[go: up one dir, main page]

Buonanno et al., 2009 - Google Patents

Comparison of post-Newtonian templates for compact binary inspiral signals<? format?> in gravitational-wave detectors

Buonanno et al., 2009

View PDF
Document ID
12368601720619471560
Author
Buonanno A
Iyer B
Ochsner E
Pan Y
Sathyaprakash B
Publication year
Publication venue
Physical Review D—Particles, Fields, Gravitation, and Cosmology

External Links

Snippet

The two-body dynamics in general relativity has been solved perturbatively using the post- Newtonian (PN) approximation. The evolution of the orbital phase and the emitted gravitational radiation are now known to a rather high order up to O (v 8), v being the …
Continue reading at arxiv.org (PDF) (other versions)

Classifications

    • GPHYSICS
    • G01MEASURING; TESTING
    • G01RMEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R33/00Arrangements or instruments for measuring magnetic variables
    • G01R33/20Arrangements or instruments for measuring magnetic variables involving magnetic resonance
    • G01R33/44Arrangements or instruments for measuring magnetic variables involving magnetic resonance using nuclear magnetic resonance [NMR]
    • G01R33/46NMR spectroscopy
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06FELECTRICAL DIGITAL DATA PROCESSING
    • G06F17/00Digital computing or data processing equipment or methods, specially adapted for specific functions
    • G06F17/30Information retrieval; Database structures therefor; File system structures therefor
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06FELECTRICAL DIGITAL DATA PROCESSING
    • G06F17/00Digital computing or data processing equipment or methods, specially adapted for specific functions
    • G06F17/50Computer-aided design
    • GPHYSICS
    • G06COMPUTING; CALCULATING; COUNTING
    • G06FELECTRICAL DIGITAL DATA PROCESSING
    • G06F17/00Digital computing or data processing equipment or methods, specially adapted for specific functions
    • G06F17/10Complex mathematical operations
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01RMEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R31/00Arrangements for testing electric properties; Arrangements for locating electric faults; Arrangements for electrical testing characterised by what is being tested not provided for elsewhere
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01RMEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R23/00Arrangements for measuring frequencies; Arrangements for analysing frequency spectra
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01RMEASURING ELECTRIC VARIABLES; MEASURING MAGNETIC VARIABLES
    • G01R13/00Arrangements for displaying electric variables or waveforms
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01NINVESTIGATING OR ANALYSING MATERIALS BY DETERMINING THEIR CHEMICAL OR PHYSICAL PROPERTIES
    • G01N30/00Investigating or analysing materials by separation into components using adsorption, absorption or similar phenomena or using ion-exchange, e.g. chromatography or field flow fractionation
    • G01N30/02Column chromatography
    • GPHYSICS
    • G01MEASURING; TESTING
    • G01VGEOPHYSICS; GRAVITATIONAL MEASUREMENTS; DETECTING MASSES OR OBJECTS
    • G01V1/00Seismology; Seismic or acoustic prospecting or detecting

Similar Documents

Publication Publication Date Title
Buonanno et al. Comparison of post-Newtonian templates for compact binary inspiral signals<? format?> in gravitational-wave detectors
Romero-Shaw et al. Bayesian inference for compact binary coalescences with bilby: validation and application to the first LIGO–Virgo gravitational-wave transient catalogue
Pratten et al. Setting the cornerstone for a family of models for gravitational waves from compact binaries: The dominant harmonic for nonprecessing quasicircular black holes
Boyle et al. The SXS Collaboration catalog of binary black hole simulations
Cotesta et al. Frequency-domain reduced-order model of aligned-spin effective-one-body waveforms with higher-order modes
Buonanno et al. Inspiral, merger, and ring-down of equal-mass black-hole binaries
Estellés et al. Time-domain phenomenological model of gravitational-wave subdominant harmonics for quasicircular nonprecessing binary black hole coalescences
Muñoz et al. Probing the small-scale matter power spectrum with large-scale 21-cm data
Chu et al. On the accuracy and precision of numerical waveforms: Effect of waveform extraction methodology
Boyle et al. High-accuracy numerical simulation of black-hole binaries: Computation of the gravitational-wave energy flux and comparisons with post-Newtonian approximants
Bohé et al. Improved effective-one-body model of spinning, nonprecessing binary black holes for the era of gravitational-wave astrophysics with advanced detectors
Hannam et al. Where post-Newtonian and numerical-relativity waveforms meet
Pan et al. Inspiral-merger-ringdown multipolar waveforms of nonspinning black-hole<? format?> binaries using the effective-one-body formalism
Mosser et al. Period-luminosity relations in evolved red giants explained by solar-like oscillations
Vaishnav et al. Matched filtering of numerical relativity templates of spinning binary black holes
Bernuzzi et al. Binary black hole coalescence in the extreme-mass-ratio limit: Testing<? format?> and improving the effective-one-body multipolar waveform
Katz et al. GPU-accelerated massive black hole binary parameter estimation with LISA
East et al. Comparing fully general relativistic and Newtonian calculations of structure formation
Verde et al. Early cosmology constrained
Mangiagli et al. Post-Newtonian phase accuracy requirements for stellar black hole binaries with LISA
Archidiacono et al. Dark Radiation in extended cosmological scenarios
Cai et al. No-go guide for late-time solutions to the Hubble tension: Matter perturbations
Antony et al. Discordances in cosmology and the violation of slow-roll inflationary dynamics
Emami et al. Cosmological tests of an axiverse-inspired quintessence field
Hoffmann et al. Signatures of cosmic reionization on the 21-cm two-and three-point correlation function I: quadratic bias modelling