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

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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


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The Universe Speaks

LIGO & the a5empt to detect Gravita:onal Waves

With funding from the Na:onal Science Founda:on PHY-0757058

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The Universe Speaks

LIGO & the a5empt to detect Gravita:onal Waves

With funding from the Na:onal Science Founda:on PHY-0757058 By William Katzman, LIGO-SEC Program Leader

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Speaking through light

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Speaking through light

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Speaking through light

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Speaking through light

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Spectrum

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What if we could hear the universe?

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LIGO 
 Gravitational Wave Observing

  • Visible light, radio waves, ultraviolet,

infrared, microwaves, gamma rays are all electromagnetic waves – or LIGHT!

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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)

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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

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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.

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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.

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Einstein’s Gravity

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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.

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 Gravitational Waves

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If we could see space-:me…

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What if we were there?

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What is a black hole?

  • The escape velocity is greater than the speed
  • f light.
  • Light is the universe’s speed limit.
  • Radius of a black hole (non-spinning):

r = (2MG)/ c2 where r is radius M is the mass, G is a constant c is the constant of the speed

  • f light
  • radius = Mass x 1.5 x 10-27 meters/kg
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The Observatory

Livingston, Louisiana Hanford, Washington

Supported by NSF grants PHY-0917587, PHY-1506037, PHY-0757058

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Laser Interferometer

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The improved laser interferometer

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The improved laser interferometer

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Our Control room

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Our Control room

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What we saw GW150914

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What we “heard” GW150914

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Two black holes collide

  • Frequency change
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Two black holes collide

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

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

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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
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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

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What we’ve seen so far…

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Black Holes currently detected

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Why Care?

  • This is pure research…
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Why Care?

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

  • This is pure research…
  • May allow us to get a TOE (Theory of Everything)
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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

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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…?
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Journey of a G wave

Par:ally funded by the Na:onal Science Founda:on

Bio: Leader of LIGO’s Science Educa:on Center What is LIGO?