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dc.contributor.authorChen, Pisinen_US
dc.contributor.authorLai, Kwang-Changen_US
dc.date.accessioned2019-04-03T06:40:40Z-
dc.date.available2019-04-03T06:40:40Z-
dc.date.issued2007-12-07en_US
dc.identifier.issn0031-9007en_US
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevLett.99.231302en_US
dc.identifier.urihttp://hdl.handle.net/11536/10013-
dc.description.abstractWe point out that during the reionization epoch of the cosmic history, the plasma collective effect among the ordinary matter would suppress the large scale structure formation. The imperfect Debye shielding at finite temperature would induce an electrostatic pressure which, working together with the thermal pressure, would counter the gravitational collapse. As a result, the effective Jeans length, (lambda) over tilde (J) is increased by a factor (lambda) over tilde (J)/(lambda) over tilde (J) = root 8/5, relative to the conventional one. For scales smaller than the effective Jeans scale the plasma would oscillate at the ion-acoustic frequency. The modes that would be influenced by this effect lie roughly in the range 0.5h Mpc(-1)< k, which corresponds to the Lyman-alpha forest from the intergalactic medium. We predict that in the linear regime of density-contrast growth, the plasma suppression of the matter power spectrum would approach 1 - (Omega(dm)/Omega(m))(2) similar to 1 - (5/6)(2) similar to 30%.en_US
dc.language.isoen_USen_US
dc.titlePlasma suppression of large scale structure formation in the universeen_US
dc.typeArticleen_US
dc.identifier.doi10.1103/PhysRevLett.99.231302en_US
dc.identifier.journalPHYSICAL REVIEW LETTERSen_US
dc.citation.volume99en_US
dc.citation.issue23en_US
dc.citation.spage0en_US
dc.citation.epage0en_US
dc.contributor.department物理研究所zh_TW
dc.contributor.departmentInstitute of Physicsen_US
dc.identifier.wosnumberWOS:000251451000011en_US
dc.citation.woscount7en_US
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