cosmological model

collocation in English

meaningsofcosmologicalandmodel

These words are often used together. Click on the links below to explore the meanings. Or,see other collocations withmodel.
cosmological
adjective
uk
/ˌkɒz.məˈlɒdʒ.ɪ.kəl/us
/ˌkɑːz.məˈlɑː.dʒɪ.kəl/
involving or relating to cosmology (= the study of the nature and origin of the ...
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model
noun[C]
uk
/ˈmɒd.əl/us
/ˈmɑː.dəl/
something that a copy can be based on because it is an extremely good example of ...
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(Definition ofcosmologicalandmodelfrom theCambridge English Dictionary© Cambridge University Press)

Examplesofcosmological model

These examples are from corpora and from sources on the web. Any opinions in the examples do not represent the opinion of the Cambridge Dictionary editors or of Cambridge University Press or its licensors.
In order to arrive at acosmologicalmodel, however, theoreticians needed to make assumptions about the nature of the largest scales of the universe.
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By contrast hot dark matter would smear out the large-scale structure of galaxies and thus is not considered a viablecosmologicalmodel.
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And inflation, in some form or other, is widely considered to be our best availablecosmologicalmodel.
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The nature and history of the universe is coded in this radiation field and any realisticcosmologicalmodelmust be able to describe it.
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The time delay differences from different images can be determined by the mass model and thecosmologicalmodel.
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In studying the relationship between the landscape and religious representations we have to assume that the participants had cosmological models, and that these models determined their use of the landscape.
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However, it is argued that dark energy, described in the recent forms of 'quintessence ' cosmological models may show the current conclusions from observations to be too presumptive.
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Many other exact solutions which can be interpreted as cosmological models of rotating universes are known.
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In the modern cosmological models, most energy in the universe is in forms that have never been detected directly, namely dark energy and dark matter.
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Comparing how galaxy clusters are distributed in mass and redshift to predictions made by cosmological models, we can test these cosmological models.
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The last two are often used as cosmological models for (respectively) matter-dominated and radiation-dominated epochs.
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According to standard cosmological models, the motion of galaxy clusters with respect to the cosmic microwave background should be randomly distributed in all directions.
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Distance of these objects are derived from their measured redshifts, which depends on the cosmological models used.
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It provides an observable constraint for cosmological models, which may diverge at temperatures beyond their predicted critical cluster temperature.
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Examples of cosmological models without an event horizon are universes dominated by matter or by radiation.
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It is one out of a half-dozen cosmological tests that was conceived in the 1930s to check the viability of and compare new cosmological models.
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Early work on cataloguing radio sources had as an aim the determination of the source counts distribution to help astronomers decide between cosmological models.
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As such, measurements of its abundance contribute to cosmological models.
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As of 2004, measurements of this subtle shear showed considerable promise as a test of cosmological models.
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The problem is sometimes discussed in cosmology as an analogue of questions about the number of observers in various cosmological models.
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These examples are from corpora and from sources on the web. Any opinions in the examples do not represent the opinion of the Cambridge Dictionary editors or of Cambridge University Press or its licensors.
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