources has been extensively explored in recent years, and progress on physical processes in binary interaction has been made as well. Furthermore, some studies have shown that the progress in binary evolution may significantly affect the properties of the stellar GW sources.}

arXiv comment33 pages, 8 figures; Invited Review of Results in Physics; Accepted for publication; References updated

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• Mass-loss predictions for evolved very metal-poor massive stars
• Prospects for Gravitational Wave Measurement of ZTFJ1539+5027
• Hydrodynamic Simulations of Electron-capture Supernovae: Progenitor and Dimension Dependence
• The Orbital Nature of 81 Ellipsoidal Red Giant Binaries in the Large Magellanic Cloud
• Exploring compact binary populations with the Einstein Telescope
• Internal circulation in tidally locked massive binary stars -- Consequences for double black hole formation
• On the energy source of ultra-stripped supernovae
• Extremely low-mass white dwarf stars observed in Gaia DR2 and LAMOST DR8
• Effects of Irradiation on the Evolution of Ultra-compact X-ray Binaries
• On the progenitors of AM CVn stars as LISA sources: the evolved donor star channel
• Criteria for Dynamical Timescale Mass Transfer of Metal-poor Intermediate-mass Stars
• Monte Carlo population synthesis on massive star binaries: Astrophysical implications for gravitational wave sources
• Accretion-Induced Collapse of Dark Matter Admixed White Dwarfs -- I: Formation of Low-mass Neutron Stars
• On the Angular Momentum Transport Efficiency within the Star Constrained from Gravitational-wave Observations
• Formation of black widows through ultra-compact X-ray binaries with He star companions
• Weighing Milky Way Satellites with LISA
• The Tail of PSR J0002+6216 and the Supernova Remnant CTB 1
• Reverse Algols and hydrogen-rich Wolf-Rayet stars from very massive binaries
• A high-mass X-ray binary descended from an ultra-stripped supernova
• Hydrodynamic Winds From Twin-Star Binaries
• A Black Hole Kicked At Birth: MAXI J1305-704
• Alfvén wave-driven wind from RGB and AGB stars
• Binary black hole mergers from young massive and open clusters: comparison to GWTC-2 gravitational wave data
• Evolution of AM CVn binaries with WD donors
• The Large Magellanic Cloud Revealed in Gravitational Waves with LISA
• A Roche Lobe-filling hot Subdwarf and White Dwarf Binary: possible detection of an ejected common envelope
• Merging binary black holes formed through double-core evolution
• Evolved cataclysmic variables as progenitors of AM CVn stars
• Multi-Messenger Constraints on Magnetic Fields in Merging Black Hole-Neutron Star Binaries
• Cataclysmic variables are a key population of gravitational wave sources for LISA
• Repeated mergers of black hole binaries: implications for GW190521
• Hot subdwarf B stars with neutron star components II: Binary population synthesis
• Black Hole Ultra-compact X-ray Binaries: Galactic Low-Frequency Gravitational Wave Sources
• Simulations of the progenitors of black hole-neutron star gravitational wave sources
• New insights into the helium star formation channel of AM CVn systems with explanations of Gaia14aae and ZTFJ1637+49
• How many extra-Galactic stellar-mass binary black holes will be detected by space gravitational-wave interferometers?
• X-ray and Radio Variabilities of PSR J2032+4127 near Periastron
• Constraining Progenitors of Observed LMXBs Using CARB Magnetic Braking
• Massive Double White Dwarfs and the AM CVn Birthrate
• Does Nature allow formation of ultra-compact black hole X-ray binaries via accretion-induced collapse of neutron stars?
• He-star donor AM CVn stars and their progenitors as LISA sources
• Evolving ONe WD+He WD systems to ultra-compact X-ray binaries
• ELM of ELM-WD: An extremely low mass hot star discovered in LAMOST survey
• Mechanisms for high spin in black-hole neutron-star binaries and kilonova emission: inheritance and accretion
• The effects of Galactic model uncertainties on LISA observations of double neutron stars

Cited by in corpus (5)

• Gravitational Wave Astronomy With TianQin
• Evolution and final fate of massive post-common-envelope binaries
• Resolution of a paradox: SDSS J1257+5428 can be explained as a descendant of a cataclysmic variable with an evolved donor
• Ultra-compact X-ray Binaries: A Review
• Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss