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Zwerger Muller SN waveforms

Zwerger Muller SN waveforms. The 78 ZM waveforms differ in initial angular momentum they have (A parameter), governing degree of differential rotation initial rotational energy (B, or b = E rot /E pot ). A,B roughly govern how many bounce peaks are in the waveform, as seen on the left.

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Zwerger Muller SN waveforms

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  1. Zwerger Muller SN waveforms • The 78 ZM waveforms differ in • initial angular momentum they have (A parameter), governing degree of differential rotation • initial rotational energy (B, or b = Erot/Epot). A,B roughly govern how many bounce peaks are in the waveform, as seen on the left. • Within each (AB) set, the adiabatic index Gr is varied from 1.325 to 1.28 (stiff to soft), and the peak amplidue of the wave depends strongly on this parameter, as seen in the right. AJW, Caltech, LIGO Project

  2. SineGaussians Sine Gaussians, f0 evenly spaced in logf Left: t = 0.05 s, Df = 6.3 Hz Middle: t = 0.005 s, Df = 63 Hz Right: t = 10/f0 , Df ~ /f0 AJW, Caltech, LIGO Project

  3. sensitivity with PZ fit to S1H2 My reconstruction with Mike’s PZ fit, on left. Right: Calibration web page. They agree very well. AND, the burst at 100 Hz injected into LDAS and passed through the response function in datacond, agrees perfectly with the matlab simulation. Confidence in use of response function! AJW, Caltech, LIGO Project

  4. Same for S1H1 AJW, Caltech, LIGO Project

  5. And for L1 AJW, Caltech, LIGO Project

  6. AJW, Caltech, LIGO Project

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