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The Universe Speaks LIGO & the a5empt to detect Gravita:onal - PowerPoint PPT Presentation

The Universe Speaks LIGO & the a5empt to detect Gravita:onal Waves With funding from the Na:onal Science Founda:on PHY-0757058 The Universe Speaks LIGO & the a5empt to detect Gravita:onal Waves By William Katzman, LIGO-SEC Program


  1. The Universe Speaks LIGO & the a5empt to detect Gravita:onal Waves With funding from the Na:onal Science Founda:on PHY-0757058

  2. The Universe Speaks LIGO & the a5empt to detect Gravita:onal Waves By William Katzman, LIGO-SEC Program Leader With funding from the Na:onal Science Founda:on PHY-0757058

  3. Speaking through light

  4. Speaking through light

  5. Speaking through light

  6. Speaking through light

  7. Spectrum

  8. What if we could hear the universe?

  9. LIGO 
 Gravitational Wave Observing • Visible light, radio waves, ultraviolet, infrared, microwaves, gamma rays are all electromagnetic waves – or LIGHT!

  10. LIGO 
 Gravitational Wave Observing • Visible light, radio waves, ultraviolet, infrared, microwaves, gamma rays are all electromagnetic waves – or LIGHT! • Light can be blocked & scattered...Gravity waves can ’ t (practically speaking)

  11. LIGO 
 Gravitational Wave Observing • Visible light, radio waves, ultraviolet, infrared, microwaves, gamma rays are all electromagnetic waves – or LIGHT! • Light can be blocked & scattered...Gravity waves can ’ t (practically speaking) • Light travels through space & time – gravity is a change OF space-time

  12. LIGO 
 Gravitational Wave Observing • Visible light, radio waves, ultraviolet, infrared, microwaves, gamma rays are all electromagnetic waves – or LIGHT! • Light can be blocked & scattered...Gravity waves can ’ t (practically speaking) • Light travels through space & time – gravity is a change OF space-time • Shake a charge you get light. • Shake a mass you get a gravitational wave.

  13. Newton’s Gravity Newton ’ s Gravity Two Masses attract at a distance. If the sun were to disappear the planets fly off in a straight line immediately.

  14. Einstein’s Gravity

  15. Warped Space:me – Gravity Fields • We can use Lycra/Spandex on embroidery hoops to model space:me & a metal sphere as a star. • A wave in that fabric is the analogue to a gravita:onal wave.

  16. 
 Gravitational Waves

  17. If we could see space-:me…

  18. What if we were there?

  19. What is a black hole? • The escape velocity is greater than the speed of light. • Light is the universe’s speed limit. • Radius of a black hole (non-spinning): r = (2MG)/ c 2 where r is radius M is the mass, G is a constant c is the constant of the speed of light • radius = Mass x 1.5 x 10 -27 meters/kg

  20. The Observatory Livingston, Louisiana Hanford, Washington Supported by NSF grants PHY-0917587, PHY-1506037, PHY-0757058

  21. Laser Interferometer

  22. The improved laser interferometer

  23. The improved laser interferometer

  24. Our Control room

  25. Our Control room

  26. What we saw GW150914

  27. What we “heard” GW150914

  28. Two black holes collide • Frequency change

  29. Two black holes collide • Frequency change • Over a billion years ago

  30. Two black holes collide • Frequency change • Over a billion years ago • 2 black holes (36 solar mass and 29 solar mass)

  31. Two black holes collide • Frequency change • Over a billion years ago • 2 black holes (36 solar mass and 29 solar mass) • 36 + 29 = 62 + 3 solar mass radiated – Equivalent to 1 million earth’s energy

  32. Two black holes collide • Frequency change • Over a billion years ago • 2 black holes (36 solar mass and 29 solar mass) • 36 + 29 = 62 + 3 solar mass radiated – Equivalent to 1 million earth’s energy • More power than all the stars in the universe

  33. Two black holes collide • Frequency change • Over a billion years ago • 2 black holes (36 solar mass and 29 solar mass) • 36 + 29 = 62 + 3 solar mass radiated – Equivalent to 1 million earth’s energy • More power than all the stars in the universe • Just the beginning…other instruments such as LISA and the Pulsar Timing Array

  34. What we’ve seen so far…

  35. Black Holes currently detected

  36. Why Care? • This is pure research…

  37. Why Care? • This is pure research… • May allow us to get a TOE

  38. Why Care? • This is pure research… • May allow us to get a TOE (Theory of Everything)

  39. Why Care? • This is pure research… • May allow us to get a TOE (Theory of Everything) • Current results…include most stable lasers, new processes for crea:ng mirrors, and smart people

  40. Why Care? • This is pure research… • May allow us to get a TOE (Theory of Everything) • Current results…include most stable lasers, new processes for crea:ng mirrors, and smart people • Future results…?

  41. Journey of a G wave Bio: Leader of LIGO’s Science Educa:on Center What is LIGO? Par:ally funded by the Na:onal Science Founda:on

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