gravitational wave astronomy
play

Gravitational-Wave Astronomy 1060-711: Astronomical Observational - PowerPoint PPT Presentation

Gravitational-Wave Physics Gravitational-Wave Detectors Gravitational-Wave Astronomy Gravitational-Wave Astronomy 1060-711: Astronomical Observational Techniques and Instrumentation Guest Lecturer: Prof. John T. Whelan 2013 May 1


  1. Gravitational-Wave Physics Gravitational-Wave Detectors Gravitational-Wave Astronomy Gravitational-Wave Astronomy 1060-711: Astronomical Observational Techniques and Instrumentation Guest Lecturer: Prof. John T. Whelan 2013 May 1 Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  2. Gravitational-Wave Physics Gravitational-Wave Detectors Gravitational-Wave Astronomy References Creighton & Anderson, Gravitational-Wave Physics and Astronomy (Wiley, 2011). ISBN 978-3-527-40886-3 Maggiore, Gravitational Waves: Volume 1: Theory and Experiments (Oxford, 2007). ISBN 978-0-198-57074-5 Saulson, Fundamentals of Interferometric Gravitational Wave Detectors (World Scientific, 1994). ISBN 978-9-810-21820-1 Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  3. Gravitational-Wave Physics Gravitational-Wave Detectors Gravitational-Wave Astronomy Outline Gravitational-Wave Physics 1 Physical Motivation Mathematical Description Generation of Gravitational Waves Gravitational-Wave Detectors 2 Overview Details of Ground-Based Interferometers Prospects for Space-Based Interferometers Gravitational-Wave Astronomy 3 Gravitational Wave Sources Gravitational Wave Data Analysis Selected Results from First-Generation GW Detectors Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  4. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Outline Gravitational-Wave Physics 1 Physical Motivation Mathematical Description Generation of Gravitational Waves Gravitational-Wave Detectors 2 Overview Details of Ground-Based Interferometers Prospects for Space-Based Interferometers Gravitational-Wave Astronomy 3 Gravitational Wave Sources Gravitational Wave Data Analysis Selected Results from First-Generation GW Detectors Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  5. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Action at a Distance Newtonian gravity: mass generates gravitational field Lines of force point towards object Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  6. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Issues with Causality Move object; Newton says: lines point to new location Relativity says: can’t communicate faster than light to avoid paradoxes You could send me supraluminal messages via grav field Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  7. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravitational Speed Limit If I’m 10 light years away, I can’t know you moved the object 6 years ago Far away, gravitational field lines have to point to old location of the object Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  8. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravitational Shock Wave Sudden motion (acceleration) of object generates gravitational shock wave expanding at speed of light Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  9. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Ripples in the Gravitational Field Move object back & forth − → gravitational wave Same argument applies to electricity: can derive magnetism as relativistic effect accelerating charges generate electromagnetic waves propagating @ speed of light Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  10. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravitational Wave from Orbiting Mass? Move around in a circle Still get grav wave pattern, but looks a bit funny Time to move beyond simple pseudo-Newtonian picture Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  11. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravity + Causality = Gravitational Waves In Newtonian gravity, force dep on distance btwn objects If massive object suddenly moved, grav field at a distance would change instantaneously In relativity, no signal can travel faster than light − → time-dep grav fields must propagate like light waves Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  12. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravity as Geometry Minkowski Spacetime: ds 2 = − c 2 ( dt ) 2 + ( dx ) 2 + ( dy ) 2 + ( dz ) 2   tr     − c 2 dt 0 0 0 dt dx dx 0 1 0 0        = η µν dx µ dx ν =       dy dy 0 0 1 0      dz 0 0 0 1 dz General Spacetime:   tr     dx 0 dx 0 g 00 g 01 g 02 g 03 dx 1 dx 1 g 10 g 11 g 12 g 13 ds 2 =        = g µν dx µ dx ν       dx 2 dx 2 g 20 g 21 g 22 g 23      dx 3 dx 3 g 30 g 31 g 32 g 33 Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  13. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravitational Wave as Metric Perturbation For GW propagation & detection, work to 1st order in h µν ≡ difference btwn actual metric g µν & flat metric η µν : g µν = η µν + h µν ( h µν “small” in weak-field regime, e.g. for GW detection) Convenient choice of gauge is transverse-traceless: η νλ ∂ h µν η µν h µν = δ ij h ij = 0 h 0 µ = h µ 0 = 0 ∂ x λ = 0 In this gauge: Test particles w/constant coörds are freely falling Vacuum Einstein eqns = ⇒ wave equation for { h ij } : � � ∂ 2 − 1 ∂ t 2 + ∇ 2 h ij = 0 c 2 Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  14. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Gravitational Wave Polarization States Far from source, GW looks like plane wave prop along � k TT conditions mean, in convenient basis,     0 h + h × 0 { k i } ≡ k = 0 { h ij } ≡ h = h × − h + 0     1 0 0 0 � � � � t − x 3 t − x 3 where h + and h × are components c c in “plus” and “cross” polarization states More generally � � � � � � k · � k · � r r ↔ ↔ ↔ = h + t − + + h × t − h e e × c c Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  15. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves The Polarization Basis wave propagating along � k ; ↔ + , × from ⊥ unit vectors � ℓ & � construct e m : ↔ ↔ + = � ℓ ⊗ � × = � m ⊗ � ℓ − � m ⊗ � ℓ ⊗ � m + � e m e ℓ Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  16. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Effects of Gravitational Wave Fluctuating geom changes distances btwn particles in free-fall: Plus ( + ) Polarization Cross ( × ) Polarization Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

  17. Gravitational-Wave Physics Physical Motivation Gravitational-Wave Detectors Mathematical Description Gravitational-Wave Astronomy Generation of Gravitational Waves Multipole Expansion for Gravitational Radiation “Electric Dipole”? � � No, “dipole moment” r dm ∝ ctr of mass COM can’t oscillate (also no negative “charge” in GR) “Magnetic Dipole”? No, “mag moment” � � 1 r × � v dm ∝ spin, another conserved quantity 2 “Electric Quadrupole”? Yes! In TT gauge, h ij ( t ) = 2 G c 4 d P TT � ij ¨ k k ℓ − I k ℓ ( t − d / c ) in terms of mass quadrupole moment � � � r 2 − I ij = r i r j − δ ij dm 3 Astronomical Observational Techniques and Instrumentation Gravitational-Wave Astronomy

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend