https://frbtheorycat.org/index.php?title=KNBH-BH_(Magneto._Collapse)&feed=atom&action=history
KNBH-BH (Magneto. Collapse) - Revision history
2024-03-29T04:27:23Z
Revision history for this page on the wiki
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https://frbtheorycat.org/index.php?title=KNBH-BH_(Magneto._Collapse)&diff=248&oldid=prev
Jake Gordin at 09:38, 11 October 2018
2018-10-11T09:38:48Z
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<td colspan="2" style="background-color: #fff; color: #202122; text-align: center;">Revision as of 05:38, 11 October 2018</td>
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<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>|NeutrinoCounterpart = --</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>|NeutrinoCounterpart = --</div></td></tr>
<tr><td class="diff-marker" data-marker="−"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #ffe49c; vertical-align: top; white-space: pre-wrap;"><div>|References = <del style="font-weight: bold; text-decoration: none;">https</del>://<del style="font-weight: bold; text-decoration: none;">arxiv</del>.<del style="font-weight: bold; text-decoration: none;">org</del>/<del style="font-weight: bold; text-decoration: none;">pdf</del>/1602.06907<del style="font-weight: bold; text-decoration: none;">.pdf</del></div></td><td class="diff-marker" data-marker="+"></td><td style="color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #a3d3ff; vertical-align: top; white-space: pre-wrap;"><div>|References = <ins style="font-weight: bold; text-decoration: none;">http</ins>://<ins style="font-weight: bold; text-decoration: none;">adsabs</ins>.<ins style="font-weight: bold; text-decoration: none;">harvard.edu</ins>/<ins style="font-weight: bold; text-decoration: none;">cgi-bin</ins>/<ins style="font-weight: bold; text-decoration: none;">bib_query?arXiv:</ins>1602.06907</div></td></tr>
<tr><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>|Comments = Can only account for a sub-population of FRBs.</div></td><td class="diff-marker"></td><td style="background-color: #f8f9fa; color: #202122; font-size: 88%; border-style: solid; border-width: 1px 1px 1px 4px; border-radius: 0.33em; border-color: #eaecf0; vertical-align: top; white-space: pre-wrap;"><div>|Comments = Can only account for a sub-population of FRBs.</div></td></tr>
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Jake Gordin
https://frbtheorycat.org/index.php?title=KNBH-BH_(Magneto._Collapse)&diff=104&oldid=prev
Emma Platts: Created page with " <!-- Brings in the summary table --> <!-- This is an example. Change the right hand side of all these assignments --> {{FRBTableTemplate |Category = Merger |Pr..."
2018-09-26T18:46:17Z
<p>Created page with " <!-- Brings in the summary table --> <!-- This is an example. Change the right hand side of all these assignments --> {{FRBTableTemplate |Category = Merger |Pr..."</p>
<p><b>New page</b></p><div><br />
<br />
<!-- Brings in the summary table --><br />
<!-- This is an example. Change the right hand side of all these assignments --><br />
{{FRBTableTemplate<br />
|Category = Merger<br />
|Progenitor = KNBH-BH<br />
|Type = Single<br />
|EnergyMechanism = Mag. reconnection<br />
|EmissionMechanism = Curv.<br />
|LFRadioCounterpart = Yes<br />
|HFRadioCounterpart = Afterglow<br />
|MicrowaveCounterpart = --<br />
|THzCounterpart = --<br />
|OIRCounterpart = --<br />
|XrayCounterpart = --<br />
|GammarayCounterpart = Afterglow<br />
|GWCounterpart = Yes<br />
|NeutrinoCounterpart = --<br />
|References = https://arxiv.org/pdf/1602.06907.pdf<br />
|Comments = Can only account for a sub-population of FRBs.<br />
}}<br />
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== Model Description ==<br />
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For merging BH binaries in which at least one of the BHs is Kerr-Newman, instabilities due to tidal forces induce reconnection in the KNBH prior to coalescence. The magnetic field violently reconnects, triggering strong relativistic shock waves through the surrounding plasma to produce curvature radiation consistent with an FRB.<br />
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== Observational Constraints ==<br />
<br />
KNBHs have no thermal emission because they lack solid surfaces, and are non-pulsating because their magnetic and rotation axes are aligned.</div>
Emma Platts