Results 61 to 70 of about 136,037 (243)
The Impact of Angular Momentum Loss on the Outcomes of Binary Mass Transfer
We use the rapid binary population synthesis code COMPAS to investigate commonly used prescriptions for the determination of mass transfer stability in close binaries and the orbital separations after stable mass transfer.
Reinhold Willcox +3 more
doaj +1 more source
Search for Electromagnetic Counterparts to LIGO-Virgo Candidates: Expanded Very Large Array
This paper summarizes a search for radio wavelength counterparts to candidate gravitational wave events. The identification of an electromagnetic counterpart could provide a more complete understanding of a gravitational wave event, including such ...
Collaboration, the LIGO Scientific +5 more
core +1 more source
The missing link in gravitational-wave astronomy: discoveries waiting in the decihertz range
The gravitational-wave astronomical revolution began in 2015 with LIGO’s observation of the coalescence of two stellar-mass black holes. Over the coming decades, ground-based detectors like laser interferometer gravitational-wave observatory (LIGO ...
M. A. Sedda +29 more
semanticscholar +1 more source
A key challenge in advancing messenger RNA (mRNA) therapeutics in cardiovascular diseases lies in achieving controlled release at the precise site within the vasculature. This study presents the development of perfluorocarbon nanodroplets with exceptional theranostic potential, enabling real‐time tracking through ultrasound and fluorine‐19 (19F ...
Haikun Liu +14 more
wiley +1 more source
Abstract The majority of planetary impacts occur at oblique angles. Impact structures on Earth are commonly eroded or buried, rendering the identification of the direction and angle of impact—using methods such as asymmetries in ejecta distribution, surface topographic expression, central uplift structure, and geophysical anomalies—challenging. In this
Eloise E. Matthews +5 more
wiley +1 more source
A quantum measurement-like event can produce any of a number of macroscopically distinct results, with corresponding macroscopically distinct gravitational fields, from the same initial state. Hence the probabilistically evolving large-scale structure of
Kent, Adrian
core +1 more source
Hands-on Gravitational Wave Astronomy: Extracting astrophysical information from simulated signals [PDF]
In this paper we introduce a hands-on activity in which introductory astronomy students act as gravitational wave astronomers by extracting information from simulated gravitational wave signals. The process mimics the way true gravitational wave analysis
Carroll B. W. +4 more
core +3 more sources
Detectability of intermediate-mass black holes in multiband gravitational wave astronomy [PDF]
The direct measurement of gravitational waves is a powerful tool for surveying the population of black holes across the universe. While LIGO has detected black holes as heavy as ~50 M ⊙ (ref.
K. Jani, D. Shoemaker, C. Cutler
semanticscholar +1 more source
Seismic reflection and topography insights into Ries crater diameter and megablock zone
Abstract Most of the extensive crater‐wide geophysical studies at the Ries impact structure were made decades ago when the origin of the structure was still being debated. Although it is one of the most studied impact structures, its internal structure was not imaged in high resolution until recently.
Kaidi Karro +5 more
wiley +1 more source
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.
Wenbo Chang +10 more
doaj +1 more source

