Dissipation during inflation
APA
Peloso, M. (2016). Dissipation during inflation. Perimeter Institute. https://pirsa.org/16030074
MLA
Peloso, Marco. Dissipation during inflation. Perimeter Institute, Mar. 15, 2016, https://pirsa.org/16030074
BibTex
@misc{ pirsa_PIRSA:16030074, doi = {10.48660/16030074}, url = {https://pirsa.org/16030074}, author = {Peloso, Marco}, keywords = {Cosmology}, language = {en}, title = {Dissipation during inflation}, publisher = {Perimeter Institute}, year = {2016}, month = {mar}, note = {PIRSA:16030074 see, \url{https://pirsa.org}} }
I will discuss phenomena associated with particle production and field excitation during inflation. In the first part of the talk I will present several
signatures that can originate from the coupling of an axion inflaton to gauge fields. In the second part I will test the robustness of the standard
implications associated with the detection of a gravity wave (GW) signal at CMB scales, by discussing what conditions can allow a visible
sourced GW background that exceeds the vacuum one (without simultaneously overproduce scalar perturbations), and by providing a concrete
example. In the final part I will review the phenomenology of trapped inflation, which is an interesting and minimal mechanism where particle production
provides the main friction for the motion of the inflaton.