2009
DOI: 10.1103/physrevd.79.083515
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CMB anisotropies from acausal scaling seeds

Abstract: We investigate models where structure formation is initiated by scaling seeds: We consider rapidly expanding relativistic shells of energy and show that they can fit current CMB and large scale structure data if they expand with super-luminal velocities. These acausally expanding shells provide a viable alternative to inflation for cosmological structure formation with the same minimal number of parameters to characterize the initial fluctuations. Causally expanding shells alone cannot fit present data. Hybrid… Show more

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Cited by 10 publications
(9 citation statements)
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“…This can only be circumvented if one allows for acausality, i.e. superluminal motion, of the seeds [19], however improbable. In Ref.…”
Section: Resultsmentioning
confidence: 99%
“…This can only be circumvented if one allows for acausality, i.e. superluminal motion, of the seeds [19], however improbable. In Ref.…”
Section: Resultsmentioning
confidence: 99%
“…It is surprisingly difficult to create this observed fluctuation spectrum in alternative scenarios that are strictly causal and only act on sub-horizon scales (Spergel and Zaldarriaga 1997 ; Scodeller et al. 2009 ).…”
Section: Part I Dark Energymentioning
confidence: 99%
“…While there is no conclusive proof that an inflationary phase took place in the early universe, it is surprisingly difficult to create the observed fluctuation spectrum in alternative scenarios that are strictly causal and only act on sub-horizon scales [ 854 , 803 ].…”
Section: Dark Energymentioning
confidence: 99%