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Dark Matter, Dark Energy, and
the Fate of the Universe
Mass within Sun’s
orbit:
1011 MSun
Observable stars
and gas clouds:
~few 109 MSun
Dark Matter: An undetected form of mass that emits little or
no photons, but we know it must exist because we observe
the effects of its gravity
Dark Energy: An unknown form of energy that is causing
the universe to expand faster over time
Dark matter and dark energy
• “Normal” Matter: ~ 4.4%
– Normal Matter inside stars: ~ 0.6%
– Normal Matter outside stars: ~ 3.8%
• Dark Matter: ~ 25%
• Dark Energy ~ 71%
What is the Universe made of?
Spiral galaxies all tend to have flat rotation curves
indicating large amounts of dark matter
The visible
portion of a
galaxy lies
deep in the
heart of a
large halo of
dark matter
measure the
velocities of
galaxies in a
cluster from
their Doppler
shifts
Mass is 50 x
larger than
the mass in
stars!
Clusters contain
large amounts hot
gas: emits x rays
Temperature of hot
gas tells us cluster
mass:
85% dark matter
13% hot gas
2% stars
Gravitational lensing of background galaxies also tells us
the mass
• Ordinary Dark Matter (MACHOS)
– Massive Compact Halo Objects:
dead or failed stars in halos of galaxies
• Extraordinary Dark Matter (WIMPS)
– Weakly Interacting Massive Particles:
mysterious neutrino-like particles
The
Best
Bet
What is dark matter made of?
MACHOs do not
cause enough
lensing events to
explain all the
dark matter
• There’s not enough ordinary matter
• WIMPs could be left over from Big Bang
• Models involving WIMPs explain how galaxy
formation works
Why Believe in WIMPs?
Gravity of dark matter is what caused protogalactic clouds
to contract early in time

WIMPs don’t
contract to
center because
they don’t emit
photons, so
they can not
radiate away
their orbital
energy
Maps of galaxy positions reveal extremely large
structures: superclusters and voids
WIMP models agree better with observations
Critical
density of
matter
Not enough
dark matter
Fate of
universe
depends
on the
amount
of dark
matter
Lots of
dark matter
Amount of dark matter
is ~25% of the critical
density suggesting fate
is eternal expansion
Not enough
dark matter
But expansion
appears to be
speeding up!
Not enough
dark matter
Dark
Energy?
Brightness of distant white-dwarf supernovae tells us how
much universe has expanded since they exploded
Accelerating universe is best fit to supernova data

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dark-matter.ppt

  • 1. Dark Matter, Dark Energy, and the Fate of the Universe
  • 2. Mass within Sun’s orbit: 1011 MSun Observable stars and gas clouds: ~few 109 MSun
  • 3. Dark Matter: An undetected form of mass that emits little or no photons, but we know it must exist because we observe the effects of its gravity Dark Energy: An unknown form of energy that is causing the universe to expand faster over time Dark matter and dark energy
  • 4. • “Normal” Matter: ~ 4.4% – Normal Matter inside stars: ~ 0.6% – Normal Matter outside stars: ~ 3.8% • Dark Matter: ~ 25% • Dark Energy ~ 71% What is the Universe made of?
  • 5.
  • 6. Spiral galaxies all tend to have flat rotation curves indicating large amounts of dark matter
  • 7. The visible portion of a galaxy lies deep in the heart of a large halo of dark matter
  • 8. measure the velocities of galaxies in a cluster from their Doppler shifts Mass is 50 x larger than the mass in stars!
  • 9. Clusters contain large amounts hot gas: emits x rays Temperature of hot gas tells us cluster mass: 85% dark matter 13% hot gas 2% stars
  • 10. Gravitational lensing of background galaxies also tells us the mass
  • 11.
  • 12.
  • 13.
  • 14. • Ordinary Dark Matter (MACHOS) – Massive Compact Halo Objects: dead or failed stars in halos of galaxies • Extraordinary Dark Matter (WIMPS) – Weakly Interacting Massive Particles: mysterious neutrino-like particles The Best Bet What is dark matter made of?
  • 15. MACHOs do not cause enough lensing events to explain all the dark matter
  • 16. • There’s not enough ordinary matter • WIMPs could be left over from Big Bang • Models involving WIMPs explain how galaxy formation works Why Believe in WIMPs?
  • 17. Gravity of dark matter is what caused protogalactic clouds to contract early in time 
  • 18. WIMPs don’t contract to center because they don’t emit photons, so they can not radiate away their orbital energy
  • 19. Maps of galaxy positions reveal extremely large structures: superclusters and voids
  • 20. WIMP models agree better with observations
  • 21. Critical density of matter Not enough dark matter Fate of universe depends on the amount of dark matter Lots of dark matter
  • 22. Amount of dark matter is ~25% of the critical density suggesting fate is eternal expansion Not enough dark matter
  • 23. But expansion appears to be speeding up! Not enough dark matter Dark Energy?
  • 24. Brightness of distant white-dwarf supernovae tells us how much universe has expanded since they exploded
  • 25. Accelerating universe is best fit to supernova data