Coalescing binaries as possible standard candles

@article{Capozziello2009CoalescingBA,
  title={Coalescing binaries as possible standard candles},
  author={Salvatore Capozziello and Mariafelicia De Laurentis and Michelangelo Formisano},
  journal={Astroparticle Physics},
  year={2009},
  volume={33},
  pages={190-194}
}

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References

SHOWING 1-10 OF 44 REFERENCES

Short GRB and binary black hole standard sirens as a probe of dark energy

Observations of the gravitational radiation from well-localized, inspiraling compact-object binaries can measure absolute source distances with high accuracy. When coupled with an independent

The last three minutes: Issues in gravitational-wave measurements of coalescing compact binaries.

Improved wave form modeling is needed as a foundation for extracting the waves’ information, but is not necessary for wave detection.

Determining the Hubble constant from gravitational wave observations

I report here how gravitational wave observations can be used to determine the Hubble constant, H0. The nearly monochromatic gravitational waves emitted by the decaying orbit of an ultra–compact,

Gravitational waves from merging compact binaries: How accurately can one extract the binary's parameters from the inspiral waveform?

This work investigates how accurately the distance to the source and the masses and spins of the two bodies will be measured from the inspiral gravitational wave signals by the three-detector LIGO-VIRGO network using ``advanced detectors'' (those present a few years after initial operation).

Measurements of general relativistic effects in the binary pulsar PSR1913 + 16

Measurements of second- and third-order relativistic effects in the orbit of binary pulsar PSR1913 + 16 have yielded self-consistent estimates of the masses of the pulsar and its companion,

Host Galaxies Catalog Used in LIGO Searches for Compact Binary Coalescence Events

An up-to-date catalog of nearby galaxies considered to be hosts of binary compact objects is provided, with complete information about sky position, distance, extinction-corrected blue luminosity,

The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for the Laser Interferometer Gravitational-Wave Observatory

The recent discovery of the first four afterglows of short-hard gamma-ray bursts (SHBs) suggests that they typically result from long-lived progenitor systems. The most popular progenitor model

The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for LIGO

The recent discovery of the first four afterglows of short-hard gamma-ray bursts (SHBs), suggests that they typically result from long-lived progenitor systems. The most popular progenitor model

Plunge waveforms from inspiralling binary black holes.

This work uses a technique that combines the full numerical approach to solve the Einstein equations, applied in the truly nonlinear regime, and linearized perturbation theory around the final distorted single black hole at later times to compute the plunge waveforms.

LISA observations of rapidly spinning massive black hole binary systems

Binary systems of massive black holes will be detectable by the Laser Interferometer Space Antenna (LISA) throughout the entire Universe. Observations of gravitational waves from this class of