Epstein Secrets

ona State University. Tempe. AZ 85827-1404 2Research School of Astronomy and Astrophysics, Mt. Stromlo Observatory. Australian National University, Canberra, Australia 2611 (Dated: March 19, 2014) We consider the status of Higgs Inflation in light of the recently announced detection of B-modes in the po

erved values, MH 125 GeV and Mt :4 173 GeV, the coupling runs neg- ative at h 107° — 1012 GeV; this is the well-known vacuum stability problem of the Standard Model [26]. Successful HI requires an O(2e) deviation from central values toward either larger Higgs boson mass or smaller top quark mass. Gauge depende

ona State University. Tempe. AZ 85827-1404 2Reseatrh School of Astronomy and Astrophysics, Mt. Stromlo Observatory, Australian National University. Canberra, Australia 2611 (Dated: March 19, 2014) We consider the status of Higgs Inflation in light of the recently announced detection of B-modes in the po

bserved values, 125 GeV and Mt xr. 173 GeV, the coupling runs neg- ative at h ot 101° —1012 GeV; this is the well-known vacuum stability problem of the Standard Model [26). Successful HI requires an O(2o) deviation from central values toward either larger Higgs boson mass or smaller top quark mass. Gauge depende

gan to fly in the community. Many of these came from the experimenters themselves. I have a part-time position at Australian National University in Canberra, and the International Con- ference on High Energy Physics was going to be in held in Melbourne in July of 2012. Melbourne has a big LHC contingent,

ne wanted to talk about the details in public. 2P_GrealetaleryEverTold_AC.indd 254 12/16116 3:06 PIA EFTA00286176 Spanking the Vacuum 255 That the Standard Model didn't fix in advance many of the details of the Higgs sector didn't dissuade many theorists from proposing models that "predicted" the Higgs mass