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Earth–lunar thermal effect on the temperature stability of TianQin telescope and the suppression methods
Published 2025-03-01“…TianQin is a geocentric space-based gravitational wave detection mission, it will confront a more complex and variable orbital thermal environment compared to heliocentric orbit missions like LISA. …”
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62
Dealing with data gaps for TianQin with massive black hole binary signal
Published 2025-01-01“…Abstract Space-borne gravitational wave detectors like TianQin might encounter data gaps due to factors like micro-meteoroid collisions or hardware failures. …”
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63
3D Localization of FRB 20190425A for Its Potential Host Galaxy and Implications
Published 2025-01-01“…Although the absence of optical emission detection raises doubts, it does not definitively disprove the connection between the gravitational wave (GW) and FRB.…”
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64
Kilonova/Macronova Emission from Compact Binary Mergers
Published 2016-01-01“…Since the high expansion velocity (v~0.1–0.2c) is a robust outcome of compact binary mergers, the detection of smooth spectra will be the smoking gun to conclusively identify the gravitational wave source.…”
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65
Analysis of the Conformally Flat Approximation for Binary Neutron Star Initial Conditions
Published 2017-01-01“…We illustrate the use of this approximation for orbiting neutron stars in the quasicircular orbit approximation to demonstrate the equation of state dependence of these initial conditions and how they might affect the emergent gravitational wave frequency as the stars approach the innermost stable circular orbit.…”
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66
Gravitational echoes from braneworlds
Published 2025-01-01“…Furthermore, we can restrict the parameters of the braneworld by calculating the strength of the first gravitational echo and using the current gravitational wave data.…”
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67
A Possible Solution of the Cosmological Constant Problem Based on GW170817 and Planck Observations with Minimal Length Uncertainty
Published 2022-01-01“…We demonstrate that the GUP parameter, β0, could be best constrained by the gravitational wave observations, GW170817 event. To determine the difference between the group velocity of graviton and that of the light, we suggest another proposal based on the modified dispersion relations (MDRs). …”
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68
Multi-messenger probes of asteroid mass primordial black holes: Superradiance spectroscopy, Hawking radiation, and microlensing
Published 2025-02-01“…Further complementarity from a stochastic gravitational-wave background emerging from the black hole formation mechanism is also considered.…”
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69
Reduction of absorption of Ta2O5 monolayers through the suppression of structural defects by employing an appropriate ionic oxygen concentration
Published 2025-02-01“…Abstract Ultralow-absorption laser films have critical applications in high-power continuous-laser and gravitational-wave-detection systems. During film deposition, the ionic oxygen concentration significantly affects the absorption loss of the film. …”
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70
Singlet-doublet fermionic dark matter in gauge theory of baryons
Published 2025-01-01“…We show that the model offers a viable parameter space for a cosmologically consistent DM candidate that can be probed through direct detection searches, collider experiments, and gravitational wave (GW) experiments.…”
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71
Electroweak phase transition in two scalar singlet model with pNGB dark matter
Published 2025-01-01“…Moreover, we delve into the gravitational wave signatures associated with this framework, offering valuable insights that complement traditional dark matter direct and indirect detection methods.…”
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72
New models of quintessential inflation featuring plateau and hilltop potentials
Published 2025-01-01“…A forecast for the gravitational wave background generated in these models is provided.…”
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73
Quasinormal modes and GUP-corrected Hawking radiation of BTZ black holes within modified gravity frameworks
Published 2025-02-01“…The study concludes that modified gravity parameters significantly influence QNM frequencies and effective potential profiles, offering insights into black hole stability and suggesting that these theoretical predictions may be tested through gravitational wave observations.…”
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74
Black Hole Accretion and Spin-up through Stellar Collisions in Dense Star Clusters
Published 2025-01-01“…Dynamical interactions in dense star clusters could significantly influence the properties of black holes, leaving imprints on their gravitational-wave signatures. While previous studies have mostly focused on repeated black hole mergers for spin and mass growth, this work examines the impact of physical collisions and close encounters between black holes and (noncompact) stars. …”
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75
Simulation analysis of radiometer effect and outgassing based on molecular particle source perturbation
Published 2025-01-01“…Abstract The Laser Interferometer Space Antenna (LISA) mission is designed to detect space gravitational wave sources in the millihertz band. A critical factor in the success of this mission is the residual acceleration noise metric of the internal test mass (TM) within the ultra-precise inertial sensors. …”
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76
X-ray pulsed light curves of highly compact neutron stars as probes of scalar–tensor theories of gravity
Published 2024-12-01“…Consequently, scalar parameters might be better constrained when uncertainties in NS radii decrease, where this could occur with the advent of next-generation gravitational wave detectors, such as the Einstein Telescope and LISA, as well as future electromagnetic missions like eXTP and ATHENA. …”
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Improving the Determination of Supernova Cosmological Redshifts by Using Galaxy Groups
Published 2025-01-01Get full text
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