LIGO Document T1600262-v4
- We will look into the measurement and bounding of the speed of continuous
gravitational waves by comparing variances observed in long-term signals using
the motion of the detector relative to the source. We can use Doppler effects in
the phasing of these waves to get an estimate for their speed, even in the absence
of electromagnetic counterparts. However, in order to measure this speed, we
will use a known EM signal and measure its continuous wave partner.
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- Other Files:
- First_Project_Report.pdf (file is not accessible)
- Fourier Transform of the non-GR waveforms; higher deviations mean higher modes (FTOfGRDeviations.png, file is not accessible)
- Generates curves for any speed of CWs (AntennaFullGeometry.py, file is not accessible)
- Generates the curves for further use (nonGRCurves.py, file is not accessible)
- Implementation of MCMC in order to find given parameters (emceeFit.py, file is not accessible)
- Misc. constants used throughout (const.py, file is not accessible)
- Original code to demonstrate Roemer delay calculation (romerDelay.py, file is not accessible)
- Original project plan (Jake_Mattinson_SURF_Proposal_20160512.pdf, file is not accessible)
- Picture of generated GR waveform (line) and the treated data, just to check the ability to retrieve signal with c_g = c (CheckTheGRCase.png, file is not accessible)
- Picture of generated non-GR waveforms for various deviation values (WaveformsNotGR.png, file is not accessible)
- Presentation First Draft (Mattinson_Jake_Presentation_160816.ppt, file is not accessible)
- Presentation Second Draft (Mattinson_Jake_Presentation_170816.ppt, file is not accessible)
- Second project update (SecondProjectReport-JMattins.pdf, file is not accessible)
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