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TheCOSMIC WEB
Cosmic
THE
Web
Peter Coles
BLOG: http://telescoper.wordpress.com
The Hubble Expansion
DS
U

2dFGRS
The Cosmic Web of
Ideas
DarkTHE
matter

COSMIC WEB
Dark

Energy

The Big
Bang
Cosmic
Inflation

General
Relativity
THE COSMIC WEB
The Stretching of Light!
The Cosmic Microwave
Background
• Discovered by accident by Penzias &
Wilson (1965); Nobel Prize in 1978.
• Thermal (“black body”) radiation with a
temperature about 3 degrees above
absolute zero
• This radiation was produced when the
Universe was 1000 times smaller, and
1000 times hotter
• The “Smoking Gun” of the Big Bang
What put the Bang in Big
Bang?
• A “bang” must involve sound waves…
• These could have been generated
during the inflationary era by quantum
processes
• These are random noise with a
particular spectrum
• Gravity eventually turns these into
galaxies and clusters of galaxies
Planck Time!
What put the Bang in Big
Bang?
• If there was a “Big Bang” there
must have been sound waves…
• These could have been generated
in the very early Universe
• They started the process by which
galaxies and stars eventually
formed.
The Big Bang theory is not
complete!
• There are infinitely many possible big
bang universes described by the same
equations, but with different initial
conditions.
• Some expand forever, some recollapse.
• We have to use observations to pick
which of the big bang family is closest
to our universe.
Dark Matter…..
• Most of the matter in the Universe
is dark..
• “Dark Matter” can be detected in
galaxies and galaxy clusters.
• Observations suggest Ω0≈0.25, not
enough to close the Universe
• But the Universe appears flat...
• ….and it is accelerating!
Weighing Space
• As well as weighing individual
objects, it is also possible to weigh
the Universe as a whole
• To do this we need “standard rods”
or “standard candles” which we
view through curved space-time
• This can tell us about the
curvature of space-time.
Flat Space
Open Space

Closed Space
Dark Energy
• The “Cosmological Constant” (Λ) was
introduced by Einstein to make a static
universe (his “biggest blunder”)
• Now we think of Λ as “vacuum energy”
that causes the expansion Universe to
speed up..
• The vacuum energy is directly
connected to the microscopic physics of
elementary particles.
fainter
The Accelerating Universe
• Gravity pulls “normal” matter and
energy; it doesn’t push.
• It is possible to engineer anti-gravity,
but only with peculiar energy called
“Vacuum Energy” or “Dark Energy”
• This is the idea behind inflation in the
early Universe ..
• ..and possibly why the Universe
accelerates now
“CONCORDANCE”
Precision Cosmology
“…as we know, there are known knowns;

there are things we know we know. We
also know there are known unknowns;
that is to say we know there are some
things we do not know. But there are also
unknown unknowns -- the ones we don't
know we don't know.”

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The Cosmic Web - Evening Lecture at Sussex University on 9th December 2013

  • 1. TheCOSMIC WEB Cosmic THE Web Peter Coles BLOG: http://telescoper.wordpress.com
  • 2.
  • 3.
  • 4.
  • 5.
  • 6.
  • 7.
  • 9.
  • 10.
  • 11.
  • 12.
  • 13.
  • 14.
  • 15.
  • 17.
  • 18. The Cosmic Web of Ideas DarkTHE matter COSMIC WEB Dark Energy The Big Bang Cosmic Inflation General Relativity
  • 21.
  • 22.
  • 23.
  • 24.
  • 25. The Cosmic Microwave Background • Discovered by accident by Penzias & Wilson (1965); Nobel Prize in 1978. • Thermal (“black body”) radiation with a temperature about 3 degrees above absolute zero • This radiation was produced when the Universe was 1000 times smaller, and 1000 times hotter • The “Smoking Gun” of the Big Bang
  • 26.
  • 27.
  • 28.
  • 29.
  • 30. What put the Bang in Big Bang? • A “bang” must involve sound waves… • These could have been generated during the inflationary era by quantum processes • These are random noise with a particular spectrum • Gravity eventually turns these into galaxies and clusters of galaxies
  • 31.
  • 32.
  • 33.
  • 35.
  • 36. What put the Bang in Big Bang? • If there was a “Big Bang” there must have been sound waves… • These could have been generated in the very early Universe • They started the process by which galaxies and stars eventually formed.
  • 37.
  • 38.
  • 39.
  • 40.
  • 41. The Big Bang theory is not complete! • There are infinitely many possible big bang universes described by the same equations, but with different initial conditions. • Some expand forever, some recollapse. • We have to use observations to pick which of the big bang family is closest to our universe.
  • 42.
  • 43. Dark Matter….. • Most of the matter in the Universe is dark.. • “Dark Matter” can be detected in galaxies and galaxy clusters. • Observations suggest Ω0≈0.25, not enough to close the Universe • But the Universe appears flat... • ….and it is accelerating!
  • 44.
  • 45.
  • 46.
  • 47. Weighing Space • As well as weighing individual objects, it is also possible to weigh the Universe as a whole • To do this we need “standard rods” or “standard candles” which we view through curved space-time • This can tell us about the curvature of space-time.
  • 48.
  • 49.
  • 51.
  • 52.
  • 53. Dark Energy • The “Cosmological Constant” (Λ) was introduced by Einstein to make a static universe (his “biggest blunder”) • Now we think of Λ as “vacuum energy” that causes the expansion Universe to speed up.. • The vacuum energy is directly connected to the microscopic physics of elementary particles.
  • 54.
  • 56. The Accelerating Universe • Gravity pulls “normal” matter and energy; it doesn’t push. • It is possible to engineer anti-gravity, but only with peculiar energy called “Vacuum Energy” or “Dark Energy” • This is the idea behind inflation in the early Universe .. • ..and possibly why the Universe accelerates now
  • 57.
  • 58.
  • 60.
  • 61. Precision Cosmology “…as we know, there are known knowns; there are things we know we know. We also know there are known unknowns; that is to say we know there are some things we do not know. But there are also unknown unknowns -- the ones we don't know we don't know.”