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Survey of the Universe
Survey of the Universe
Greg Snow
U Nebraska Lincoln
CROP
Survey of the Universe
• Powers of Ten – a View of the Universe over distance scales from the very large to the very small
• We live in an expanding Universe
• What’s within 50 Megaparsecs = 150 Million Light Years from us?• Reminder why this distance is relevant to
Ultra High Energy Cosmic Rays
• Candidate sources of Ultra High Energy Cosmic Rays
• Ultimate fate of the Universe
Survey of the Universe
The Universe began about 14 billion years ago with the BIG BANGand has been expanding ever since.
How do we know the Universe is expanding?
Observations of near and far objects in the Universe by Edwin Hubble in the first half of the 20th century led to the conclusion that:
The farther an object is from us, the faster it is moving away from us.
Survey of the Universe
This observation is summarized by the “Hubble Law”.
Velocity of recession, v = H distance, where H is the Hubbleconstant.
Distance in light years
Velocity in kilometers/second
The slope of this lineis the Hubble constant.
(See data in figure from text.)
Survey of the Universe
Do these observations mean that we (i.e. the earth and ourgalaxy) are at the center of the Universe?
• Balloon example
• 5 Volunteers example
The answer is NO – the Universe looks the same from anyvantage point – this is part of the “Cosmological Principle” .
Survey of the Universe
What’s within 50 Megaparsecs = 150 Million Light Years from us?
Why is this relevant to the study of Ultra High Energy CosmicRays?
There are two current theories about the origin of the highestenergy cosmic rays1. “Bottom Up” ScenarioParticles are accelerated by some extreme astrophysical phenomenon – galaxies colliding, inferno in the center of anactive galaxy (an Active Galactic Nucleus, or “AGN”).
2. “Top Down” scenarioParticles are the decay products of heavy unstable objectscreated at the time of the Big Bang
Survey of the Universe
The “Top Down” scenarioHighest energy cosmic ray particles are the decay products of heavy unstable particles created at the time of the Big Bang
Such particles would have to be extremely heavy
Simple-minded example:
Unstable objectwith mass 2 1020 eV
Decays to two protonswith energy 1 1020 eV
Decays to two protonswith energy 1 1020 eV
Survey of the Universe
The “Top Down” scenario2 1020 eV is an enormous mass for a single particle.
Unstable objectwith mass 2 1020 eV
2 1020 eV is equal to 2 1011 GeV, which is the massof 2 1011 protons. (Proton mass is about 1 GeV in energyunits.) Reminder – the heaviest particle discovered to dateis the top quark with mass 170 GeV or 170 protons.
Candidate particles that theoretical astrophysicists talk about:• WIMPZILLA’s – WIMPs are “Weakly Interacting Massive Particles”, a dark matter candidate particle• “Topological defects” – space-time deformities
Survey of the Universe
The “Top Down” scenario
In the Top Down scenario, we would expect ultra high energy cosmic rays to come uniformly from all directions of the sky.
That is, there would be no particular “point sources” .
Survey of the Universe
The “Bottom Up” ScenarioParticles are accelerated by some extreme astrophysical phenomenon – galaxies colliding, inferno in the center of anactive galaxy (an Active Galactic Nucleus, or “AGN”).
Reminder of the GZK cutoff:• If particles accelerated to energies greater than 1019 eV originate at distances greater than about 150 Million Light Years, they will lose energy by interacting with the sea of low energy photons that fill the Universe The Cosmic Microwave Background Radiation• Hence they will reach the earth with a reduced energy• So particles with energy greater than 1019 eV must originate within 150 Million Light Years from earthIn the Bottom Up scenario, we expect primary cosmic raydirections to point back to particular sources in the sky.
Survey of the Universe
How the Universe is Organized
• First, how big is the present Universe?• Since the Big Bang happened 14 billion years ago, the largest the Universe can be is a sphere of radius 14 billion Light Years, the “light horizon”.• The farthest galaxies observed from earth are 10-12 billion Light Years away.
14 Billion LY radius
UniverseSphere of radius150 Million LY,the region whereour highest energycosmic rays originateaccording to the GZK cutoff.
Survey of the Universe
How the Universe is Organized
• The Universe is clumpy – stars are clumped into Galaxies, Galaxies into Clusters, Clusters into Superclusters, some Superclusters into Walls.
• The clumpiness is due to the gravitational attraction among objects small and large, superposed on the overall expansion of the Universe.
• Otherwise, there are tremendous voids between these groupings of matter
Survey of the Universe
Some distance scales
• Diameter of our solar system – 0.0012 LY
• Nearest star, Proxima Centauri – 4 LY
• Diameter of our galaxy – 100,000 LY
• Distance to nearest galaxy – the Sagittarius dwarf galaxy, which is being “eaten” by the Milky Way – 80,000 LY
• Size of our “Local Group” – a collection of at least 30 galaxies, including Andromeda – 3 Million LY
• Size of our “Local Supercluster” which contains our Local Group, the Virgo Cluster, and others – 100 Million LY (see text figure)
(See web animation)
Survey of the UniverseTwo possible sources of the highest energy cosmic rays
Colliding galaxies
Active galactic nucleus
But the true origin andacceleration mechanismfor the highest energy
cosmic rays is UNKNOWN
-- that’s why we want to study them
Supernovae are not violent enough – “Fermi shock acceleration” can explain cosmic
rays up to energies of only about 1015 eV
Survey of the Universe
#S
#S
The Pierre Auger Observatory – the World’s Largest Array
Southern Hemisphere:Malargüe
Province of MendozaArgentina
(being constructed now)
Northern Hemisphere:Millard County, USA
(to be built)
1600 detectors, 3000 km2 each site
The Southern Hemispheresite is being built first sinceit has a better view of the center of the MilkyWay galaxy where there might be a black hole emitting high energy cosmic rays.
Survey of the Universe
The ultimate fate of the Universe
Since the discovery of the Hubble Law, it has been a questionwhether we live in:A closed Universe – gravitational attraction will ultimatelyslow the Universe’s expansion and lead to the eventualcoalescing of all matter – the “Big Crunch” An open Universe – expansion will continue forever in alldirections
It has now been determined that the Universe rate of expansionis in fact accelerating – recession speeds are increasing – so we live in an open Universe.
The “engine” that powers the acceleration is unknown and isreferred to as the Dark Energy of the Universe.
(See web animation)