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Davidson Scholars Lecture Einstein, Black Holes and Gravity Waves, oh my! Prof David Toback Prof. David Toback Texas A&M University Mitchell Institute for April 2016 David Toback, Davidson Scholars Mitchell Institute for Fundamental Physics and Astronomy April 2016

Davidson Scholars Lecture - Texas A&M Universitytobackgroup.physics.tamu.edu/.../Davidson_2016_04_v1.pdf · 2016. 4. 9. · Davidson Scholars Lecture Einstein, Black Holes and Gravity

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  • Davidson Scholars Lecture

    Einstein, Black Holes and Gravity Waves, oh my!

    Prof David TobackProf. David TobackTexas A&M UniversityMitchell Institute for

    April 2016 David Toback, Davidson Scholars

    Mitchell Institute for Fundamental Physics and Astronomy

    April 2016

  • Outline• Quick overview of what happenedB k k d l f h • Backtrack and learn some of the physics, especially General Relativity – Gravity, Black holes and Gravity waves

    • Back to the discovery of Gravity Waves

    • Why it’s important in many ways, and why it’s not that new in others

    April 2016 David Toback, Davidson Scholars

    why it s not that new in others

    2

  • 50 Word Summary• About a billion years ago (billion light-years

    away), two 30MSun black holes spiraled in away), two 30MSun black holes sp raled n together to create a ~55MSun black hole

    • This merger was so violent that it emitted a ghuge amount of energy in gravity waves (about 5 solar masses) over a short amount f i h l di d h of time that were recently discovered here

    on Earth by the LIGO experimentN t Thi i NOT th di f th Note: This is NOT the discovery of the

    century (IMHO), it is the discovery that took a century

    April 2016 David Toback, Davidson Scholars

    took a century– Although it IS pretty awesome

    3

  • Einstein in the 1910’s• In the early 1910’s Einstein

    was thinking about some t i t l lt recent experimental results

    that didn’t make any sense to him using Newton’s gtheories

    • Decided we need new ways of thinking about space time thinking about space, time and Gravity

    • Einstein says that Newton’s L ’t ll it Laws aren’t really quite right…

    • Einstein’s theory is known as 2nd year Grad School Course

    April 2016 David Toback, Davidson Scholars 4

    E nst n s th ory s nown as the “General Theory of Relativity”

    School Course

  • Newton vs. Einstein

    Newton: The Earth moves around the Sun because of “the force of the Sun because of the force of gravity” is pulling it

    Einstein: There is no “force” of Einstein: There is no force of Gravity, the Earth moves in a “straight line” around the Sun in straight line around the Sun in the curved space-time created by the Sun

    This is a VERY different way of thinking about things

    April 2016 David Toback, Davidson Scholars 5

    thinking about things…

  • Curved Space?An analogy is t think f to think of curved space-time as looking as looking like one of th s r vit those gravity wells you’ve

    April 2016 David Toback, Davidson Scholars 6

    yprobably seen 1st floor of the Mitchell Physics building (MPHY)

  • Another Weird Thing: Mass Curves Space-TimeCurves Space-Time

    Think of each of the heavy things in the h a y th ngs n th universe (stars, planets etc.) like a ball in the middle of a ball in the middle of a taut rubber sheet that represents pspace-time

    The weight of the ball ill k it i k i t will make it sink into

    the rubber sheet, creating a cone

    April 2016 David Toback, Davidson Scholars 7

    creating a cone shaped dent around it

  • Mass Curves Space

    The heavier the ball, the bigger the dent in space-time!April 2016 David Toback, Davidson Scholars 8

    bigger the dent in space time!

  • Mass in curved space-timeA mass moves in a

    “straight line” in straight line in curved space-time

    In this example this In this example, this straight line in curved space-time pmakes the path of the small ball looklik thi i like something is pushing it toward the big ball in 3-

    April 2016 David Toback, Davidson Scholars 9

    the big ball in 3-dimensions

  • The Earth and the Sun

    Newton: The Earth moves around the Sun because of “the force of gravity” is pulling itbecause of the force of gravity is pulling it

    Einstein: There is no force, the Earth moves in a straight line in four dimensions, but the

    d d th S k it i

    April 2016 David Toback, Davidson Scholars 10

    curved space around the Sun makes it go in an orbit in the three space dimensions

  • The way the Planets go Around the Sun in General Relativitythe Sun in General Relativity

    April 2016 David Toback, Davidson Scholars 11

  • From Curved Space Time to Gravity WavesGravity Waves

    • If I have a star, or black hole, just sitting in space then other things know where it is because of the curvature of space-timeIf i j i i h ( i i h • If its just sitting there (or moving with a constant velocity) space-time isn’t changingIf it l t th thi i f ti i • If it accelerates, then this information is passed through space-time at the speed of light as gravity waveslight as gravity waves– Similar to if an electric charge was accelerated or if I dropped a rock in

    April 2016 David Toback, Davidson Scholars

    accelerated, or if I dropped a rock in water (or dragged my finger through it).

    12

  • First Indirect Evidence of Gravity WavesGravity Waves

    • In 1974, Taylor and Hulse discovered two neutron stars discovered two neutron stars (one of which was a Pulsar which is VERY bright) orbiting each othereach other

    • They measured the period (how fast they orbit) and saw that they were CLEARLY slowing they were CLEARLY slowing down

    • Why were they losing energy? They were emitting gravity They were emitting gravity waves exactly as predicted by General Relativity – Nobel Prize 1993

    April 2016 David Toback, Davidson Scholars

    Nobel Prize 1993– Been looking for DIRECT

    detection ever since13

  • Two Black Holes Colliding/Gravity WavesGravity Waves

    From the Warp of Space-From the Warp of SpaceTime Point of view

    https://www.youtube.com/wt h? fd f0TL2Uatch?v=qfdygf0TL2U

    April 2016 David Toback, Davidson Scholars 14

  • Gravity Waves Moving Through SpaceSpace

    A good set of short clips that A good set of short clips that help tell the story, including how the gravity waves got to

    us and how they were detected us and how they were detected https://www.youtube.com/watch

    ?v=FlDtXIBrAYE

    April 2016 David Toback, Davidson Scholars 15

  • April 2016 David Toback, Davidson Scholars 16

  • April 2016 David Toback, Davidson Scholars 17

  • What the Data Looked LikeRipples In Space-Time that reached us from two ~30M Black Holes as from two ~30MSun Black Holes as they spiral into each other about a billion light years awaybillion light-years away

    April 2016 David Toback, Davidson Scholars 18

  • Conclusion• The first direct observation of gravity waves is very

    exciting, and many years in the makingg, y y g• This allows us to see things we’ve never seen before

    that don’t produce lightL f f ll b d• Lots of fun questions still remain to be answered– How often does this happen in the universe?

    Where did 30 solar mass black holes COME – Where did 30 solar mass black holes COME FROM?

    – What other new and exciting things will come g gfrom this powerful new technology?

    • Enjoy!

    April 2016 David Toback, Davidson Scholars 19

  • Interested in learning more?• Physics department offers a

    course entitled “Big Bang & Black Holes”

    (ASTR/PHYS 109)– Covers Stephen Hawking’s “Brief

    History of Time”O i i d E l ti f th U i– Origin and Evolution of the Universe

    – How do stars form?– What is Dark Matter? Dark Energy?

    Wh t Bl k H l ?– What are Black Holes?– More on General Relativity, Quantum

    Mechanics and Particle PhysicsHas a lab (if you want)– Has a lab (if you want)

    – There is an option to take is an Honors class

    April 2016 David Toback, Davidson Scholarshttp://people.physics.tamu.edu/toback/109/