Repulsive Gravity & the Cosmological Constant
Outline
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Observational Evidence
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repulsive gravity in General Relativity
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Inflation
Observational Evidence for Accelerating Expansion
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Hubble showed that the Universe is expanding
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But, is it speeding up or slowing down?
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normal matter + gravity should make it slow down
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but how do we know for sure?
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improved "Hubble Diagram"
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here's Hubble's original:
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x-axis is distance, y-axis is velocity
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How to do a better job
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get a more accurate distance indicator
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which can be seen at very large distances
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Supernovae of type Ia
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these are white dwarfs in binary systems which accrete mass
from their partner
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when M grows to ~ Mch= 1.4Msun, the
carbon-oxygen white dwarf has a spectacular nuclear explosion that totally
disrupts the star
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probably always happens at the same mass
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no outer layers to make things messy
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the core collapse Supernovae (type II) are messy because
of the outer layers of the massive star
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making a Hubble diagram:
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1st, find some supernovae at high redshift (here's
an example from HST )
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(note: HST is not actually used for a SN search - discoveries
come from the ground)
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confirm that the supernovae are of type Ia with a spectrum
(usually with the Keck 10-m telescope)
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use that same spectrum to measure the redshift
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measure the brightness of the supernova as it brightens and
then fades and compare to nearby supernovae like this one:
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Here are some SN brightness measurements. The curves are
the best fit SN light curve as determined from nearby supernovae
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Now determine the distance to the SN using
or 
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Plot d vs. v to get a Hubble diagram
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here's one from the High-z Supernovae Search Team:
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The "distance modulus" plotted on the y-axis is a peculiar distance
unit used by astronomers. It is equal to 5*log(distance/10 pc) so the
most distant SN on this plot is at about 7.6 billion pc.)
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for equal time, here's one from the Supernova Cosmology Project:
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both plots show redshift z vs. a logarithmic measure
of brightness (and therefore distance)
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So, what's the result?
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Why is Saul Permuter (leader of the SN Cosmology Project)
so happy?
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It's not because his preliminary conclusion from the supernova
video has been confirmed!
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perhaps its because the SN result is Science Magazine's Breakthrough
of the Year for 1998:
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To be fair, this is a discovery by two groups. Here's Brian
Schmidt, leader of the High-z SN Search:
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Prof. Peter Garnavich is also a member of the High-z SN Search
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So, what's going on here?
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Take a look at the bottom panel of the High-Z Hubble diagram:
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This plot has the brightnesses scaled to the expectation
for an empty Universe
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the white straight line represents an empty
= 0,
= 0 Universe
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note that
=
+
is the total density in
ordinary matter
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the magenta line
curving upward represents a
= 0,
= 1 Universe
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the SN appear to be slightly fainter than in the empty Universe
case
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expansion is accelerating
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the green line
curving downward represents a
= 1,
= 0 Universe
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the SN appear to be slightly fainter than in the brighter
Universe case
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expansion is slowing down
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this was the expected case a few years ago
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Conclusion, the Universe seems to be that the expansion of
the Universe is accelerating, but not as fast as the empty Universe
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this is good, because the Universe isn't empty!
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Here are the results from the SCP and the Hi-Z SN for a fit
to the best values of
&
:
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Both groups prefer
=
0.3 &
= 0.7.
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theory seems to prefer
+
= 1 (a flat Universe)
Repulsion in Einstein Theory of Gravity
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How can we understand gravitational repulsion in Einstein's
theory?
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isn't gravity just an attractive force? (i.e. doesn't it
just suck?)
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Gravity doesn't just depend on mass, but it depends of velocity,
too.
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gravitational acceleration

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or
in our usual notation
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the density,
> 0 for any type of matter
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the presure, p = 0 for normal slowly moving matter
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and p/c2 =
/3
for radiation (matter moving at v=c)
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for radiation
+
3p/c2 = 2
, so radiation
yields a stronger gravitational attraction than ordinary matter moving
at v << c.
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if we had negative pressure, we might get
+
3p/c2 < 0 which would give a positive acceleration.
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What is negative pressure?
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it pulls instead of pushes
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stretch a rubber band and it pulls, so it has negative pressure
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but p/c2 <<
for a rubber band, so the modification of the gravitational force is tiny
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when you let it go, the tension quickly converts into energy
of motion which gives a positive pressure.
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a hypothetical cosmic string is like a rubber band with a
very high tension
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stretch it and let it go, and it will oscillate at v ~
c.
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it only pulls in 1 of 3 directions, so it has p/c2
= -(1/3)

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or
+ 3p/c2
= 0, so a stationary cosmic string causes no gravitational acceleration
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if you stretch it and let it go, it develops a high velocity
which gives a positive contribution to the pressure
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so an oscillating loop of cosmic string will give an attractive
gravitational force.
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To get gravitational repulsion, we need something with a
very strong tension in 2 or 3 dimensions
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3 dimensions is best, and stuff that has the maximal amount
of tension in 3 dimensions is called "false vacuum"
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"false vacuum" has p/c2 = -
or
+ 3p/c2
= -2
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this is the most negative pressure that is allowed by General
Relativity
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What does this negative pressure mean?
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"false vacuum" has the peculiar property that the energy
density
is a constant
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suppose you have a piston full of ordinary matter.
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squeeze the piston and the density of matter increases
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you must input a lot of energy to squeeze it because the
pressure of the ordinary matter is pushing against you
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now, suppose you have a piston full of "false vacuum"
matter
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you don't need to squeeze it because the negative pressure
will cause it to squeeze itself
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the "false vacuum" can produce energy - it will pull you
with the piston if you are holding on
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the "false vacuum's" mass energy is proportional to its volume
(i.e. through E=mc2)
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it is 100% efficient at convering mass to energy (compared
to < 1% for nuclear reactions)
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Why is it called false vacuum?
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vacuum means essentially nothing
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a false vacuum is like a vacuum (i.e. no oridinary matter
or radiation)
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but, it has this extra energy density
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if space was filled with a false vacuum we couldn't easily
tell
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energy only comes out if we convert the false vacuum to something
else