Source orientation - PowerPoint PPT Presentation

Testing GR with LISA

Testing GR with LISA. Leor Barack University of Southampton. Why is LISA a good lab for fundamental physics?. Sources are of high SNR and/or long duration  Lots of info in waveform (note: “signal”=amplitude, not energy!) Sources abundant  can repeat experiment with different sources

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References

Marc Lalancette marc.lalancette@sickkids.ca Diagnostic Imaging, The Hospital for Sick Children, Toronto, Ontario, Canada. Rotational invariance and source orientation in LCMV vector beamformer. Introduction. Proposed new constraints and weights (highlighted), and results.

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