# Observational upper limits on the gravitational wave production of core collapse supernovae

@article{Zhu2010ObservationalUL, title={Observational upper limits on the gravitational wave production of core collapse supernovae}, author={Xing-Jiang Zhu and E J Howell and David G Blair}, journal={Monthly Notices of the Royal Astronomical Society: Letters}, year={2010}, volume={409} }

The upper limit on the energy density of a stochastic gravitational wave (GW) background obtained from the two-year science run (S5) of the Laser Interferometer Gravitational-wave Observatory (LIGO) is used to constrain the average GW production of core collapse supernovae (ccSNe). We assume that the ccSNe rate tracks the star formation history of the universe and show that the stochastic background energy density depends only weakly on the assumed average source spectrum. Using the ccSNe rate…

## 17 Citations

Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO's First Observing Run.

- Physics, MedicinePhysical review letters
- 2017

This work performs a search for the isotropic stochastic gravitational-wave background using data from Advanced Laser Interferometer Gravitational Wave Observatory's (aLIGO) first observing run, and constrain the dimensionless energy density of gravitational waves to be Ω_{0}<1.7×10^{-7} with 95% confidence.

STOCHASTIC GRAVITATIONAL WAVE BACKGROUND FROM NEUTRON STAR r-MODE INSTABILITY REVISITED

- Physics
- 2011

We revisit the possibility and detectability of a stochastic gravitational wave (GW) background produced by a cosmological population of newborn neutron stars (NSs) with r-mode instabilities. The NS…

Improved upper limits on the stochastic gravitational-wave background from 2009-2010 LIGO and Virgo data.

- Medicine, PhysicsPhysical review letters
- 2014

A search for the stochastic background with the latest data from the LIGO and Virgo detectors shows no evidence of a stochastically gravitational-wave signal, and the limits in these four bands are the lowest direct measurements to date on the stoChastic background.

Stochastic Gravitational Wave Background from PBH-ABH Mergers

- Physics
- 2021

The measurement of gravitational waves produced by binary black-hole mergers at the Advanced LIGO has encouraged extensive studies on the stochastic gravitational wave background. Recent studies have…

Gravitational waves induced by the asymmetric jets of gamma-ray bursts

- PhysicsMonthly Notices of the Royal Astronomical Society
- 2018

We study the gravitational wave (GW) production induced by the asymmetric jets of gamma-ray bursts (GRBs). The asymmetric jets result in a recoil force acted on the central compact object, whose…

Upper limits on the isotropic gravitational-wave background from Advanced LIGO and Advanced Virgo’s third observing run

- PhysicsPhysical Review D
- 2021

We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO’s and Advanced Virgo’s third observing run (O3) combined with upper limits from the…

Searching for the Stochastic Gravitational-Wave Background with Advanced LIGO and Advanced Virgo

- Physics
- 2017

The Advanced LIGO detectors have commenced observations with Advanced Virgo joining in the near future. Gravitational waves from the merger of binary black hole systems have been observed. A major…

Implications of the binary coalescence events found in O1 and O2 for the stochastic background of gravitational events

- Physics
- 2019

The Advanced LIGO and Advanced Virgo detectors have commenced observations. Gravitational waves from the merger of binary black hole systems and a binary neutron star system have been observed. A…

Scalar stochastic gravitational-wave background in Brans-Dicke theory of gravity

- PhysicsPhysical Review D
- 2019

We study the scalar stochastic gravitational-wave background (SGWB) from astrophysical sources, including compact binary mergers and stellar collapses, in the Bras-Dicke theory of gravity. By…

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