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<big>'''The TianLai Project -- A Dark Energy Radio Observation Experiment'''<big> | <big>'''The TianLai Project -- A Dark Energy Radio Observation Experiment'''<big> | ||
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The neutral hydrogen atoms in the Universe radiates with a wavelength of 21 cm, on large scales the intensity of this radiation is proportional to the matter density. By radio observation, one can probe the cosmic large scale structure distribution. Using the baryon acoustic oscillation signatures in the matter power spectrum as standard rulers, high precision cosmological measurements can be obtained, and the dark energy equation of state parameter w measured. This provides an important tool for dark energy observation. | The neutral hydrogen atoms in the Universe radiates with a wavelength of 21 cm, on large scales the intensity of this radiation is proportional to the matter density. By radio observation, one can probe the cosmic large scale structure distribution. Using the baryon acoustic oscillation signatures in the matter power spectrum as standard rulers, high precision cosmological measurements can be obtained, and the dark energy equation of state parameter w measured. This provides an important tool for dark energy observation. | ||
== Getting started == | == Getting started == | ||
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| + | <font color=red>This is a authorized wiki, only available for members of TianLai. Please email to the manager(Mr. Zhang):zhang_juyong01@163.com</font> | ||
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* [//www.mediawiki.org/wiki/Manual:Configuration_settings Configuration settings list] | * [//www.mediawiki.org/wiki/Manual:Configuration_settings Configuration settings list] | ||
* [//www.mediawiki.org/wiki/Manual:FAQ MediaWiki FAQ] | * [//www.mediawiki.org/wiki/Manual:FAQ MediaWiki FAQ] | ||
* [https://lists.wikimedia.org/mailman/listinfo/mediawiki-announce MediaWiki release mailing list] | * [https://lists.wikimedia.org/mailman/listinfo/mediawiki-announce MediaWiki release mailing list] | ||
Revision as of 23:11, 17 July 2012
The TianLai Project -- A Dark Energy Radio Observation Experiment
The neutral hydrogen atoms in the Universe radiates with a wavelength of 21 cm, on large scales the intensity of this radiation is proportional to the matter density. By radio observation, one can probe the cosmic large scale structure distribution. Using the baryon acoustic oscillation signatures in the matter power spectrum as standard rulers, high precision cosmological measurements can be obtained, and the dark energy equation of state parameter w measured. This provides an important tool for dark energy observation.
Getting started
This is a authorized wiki, only available for members of TianLai. Please email to the manager(Mr. Zhang):zhang_juyong01@163.com
