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[[Image:AstroMSseqF_063aL_(18135101).jpg|thumb|300px|right|The Millennium Run simulates the universe until the present state, where structures are abundant, manifesting themselves as stars, galaxies and clusters]]
[[Image:AstroMSseqF_063aL_(18135101).jpg|thumb|300px|right|The Millennium Run simulates the universe until the present state, where structures are abundant, manifesting themselves as stars, galaxies and clusters]]
The '''Millennium Run''' (also known as the '''Millennium Simulation''', because of its size<ref name="arx">[http://www.mpa-garching.mpg.de/galform/millennium/0504097.pdf Simulating the joint evolution of quasars, galaxies and their large-scale distribution], [[ArXiv]] pre-print, 6 April 2005 - page 3.</ref> is the name of a [[Computer simulation|simulation]] created to investigate how the [[Universe]] evolved over time, and is used by [[scientists]] working in [[physical cosmology]] to compare [[Scientific method|observations with theoretical predictions]].
The '''Millennium Run''' (also known as the '''Millennium Simulation''', because of its size<ref name="arx 3">[http://www.mpa-garching.mpg.de/galform/millennium/0504097.pdf Simulating the joint evolution of quasars, galaxies and their large-scale distribution], [[ArXiv]] pre-print, 6 April 2005 - page 3.</ref> is the name of a [[Computer simulation|simulation]] created to investigate how the [[Universe]] evolved over time, and is used by [[scientists]] working in [[physical cosmology]] to compare [[Scientific method|observations with theoretical predictions]].


==Overview==
==Overview==
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==Size of the simulation==
==Size of the simulation==
For the first scientific results, published on [[June 2]], [[2005]], the ''Millennium Run'' traced more than 10 billion "particles" (though these are not particles in the [[particle physics]] sense - each "particle" represents around a billion [[solar mass]]es of dark matter.
For the first scientific results, published on [[June 2]], [[2005]], the ''Millennium Run'' traced more than 10 billion "particles" (though these are not particles in the [[particle physics]] sense - each "particle" represents around a billion [[solar mass]]es of dark matter.<ref name="arx 19">[http://www.mpa-garching.mpg.de/galform/millennium/0504097.pdf Simulating the joint evolution of quasars, galaxies and their large-scale distribution], [[ArXiv]] pre-print, 6 April 2005 - page 19.</ref>


The region of space simulated was a [[cube (geometry)|cube]] with about 2 billion [[light year]]s as its length. This volume was populated by about 20 million "galaxies". A [[super computer]], located in [[Garching]], Germany, executed the simulation code for more than a month. The output of the simulation needed about 25 [[Terabytes]] for storage.
The region of space simulated was a [[cube (geometry)|cube]] with about 2 billion [[light year]]s as its length. This volume was populated by about 20 million "galaxies". A [[super computer]], located in [[Garching]], Germany, executed the simulation code for more than a month. The output of the simulation needed about 25 [[Terabytes]] for storage.

Revision as of 10:37, 2 May 2009

File:AstroMSseqF 063aL (18135101).jpg
The Millennium Run simulates the universe until the present state, where structures are abundant, manifesting themselves as stars, galaxies and clusters

The Millennium Run (also known as the Millennium Simulation, because of its size[1] is the name of a simulation created to investigate how the Universe evolved over time, and is used by scientists working in physical cosmology to compare observations with theoretical predictions.

Overview

A basic scientific tool to test theories in cosmology is to evaluate their consequences for the observable parts of the universe. This includes, among other things, the distribution of matter (galaxies and intergalactic gas) as it is seen, now. Since looking further into the distance also means looking back in time, a meaningful test of the evolution of that distribution over time is possible.

The Millennium Run simulation starts with the state of the universe when the cosmic background radiation was emitted, about 379,000 years after the universe began. The cosmic background radiation is known by satellite experiments and serve as the starting point for the corresponding matter distribution. Using the physical laws of the currently known cosmologies, the evolution of matter as galaxies and black holes is simulated and recorded.

This simulation was created and executed for the first time in 2005 by the Virgo Consortium, an international group of astrophysicists from Germany, the United Kingdom, Canada, Japan and the United States.

Size of the simulation

For the first scientific results, published on June 2, 2005, the Millennium Run traced more than 10 billion "particles" (though these are not particles in the particle physics sense - each "particle" represents around a billion solar masses of dark matter.[2]

The region of space simulated was a cube with about 2 billion light years as its length. This volume was populated by about 20 million "galaxies". A super computer, located in Garching, Germany, executed the simulation code for more than a month. The output of the simulation needed about 25 Terabytes for storage.

First results

The Sloan Digital Sky Survey had challenged the current understanding of cosmology by finding black hole candidates in very bright quasars at large distances. This meant that they were created much earlier than initially expected. The Millennium Run demonstrated that these objects can indeed be explained, and do not contradict our models of the evolution of the Universe.

Other large scale universe simulations

The 2007 Horizon simulation project features the largest N body simulation ever performed: 70 billions particles were evolved.

For the first time, we have performed a simulation of half the observable universe, with enough resolution to describe a Milky Way-like galaxy with more than 100 dark matter particles.

References

See also