Jove
Visualize
Contact Us

Related Concept Videos

Detection of Black Holes01:10

Detection of Black Holes

2.6K
Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
Not until the 1960s, when the first neutron...
2.6K
Reduced Mass Coordinates: Isolated Two-body Problem01:12

Reduced Mass Coordinates: Isolated Two-body Problem

2.5K
In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
2.5K
Nuclear Fusion02:45

Nuclear Fusion

34.1K
The process of converting very light nuclei into heavier nuclei is also accompanied by the conversion of mass into large amounts of energy, a process called fusion. The principal source of energy in the sun is a net fusion reaction in which four hydrogen nuclei fuse and ultimately produce one helium nucleus and two positrons.
A helium nucleus has a mass that is 0.7% less than that of four hydrogen nuclei; this lost mass is converted into energy during the fusion. This reaction produces about...
34.1K
Gravitation Between Spherically Symmetric Masses01:14

Gravitation Between Spherically Symmetric Masses

1.4K
The gravitational potential energy between two spherically symmetric bodies can be calculated from the masses and the distance between the bodies, assuming that the center of mass is concentrated at the respective centers of the bodies.
1.4K
Atomic Nuclei: Nuclear Relaxation Processes01:23

Atomic Nuclei: Nuclear Relaxation Processes

1.3K
In the absence of an external magnetic field, nuclear spin states are degenerate and randomly oriented. When a magnetic field is applied, the spins begin to precess and orient themselves along (lower energy) or against (higher energy) the direction of the field. At equilibrium, a slight excess population of spins exists in the lower energy state. Because the direction of the magnetic field is fixed as the z-axis,  the precessing magnetic moments are randomly oriented around the z-axis.
1.3K
Schwarzschild Radius and Event Horizon01:21

Schwarzschild Radius and Event Horizon

2.9K
No object with a finite mass can travel faster than the speed of light in a vacuum. This fact has an interesting consequence in the domain of extremely high gravitational fields.
The minimum speed required to launch a projectile from the surface of an object to which it is gravitationally bound so that it eventually escapes the object’s gravitational field is called the escape velocity. The escape velocity is independent of the mass of the object. Merging the idea of escape...
2.9K

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

LISA Sources in Milky Way Globular Clusters.

Physical review letters·2018
Same author

Post-Newtonian Dynamics in Dense Star Clusters: Highly Eccentric, Highly Spinning, and Repeated Binary Black Hole Mergers.

Physical review letters·2018
Same author

Erratum: Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO [Phys. Rev. Lett. 115, 051101 (2015)].

Physical review letters·2016
Same author

Binary Black Hole Mergers from Globular Clusters: Implications for Advanced LIGO.

Physical review letters·2015
Same author

Astronomy. A black widow's best friend?

Science (New York, N.Y.)·2011
Same author

Hot Jupiters from secular planet-planet interactions.

Nature·2011
Same journal

Primordial black holes and their gravitational-wave signatures.

Living reviews in relativity·2025
Same journal

Solvable models of quantum black holes: a review on Jackiw-Teitelboim gravity.

Living reviews in relativity·2023
Same journal

Electromagnetic counterparts to massive black-hole mergers.

Living reviews in relativity·2022
Same journal

Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA.

Living reviews in relativity·2020
Same journal

Kilonovae.

Living reviews in relativity·2019
Same journal

Erratum: Publisher Correction: Interferometer techniques for gravitational-wave detection.

Living reviews in relativity·2019
See all related articles
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Experiment Video

Updated: Mar 8, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

9.0K

Binary Neutron Star Mergers.

Joshua A Faber1, Frederic A Rasio2

  • 1Center for Computational Relativity and Gravitation and School of Mathematical Sciences, Rochester Institute of Technology, 85 Lomb Memorial Drive, Rochester, NY 14623 USA.

Living Reviews in Relativity
|February 7, 2017
PubMed
Summary
This summary is machine-generated.

This review covers binary neutron star mergers, from formation and rates to simulation techniques. It highlights advancements in understanding coalescence physics and future directions for gravitational-wave astronomy.

More Related Videos

Neutron Spin Echo Spectroscopy as a Unique Probe for Lipid Membrane Dynamics and Membrane-Protein Interactions
10:02

Neutron Spin Echo Spectroscopy as a Unique Probe for Lipid Membrane Dynamics and Membrane-Protein Interactions

Published on: May 27, 2021

4.6K
Neutron Crystallography Data Collection and Processing for Modelling Hydrogen Atoms in Protein Structures
10:10

Neutron Crystallography Data Collection and Processing for Modelling Hydrogen Atoms in Protein Structures

Published on: December 1, 2020

5.7K

Related Experiment Videos

Last Updated: Mar 8, 2026

Setting Limits on Supersymmetry Using Simplified Models
07:46

Setting Limits on Supersymmetry Using Simplified Models

Published on: November 15, 2013

9.0K
Neutron Spin Echo Spectroscopy as a Unique Probe for Lipid Membrane Dynamics and Membrane-Protein Interactions
10:02

Neutron Spin Echo Spectroscopy as a Unique Probe for Lipid Membrane Dynamics and Membrane-Protein Interactions

Published on: May 27, 2021

4.6K
Neutron Crystallography Data Collection and Processing for Modelling Hydrogen Atoms in Protein Structures
10:10

Neutron Crystallography Data Collection and Processing for Modelling Hydrogen Atoms in Protein Structures

Published on: December 1, 2020

5.7K

Area of Science:

  • Astrophysics
  • Gravitational-wave astronomy
  • Computational physics

Background:

  • Binary neutron star systems are key sources of gravitational waves.
  • Understanding their mergers is crucial for multi-messenger astronomy.
  • Previous studies have laid the groundwork for current research.

Purpose of the Study:

  • To provide a comprehensive review of binary neutron star coalescence.
  • To discuss formation channels, merger rates, and theoretical models.
  • To summarize numerical techniques and simulation results.

Main Methods:

  • Review of theoretical predictions for merger rates.
  • Discussion of quasi-equilibrium formalisms for pre-merger dynamics.
  • Analysis of numerical techniques for dynamical simulations (relativistic, hydrodynamics, gravitational-wave extraction, microphysics).

Main Results:

  • Overview of current understanding of binary coalescence physics.
  • Summary of recent simulation results, including relativistic and microphysically detailed studies.
  • Identification of key orbital instability processes driving mergers.

Conclusions:

  • The field is advancing rapidly with new simulation capabilities.
  • Future gravitational-wave detectors and petascale computing will drive new discoveries.
  • Continued research is essential for interpreting gravitational-wave signals from neutron star mergers.