Dark Matter in the Universe
Download
Report
Transcript Dark Matter in the Universe
[email protected]
DARK MATTER IN THE UNIVERSE
The Universe
What do we know about it
age: 14.6 billion years
Evolved from Big Bang
chemical composition
Structures in the universe
galaxy clusters
galaxies
voids
Separation of forces
gravity
strong force
weak force
what causes interaction?
gravity
electromagnetism
weak force
strong force
Some particle physics
Baryons: composed of three quarks
proton; the only long living hadron, t=1031s; measure for p
decay= test for GUT
Mesons: composed of one quark and one
antiquark
Baryons and mesons: hadrons
Hadrons are composed of quarksstrong
interaction
Leptons: no quarks, no strong interaction
Higgs particle, higgs field
mass=interaction of a particle
In empty space, the Higgs field has an
amplitude different from zero; i.e., a nonzero vacuum expectation value.
The existence of this non-zero vacuum
expectation plays a fundamental role: it gives
mass to every elementary particle which has
mass, including the Higgs boson itself.
Galaxies
Clusters
Das galaktische Zentrum
La voie lactee
The solar neighborhood
Galaxis
200-400 109 Sterne
Durchm.: 100 000 Lj
Rotation: Ort der Sonne
etwa 200 Mill Jahre
Determination of the mass of
a galaxy
2
v
Mm
m G 2
r
r
Star
Galactic center
centrigual force
attraction
Solarsystem…
Merkury: 88 days
Earth: 1 year
Jupiter: 11,6 years…
Galactic rotation curve
v (R)
Kepler
Kepler Rotation of a Galaxy
1.2
1
velocity
0.8
0.6
0.4
0.2
0
0
2
4
6
8
distance from galactic center
10
12
Rotation of a galaxy
Rotation curve of NGC 3198
Kepler Rotation of a
Galaxy
velocity
1.5
1
0.5
0
0
5
10
distance from galactic center
15
Gravity lensing
Composite image of the Bullet cluster shows distribution of
ordinary matter, inferred from X-ray emissions, in red and
total mass, inferred from gravitational lensing, in blue.
properties of dark matter
undetectable by radiation
detectable only by gravitation
rotation of galaxies
orbital velocities of galaxies in cluster of galaxies
gravitational lensing
temperature distribution of hot gas in galaxies and
clusters of galaxies
what is dark matter made of
majority: non baryonic
non baryonic matter
neutrinos
axions
supersymmetric particles
does not contribute to the formation of elements
in the cosmos
non baryonic matter
hdm hot dark matter: massive neutrinos
cdm cold dark matter: will lead to a bottom
up formation of structure in the universe;
neutralino
wdm warm dark matter
Neutralinos
big bang: neutralino halos
mass of Earth, size equal to the solar system
can be detected:
disturb Oort cloud cometary showers
produce gamma ray bursts when colliding
more probable near galactic center
baryonic matter
composed of baryons
protons
neutrons
candidates for baryonic dark matter
MACHOs: massive astropnomical compact halo
objects
brown dwarfs (M<0.08 MSun
amount can be calculated from
big bang nucelosynthesis
cosmic microwave background
MACHOS
Detect: gravity bends light
MACHO may be detected if it pass in front of
a star or nearby a star; brightening of the
star
candidates for MACHOS
black holes
neutron stars
black dwarfs
WIMPS weakly interacting
massive particles
interact through weak force and gravity
do not interact through electromagnetism
large mass, slow moving, cold particles
could interact with the Sun, produce high
energy neutrinos
CDMS cryogenic dark matter
search
RAMBOs Robust associations of
massive baryonic objects
dark cluster made of
white dwarfs
brown dwarfs
radii: 1 pc … 15 pc
supersymmetry, susy
In particle physics, supersymmetry (often
abbreviated SUSY) is a symmetry that relates
elementary particles of one spin to other
particles that differ by half a unit of spin and
are known as superpartners.
In a theory with unbroken supersymmetry,
for every type of boson there exists a
corresponding type of fermion with the same
mass and internal quantum numbers, and
vice-versa.
Λ CDM Model of Cosmology I
Λ cosmological constant associated with
a vacuum energy or dark energy
explains the current accelerating expansion of
space against the attractive (collapsing) effects of
gravity. ΩΛ, which is interpreted as the fraction of
the total mass-energy density of a flat universe
that is attributed to dark energy.
Currently, about 74% of the energy density of the
present universe is estimated to be dark energy.
Λ CDM Model of Cosmology II
CDM cold dark matter
dark matter is described as
cold (non relativistic)
collisionless (only gravity forces)
22% of the mass-energy density of the universe
quantum chromodynamics describes strong interaction