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[4097] Physics 316: Extragalactic Astronomy and Cosmology
(Summary of Lectures)
Lecture 30
In class there was a general discussion of the large-scale structure
(observed) in the universe
(much repeated from the
last lecture).
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The large-scale structure is also discussed in some detail
in
Bothun Chapt 3,
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which I expect you to be familiar with.
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Item discussed (but not in
Bothun Chapt 3):
Movies shown in class
From the movies & discussions
you have a good feel for the characteristics associated
with the various types of clustering (galaxies, clusters,
superclusters, "filaments", "voids").
However I also want you to know the typical size-scales
involved
and the problems & difficulties associated with
determining these characteristics, size-scales etc.
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Size
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"Structure"
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1 pc
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Separation between stars
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100 kpc
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Scale size for a large Galaxy
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1 Mpc
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Scale size for a typical Group of Galaxies
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10 Mpc
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Scale size for a large Cluster of Galaxies
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100 Mpc
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Scale size for a typical Supercluster
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100-300 Mpc
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Scale size for walls, filaments & voids
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5 Gpc
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size of our horizon c/H0
(assuming 1/H0 of ~1.5x1010 yrs)
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When reading about the various structures, keep in mind that
the various terms are usually used in fairly imprecise or "fuzzy" mannor.
There are no strict definitions for most of them.
- eg. what exactly constitutes a "void";
where a "void" ends, and
a "wall" begins;
when does a "filament" become a "sheet"
etc
This is because there is little point having such rigourous definitions
- the universe itself is "fuzzy"
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[Sect3.1]
- There is no time dependence on the gravitational potential
which is associated with a mass fluctuation
- Initial density fluctuations at the time of
recombination appear as fluctuations in the CMB
- Galaxies can be used as "tracers" of the
mass distribution
(at least the visible [baryonic] mass)
- Must be careful concerning any "bias"
- Effect of neighboring galaxies is that a galaxy
will not move in a
pure Hubble flow. i.e. "pure" expansion is
perturbed by the mass concentrations
- the resultant "peculiar velocities" makes measuring
distance more difficult.
- However, such motions
can be used as a diagnostic of the
the mass distribution (eg. within a cluster etc)
[Sect3.2]
- The velocity distribution is a poor predictor
as to whether a structure is gravitationally bound
(ie. whether it can be considered a "destrete entity")
- The presence of an X-ray emitting ICM is a
better means
of determining whether a "structure" is bound
- (plus physics & diagnostics of
cooling flows of course)
- There is clustering on a variety of scales
- groups & clusters
- chains of clusters (superclusters, "walls" &
"filaments")
- associated "voids" on various scales
- Various timescales for several of these
structures (eg groups & clusters)
are less than the age of the universe
- such structure can evolve significantly
- Most superclusters appear to be flattened structures
- Plus alignment of superclusters
often seems to match the alignment of
smaller scale structures.
- chance ?
- memory retention of structure collapse mechanism ?
(gravitational collapse & dynamical relaxation
ought to have erased these)
[Sect3.3]
[Sect3.4]
- the "light" (ie. electromagnetic radiation incl X-rays etc)
we detect from galaxies is not necessarily representative of
of all the baryonic matter in the universe
- as we have already discussed some (& will again in a later lecture)
Omegab < 1
- Omegatot = 1 is
is strongly suggested by the CMB results and
the observed abundances of the light elements
[Sect3.5]
- 2-D images of the sky are a good start, but the 3rd dimension
(redshift) is
obviously preferable to fully characterize and understand the
structures
- Redshifts are difficult to measure
for many faint/distant objects
- astrophysical problems associated with a lack of strong, easily
detected narrow features (with which to measure the redshift)
- in the optical band, stellar absorption lines are
often used - however these are relatively weak
& difficult (require long observations)
to measure with all but the largest telescopes
- in the radio,
the 21cm emission line due to hydrogen
is used. However, again large radio telescopes
are required (very few of these)
- "logistical" problems associated with the
observing time required
and large number of sources to be observed.
- (recent
& ongoing technical developments & dedicaded survey programs
have increased the
rate at which these studied can be performed)
- Redshift surveys generally take one of two approaches
There are uncertainties plus pros & cons with both approaches
- An artifact of the peculiar velocities is that
virialized structures (such as the core of a cluster)
appear as "straight line" when plotted in
angle-redshift space (same angle, range of redshifts).
- The (radial, towards/away from us)
components of the peculiar velocities
(due to gravitational attraction) breaks the direct
(Hubble) redshift-distance relation.
(Thus "sizes" are often quoted in velocity space).
- There are filaments & sheets/walls
that appear to be
at the intersections of voids
- The voids are devoid of bright galaxies
- there could be a population of much fainter galaxies
- (and/or dark matter)
[Sect3.6]
- Some of the issues and results regarding the
motion of the Local Group with respect to
Virgo, and in the general direction of
Hydra-Centarus Supercluster
were discussed in
Lecture 14
(see also
Homework 4).
- There is some form of large-scale "flow" that
"our" cluster/supercluster is participating in !
- Note: Sect 3.6.4 will be discussed briefly next time
(since there have been recent developments)
- The appearance of structure can/could be misleading
(optical illusions, and statistical fluctuations)
[Sect3.7]
- voids appear to be preferentially inhabited by
spiral galaxies
- can use the Tully-Fisher relation to estimate the
distances
and hence use the redshift (velocity)
to calculate the inflow/outflow
- Voids do indeed appear to be real
"structures" - they are
not an obvious artifact in redshift-space
- walls indeed appear to have a "thickness"
(ie "depth")
- walls appear to be relatively unevolving
structures
[Sect3.8]
- There have been suggestions of
a "really big flow".
- However results not confirmed using other techniques
- In disagreement with the
Dipole Anisotropy of the
CMB
Current feeling is that it unlikely
[Sect3.9]
- Peculiar velocities on large scales obviously must be
kept in mind when determining H0
- However there are obviously techniques for taking these into account.
- An example (and test of the method) is provided
by the relative distance between the Virgo &
Coma
clusters.
- These values are indeed generally consistent with the estimates
we have discussed before.
End of lecture
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