Power Counting vs Higgs Inflation
APA
Trott, M. (2009). Power Counting vs Higgs Inflation. Perimeter Institute. https://pirsa.org/09050058
MLA
Trott, Michael. Power Counting vs Higgs Inflation. Perimeter Institute, May. 21, 2009, https://pirsa.org/09050058
BibTex
@misc{ pirsa_PIRSA:09050058, doi = {10.48660/09050058}, url = {https://pirsa.org/09050058}, author = {Trott, Michael}, keywords = {Cosmology}, language = {en}, title = {Power Counting vs Higgs Inflation}, publisher = {Perimeter Institute}, year = {2009}, month = {may}, note = {PIRSA:09050058 see, \url{https://pirsa.org}} }
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Abstract
We use the power-counting formalism of effective field theory to study the size of loop corrections in theories of slow-roll inflation, with the aim of more precisely identifying the limits of validity of the usual classical inflationary treatments. Although most slow-roll models lie within the semiclassical domain, we find the consistency of the Higgs-Inflaton scenario to be more delicate due to the proximity between the Hubble scale during inflation and the upper bound allowed by unitarity on the new-physics scale.