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On the equation of state for the [Lambda] field
The recently detected accelerated expansion of the Universe is related to the existence of a new type of matter called the field or quintessence. Constraints were obtained on its equation of state from the absence of clustering of this matter on scales much smaller than the cosmological horizon. The...
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Published in: | Astronomy letters 2002-07, Vol.28 (7), p.434-437 |
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container_title | Astronomy letters |
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creator | Podolsky, D I |
description | The recently detected accelerated expansion of the Universe is related to the existence of a new type of matter called the field or quintessence. Constraints were obtained on its equation of state from the absence of clustering of this matter on scales much smaller than the cosmological horizon. The question of how these constraints affect the possibility of fitting the accelerated expansion by such cosmological models as the Chaplygin gas model is discussed. |
doi_str_mv | 10.1134/1.1491965 |
format | article |
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Constraints were obtained on its equation of state from the absence of clustering of this matter on scales much smaller than the cosmological horizon. 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subjects | Astronomy Chaplygin gas Clustering Equations of state Fittings Horizon Star & galaxy formation Universe |
title | On the equation of state for the [Lambda] field |
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