UV insensitivity of Higgs Inflation Jacopo Fumagalli Nikhef
- Slides: 19
UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli Nikhef, Amsterdam with Marieke Postma (in preparation). TEXAS Symposium 2015, Geneva, 14/12/2015 UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Motivation • Inflation A. Guth, A. Linde, P. Steinhard’ 80 • Who is the Inflaton? • Request for simplicity, SM Only one scalar field in the LHC , PLANCK • Consistent simplicity UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Overview • Higgs Inflation – Tree level – Quantum aspects (Unitarity, renormalizability. . ) • UV sensitivity – UV completion – RG flow and renormalization scale – Results for the CMB parameters UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Higgs Inflation Bezrukov-Shaposhnikov ‘ 08 • Einstein frame UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Density perturbations. Bezrukov’ 14 UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Overview • Higgs Inflation – Tree level – Quantum aspects (Unitarity, renormalizability. . ) • UV sensitivity – UV completion – RG flow and renormalization scale – Results for the CMB parameters UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Unitarity bound Burgess ‘ 09, Barbon ’ 09, Hertzberg ’ 10 • Cutoff field dependent • Considering Gauge interaction (Goldstone) Bezrukov et al. ’ 11, Burgess ’ 14, Prokopec & Weenink ’ 14 UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Renormalizability in EFT sense. D. George, S. Mooij, M. Postma ‘ 14 ‘ 15 • Small regime • Mid regime • Large regime Demand: at every order a finite number of counter terms UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Overview • Higgs Inflation – Tree level – Quantum aspects (Unitarity, renormalizability. . ) • UV sensitivity – UV completion – RG flow and renormalization scale – Results for the CMB parameters UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
UV completion Bezrukov, Rubio and Shap. ’ 14, Burgess, Patil, Trott ’ 14 • Which shape for the suppression scale? • Which form for the higher d operators? – Preserving the quasi-shift symmetry – Effect only where really needed! UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Overview • Higgs Inflation – Tree level – Quantum aspects (Unitarity, renormalizability. . ) • UV sensitivity – UV completion – RG flow and renormalization scale – Results for the CMB parameters UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
RG flow • Corrected Potential Bezrukov, Grubinov, Shaposhnikov Barvinsky, Kamenshchik, Kiefer, Starobinsky, Simone, Hertzberg, Wilzcek George, Mooij, Postma Burgess, Patil, Trott • RG improvement UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Overview • Higgs Inflation – Tree level – Quantum aspects (Unitarity, renormalizability. . ) • UV sensitivity – UV completion – RG flow and renormalization scale – Results for the CMB parameters UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Effect on the CMB observables Inflationary regime Same as tree level results ! UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Running insensitivity • • Numerical results, example For Standard Model same as A. Kyle’ 14 • Second order , h. o. corrections suppressed UV (in)sensitivity of Higgs Inflation and Jacopo Fumagalli
Conclusions • Higgs inflation at tree level gives great prediction for • The theory is not renormalizable , we need at least a particular UV completion • Threshold corrections to the slow roll parameter cancel in the expression for and independetly of the form of this UV completion UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
RG flow Coleman-Weinberg ’ 73 Quantum corrections two routes: Jordan Einstein • Diffrent results in the GB sector • Back reaction negligible only in the Einstein frame • Approx. FLRW S. Mooij, M. Postma ’ 11 D. George, S. Mooij, M. Postma ‘ 14 UV (in)sensitivity of Higgs Inflation D. George, S. Mooij, Jacopo Fumagalli
Masses. UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
Higgs instability. UV (in)sensitivity of Higgs Inflation Jacopo Fumagalli
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