Analytic CCSN Waveforms: 2. Accretion Disk Instabilities

Document #:

LIGO-T1100093-v2

Document type:

T - Technical notes

Abstract:

We derive the gravitational wave emission from accretion disk instabilities in long gamma-ray bursts or black-hole forming core-collapse supernovae based on simple analytic models of van Putten and Piro & Pfahl.

Files in Document:

• disk_instabilities.pdf (file is not accessible)
• pirowf.pdf (file is not accessible)
• doc class (ligovirgodcc.cls, file is not accessible)

Other Files:

• disk_instabilities.tex (file is not accessible)
• pirogw.py (file is not accessible)
• vPwf.pdf (file is not accessible)
• vanPuttengw.py (file is not accessible)

Topics:

• Astrophysics / Multi-messenger
• GW source predictions
• GW Bursts

Authors:

• Christian David Ott
• Lucia Santamaria Lara

Notes and Changes:

Update with the following improvements:
- more detailed derivations
- change of the Piro fragmentation-type instability waveforms; the orbital angular velocity for these waveforms is now based on the sum of BH mass and fragment mass.