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Dark Matter, Dark Energy, and the Fate of the Universe

Dark Matter, Dark Energy, and the Fate of the Universe

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Page 1: Dark Matter, Dark Energy, and the Fate of the Universe

Dark Matter, Dark Energy, and the Fate of the Universe

Page 2: 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

Page 3: Dark Matter, Dark Energy, and the Fate of the Universe

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

Page 4: Dark Matter, Dark Energy, and the Fate of the Universe

• “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?

Page 5: Dark Matter, Dark Energy, and the Fate of the Universe
Page 6: Dark Matter, Dark Energy, and the Fate of the Universe

Spiral galaxies all tend to have flat rotation curves indicating large amounts of dark matter

Page 7: Dark Matter, Dark Energy, and the Fate of the Universe

The visible portion of a galaxy lies deep in the heart of a large halo of dark matter

Page 8: Dark Matter, Dark Energy, and the Fate of the Universe

measure the velocities of galaxies in a cluster from their Doppler shifts

Mass is 50 x larger than the mass in stars!

Page 9: Dark Matter, Dark Energy, and the Fate of the Universe

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

Page 10: Dark Matter, Dark Energy, and the Fate of the Universe

Gravitational lensing of background galaxies also tells us the mass

Page 11: Dark Matter, Dark Energy, and the Fate of the Universe
Page 12: Dark Matter, Dark Energy, and the Fate of the Universe
Page 13: Dark Matter, Dark Energy, and the Fate of the Universe
Page 14: Dark Matter, Dark Energy, and the Fate of the Universe

• 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?

Page 15: Dark Matter, Dark Energy, and the Fate of the Universe

MACHOs do not cause enough lensing events to explain all the dark matter

Page 16: Dark Matter, Dark Energy, and the Fate of the Universe

• 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?

Page 17: Dark Matter, Dark Energy, and the Fate of the Universe

Gravity of dark matter is what caused protogalactic clouds to contract early in time

Page 18: Dark Matter, Dark Energy, and the Fate of the Universe

WIMPs don’t contract to center because they don’t emit photons, so they can not radiate away their orbital energy

Page 19: Dark Matter, Dark Energy, and the Fate of the Universe

Maps of galaxy positions reveal extremely large structures: superclusters and voids

Page 20: Dark Matter, Dark Energy, and the Fate of the Universe

WIMP models agree better with observations

Page 21: Dark Matter, Dark Energy, and the Fate of the Universe

Critical density of matter

Not enough dark matter

Fate of universe depends on the amount of dark matter

Lots of dark matter

Page 22: Dark Matter, Dark Energy, and the Fate of the Universe

Amount of dark matter is ~25% of the critical density suggesting fate is eternal expansion

Not enough dark matter

Page 23: Dark Matter, Dark Energy, and the Fate of the Universe

But expansion appears to be speeding up!

Not enough dark matter

Dark Energy?

Page 24: Dark Matter, Dark Energy, and the Fate of the Universe

Brightness of distant white-dwarf supernovae tells us how much universe has expanded since they exploded

Page 25: Dark Matter, Dark Energy, and the Fate of the Universe

Accelerating universe is best fit to supernova data