Skip to main navigation
Skip to search
Skip to main content
Northwestern Scholars Home
Help & FAQ
Home
Experts
Organizations
Research Output
Grants
Core Facilities
Datasets
Search by expertise, name or affiliation
Post-Newtonian SPH calculations of binary neutron star coalescence: Method and first results
Joshua A. Faber
*
,
Frederic A. Rasio
*
Corresponding author for this work
Physics and Astronomy
Research output
:
Contribution to journal
›
Article
›
peer-review
56
Scopus citations
Overview
Fingerprint
Fingerprint
Dive into the research topics of 'Post-Newtonian SPH calculations of binary neutron star coalescence: Method and first results'. Together they form a unique fingerprint.
Sort by
Weight
Alphabetically
INIS
neutron stars
100%
particles
66%
coalescence
66%
hydrodynamics
50%
star models
33%
equilibrium
33%
simulation
16%
signals
16%
distance
16%
modulation
16%
relaxation
16%
relativistic range
16%
lagrangian
16%
general relativity theory
16%
wave forms
16%
gravitational waves
16%
gravitational radiation
16%
synchronization
16%
cosmic gamma bursts
16%
equations of state
16%
Physics
Neutron Stars
100%
Model
83%
Particle
66%
Hydrodynamics
50%
Calculation
50%
Modulation
16%
Equations of State
16%
Waveform
16%
Lagrangian Function
16%
Polytropes
16%
General Relativity
16%
Simulation
16%
Work
16%
Distance
16%
Terms
16%
Misalignment
16%
Synchronism
16%