1 / 30

S. V. DHURANDHAR

THE CHANGING FACE OF GENERAL RELATIVITY. S. V. DHURANDHAR. IUCAA PUNE. General Relativity and other disciplines. GR finds its home in astronomy & astrophysics The binary blackhole problem No exact two body solution : PN + Numerical Relativity

forest
Download Presentation

S. V. DHURANDHAR

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. THE CHANGING FACE OF GENERAL RELATIVITY S. V. DHURANDHAR IUCAA PUNE 25th IAGRG meeting Kolkata

  2. General Relativity and other disciplines • GR finds its home in astronomy & astrophysics • The binary blackhole problem • No exact two body solution: PN + Numerical Relativity • Cosmology: observational data, COBE, WMAP, PLANCK • Mathematics: Commutative algebra, differential • geometry in statistics • Statistics: Hypothesis testing, statistical tests, maximum likelihood, etc. - Signal processing • Gravitation has gone experimental: Gravitational waves 25th IAGRG meeting Kolkata

  3. Effect on a ring of test particles Metric: General Wave: 25th IAGRG meeting Kolkata

  4. But h is awfully small ! Quadrupole formula : Change in arm-length: d L ~ h L 25th IAGRG meeting Kolkata

  5. LIGO Louisiana 4 km armlength (US) 25th IAGRG meeting Kolkata

  6. We did it ! *http://www.ligocaltech.edu/~lazz/distribution/LSC_Data 25th IAGRG meeting Kolkata

  7. LISA: Space based detector for detecting low frequency GW 25th IAGRG meeting Kolkata

  8. Laser frequency noise 25th IAGRG meeting Kolkata

  9. 25th IAGRG meeting Kolkata

  10. 25th IAGRG meeting Kolkata

  11. Tinto, Eastabrook, Armstrong; SVD, Nayak, Vinet, Pai 25th IAGRG meeting Kolkata

  12. 25th IAGRG meeting Kolkata

  13. 25th IAGRG meeting Kolkata

  14. 25th IAGRG meeting Kolkata

  15. 25th IAGRG meeting Kolkata

  16. Open Problems 25th IAGRG meeting Kolkata

  17. Inspiraling compact binaries GW • Broadband source best for interferometric detectors • Waveform is well modeled by PN approximations – waveform obtained to 3.5 PN • Numerical Relativity: great advances – merger • Signal is way below the noise – data analysis: filtering 25th IAGRG meeting Kolkata

  18. Breakthrough in Numerical Relativity • Numerical Relativity • solves • merger waveform • 3.5% of total restmass energy as compared to 1.5 % in inspiral waveform! Work in progress on stitching together waveforms India has the right talent/aptitude for NR 25th IAGRG meeting Kolkata

  19. Example of a filter A sinusoidal signal is embedded in noise Data: Signal: 25th IAGRG meeting Kolkata

  20. Filtering the data Best filter is the Fourier Transform: Statistic: Provides parameters of the signal: eg. frequency Generalisation: Matched Filter 25th IAGRG meeting Kolkata

  21. Matched filtering the inspiraling binary signal 25th IAGRG meeting Kolkata

  22. Statistics and geometry • Statistic: c(t) • Where does one set the threshold? – False alarm probability – choose threshold such that this is small • Detection probability: choose this high • Signal depends on many parameters: masses, kinematical parameters: initial phase, time of arrival … • Parameter space • Parameter space can be viewed as a manifold with the • parameters as coordinates • Metric: mismatch between signal and template 25th IAGRG meeting Kolkata

  23. Parameter space metric Coordinates: li gik Dli Dlk = e Choosecoordinates so that metric is simplest: Cartesian coordinates For inspiral choose chirp times instead of masses: t0 , t3 Metric const: Uniform placement of templates Number of templates = volume of parameter space / template size 25th IAGRG meeting Kolkata

  24. GEO: 0.6km VIRGO: 3km LIGO-LHO: 2km, 4km TAMA: 0.3km LIGO-LLO: 4km AIGO: (?)km International Network of GW Interferometers 1. Detection confidence 2. Source direction 3. Polarisation info 25th IAGRG meeting Kolkata

  25. Need for a (or two) detector(s) in Asia/Australia • AIGO: Australian project • INDIGO: Indian detector? • Advantages: sky coverage, resolution of sources 25th IAGRG meeting Kolkata

  26. Optimum location of a detector Courtesy A. Sengupta & S. Mitra 25th IAGRG meeting Kolkata

  27. Optimum location 25th IAGRG meeting Kolkata

  28. Network Sensitivity AIGO/INDIGO network doubles sensitivity 25th IAGRG meeting Kolkata

  29. Angular Resolution An order of magnitude improvement 25th IAGRG meeting Kolkata

  30. Summary • Connection of GR to several fields: • Astrophysics, Mathematics, Statistics, Engineering … • Numerical Relativity • Gravitation going experimental 25th IAGRG meeting Kolkata

More Related