Potpourri: Gravity - PowerPoint PPT Presentation

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Potpourri: Gravity

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Title: Potpourri: Gravity


1
Potpourri Gravity
  • by 
  • Robert Nemiroff
  • Michigan Technological University

2
Physics X About This Course
  • Officially "Extraordinary Concepts in Physics"
  • Being taught for credit at Michigan Tech
  • Light on math, heavy on concepts
  • Anyone anywhere is welcome
  • No textbook required
  • Wikipedia, web links, and lectures only
  • Find all the lectures with Google at
  • "Starship Asterisk" then "Physics X" 
  • http//bb.nightskylive.net/asterisk/viewforum.php?
    f39

3
Birkhoff's Theorem
  • A very useful theorem that leverages spherical
    symmetry in General Relativity.  Two common
    applications
  •  
  • Outside a spherically symmetric mass distribution
    (hence not rotating), the solution is always the
    Schwarzschild metric. 
  • useful for ignoring stellar pulsations
  • Inside a spherically symmetric mass shell, the
    gravitational "field" will vanish. 
  • useful for ignoring the outside universe

4
Virial Theorem
  • A relation between the average total kinetic
    energy of a system of particles (Ktot) and the
    average potential energy of the particles (Vtot).
     For Newtonian gravity
  • 2 Ktot - Vtot
  • Useful for determining the amount of dark matter
    in clusters of galaxies (for example).  Theorem
    can apply to even one particle.

5
Gravothermal Catastrophe
  • The center of a gravitationally bound system of
    particles will heat up at it gravitationally
    collapses.  For those particles, the increase in
    energy comes from a conversion of potential
    energy to kinetic energy.
  • However, some other particles will be thrown out
    from the center and will "cool down".
  • Runaway For sufficiently condensed systems of
    particles acting gravitationally, the center will
    be unstable to becoming increasingly dense and
    hot, since that will decrease system entropy.  A
    single temperature will no longer describe the
    system.

6
Gravitomagnetism
  • A gravitational force that complements standard
    gravity like magnetism complements standard
    electric force.
  • Predicted by General Relativity (and even other
    gravitational theories that predate GR).
  • A small effect -- it is being tested by Gravity
    Probe B, although these results have not yet been
    announced.  

7
Gravitomagnetism
  • Typically a very small effect.
  • If two wheels are spun on a common axis, their
    mutual gravitational attraction will be
    (slightly) greater if they spin in opposite
    directions.
  • A ring rotating about its minor axis (a circle
    inside the ring) will accelerate matter through
    the ring while that matter feels no
    acceleration. 
  • Earth's gravitomagnetic acceleration at the
    Equator is about 10-7 g.
  • Cannot be used to create a perpetual motion
    machine.

8
Frame Dragging
  • The General Relativity expected effect that
    rotating objects drag spacetime around with them.
  •  
  • A gravitomagnetic effect.
  • Also known as the Lens-Thirring Effect
  • When near a massive rotating object, you may feel
    that you are not rotating with respect to the
    universe, even though you can see that you are.
  • Typically a small effect.

9
Frame Dragging
  • FD has never been measured in the laboratory
  • very difficult to do
  •  
  • Would rotating a bucket create the same effect as
    rotating the entire universe?
  •  
  • Might be relevant to jets emitted from active
    galaxies.

10
Gravitational Radiation
  • Emitted by accelerating masses in GR, in analogy
    to electromagnetic radiation emitted by
    accelerating charges.
  • Acceleration must be non-spherically symmetric.
  • Very weak compared to common photon energies.
  • Not yet directly detected on Earth.
  • Ongoing searches include LIGO

11
Gravitational Radiation
  • Strongly emitted by massive and rapidly changing
    astronomical objects.
  • Supernovas (we know)
  • Gamma ray bursts (we think)
  • Steadily emitted by decaying binary star systems
  • binary pulsar's orbital decay can be attributed
    to gravitational radiation to high accuracy

12
Gravitational Radiation
  • moves at the speed of light.
  • has wavelength and frequency like light lambda
    c f.
  • A passing polarized gravitational wave would have
    this effect on a ring of particles
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