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Presentation . 2019
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Presentation . 2019
License: CC BY
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ZENODO
Presentation . 2019
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ZENODO
Other literature type . 2019
License: CC BY
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NANOGrav: progress toward detecting a SMBHB stochastic background

descriptionPublicationkeyboard_double_arrow_right Presentation , Other literature type 20 Nov 2019Publisher:Zenodo
Authors: Stinebring, Dan;

doi: 10.5281/zenodo.3563106 , 10.5281/zenodo.3548180 , 10.5281/zenodo.3548179 , 10.5281/zenodo.3563107

NANOGrav: progress toward detecting a SMBHB stochastic background

Abstract

The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) has recently released its 12.5 year data set. I will summarize the GW results and their implications for limits on Supermassive Black Hole Binaries through hierarchical galaxy merging. These limits are starting to substantially constrain models for SMBHB. We anticipate detection of the stochastic background of GWs from these sources within the next 3 - 7 years.

Lightning talk at GW4FP

Related Organizations
Keywords

pulsars, gravitational waves, fundamental physics, nanograv

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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
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