000153707 001__ 153707
000153707 005__ 20211110122336.0
000153707 0247_ $$2arXiv$$aarXiv:1304.7813
000153707 0247_ $$2altmetric$$aaltmetric:1423478
000153707 0247_ $$2inspire$$ainspire:1231492
000153707 037__ $$aDESY-2013-00673
000153707 041__ $$aEnglish
000153707 0881_ $$aDESY-13-074; arXiv:1304.7813
000153707 088__ $$2DESY$$aDESY-13-074
000153707 088__ $$2arXiv$$aarXiv:1304.7813
000153707 1001_ $$0P:(DE-H253)PIP1003770$$aJegerlehner, Fred$$b0$$eCorresponding author
000153707 245__ $$aThe Standard model as a low-energy effective theory: what is triggering the Higgs mechanism?
000153707 260__ $$c2013
000153707 300__ $$a29 p.
000153707 3367_ $$2DRIVER$$areport
000153707 3367_ $$2BibTeX$$aTECHREPORT
000153707 3367_ $$010$$2EndNote$$aReport
000153707 3367_ $$0PUB:(DE-HGF)15$$2PUB:(DE-HGF)$$aInternal Report$$bintrep$$mintrep$$s153707
000153707 4900_ $$aRed Report
000153707 500__ $$a27 pages, 9 figures.
000153707 520__ $$aThe discovery of the Higgs by ATLAS and CMS at the LHC not only provided the last missing building block of the electroweak Standard Model, the mass of the Higgs has been found to have a very peculiar value about 125 GeV, which is such that vacuum stability is extending up to the Planck scale. This may have much deeper drawback than anticipated so far. The impact on the running of the SM gauge, Yukawa and Higgs couplings up to the Planck scale has been discussed in several articles recently. Here we consider the impact on the running masses and we discuss the role of quadratic divergences within the Standard Model. The change of sign of the coefficient of the quadratically divergent terms showing up at about mu_0 ~ 7 x 10^16 GeV may be understood as a first order phase transition restoring the symmetric phase, while its large negative values at lower scales triggers the Higgs mechanism, running parameters evolve in such a way that the symmetry is restored two orders of magnitude before the Planck scale. Thus, the electroweak phase transition takes place at the scale mu_0 and not at the electroweak scale v ~ 250 GeV. The SM Higgs system and its phase transition could play a key role for the inflation of the early universe. Also baryogenesis has to be reconsidered under the aspect that perturbative arguments surprisingly work up to the Planck scale.
000153707 536__ $$0G:(DE-HGF)POF2-514$$a514 - Theoretical Particle Physics (POF2-514)$$cPOF2-514$$fPOF II$$x0
000153707 588__ $$aDataset connected to
000153707 693__ $$0EXP:(DE-MLZ)NOSPEC-20140101$$5EXP:(DE-MLZ)NOSPEC-20140101$$eNo specific instrument$$x0
000153707 8564_ $$uhttps://de.arxiv.org/pdf/1304.7813v2
000153707 8564_ $$uhttps://bib-pubdb1.desy.de/record/153707/files/DESY-2013-00673.pdf$$yOpenAccess
000153707 8564_ $$uhttps://bib-pubdb1.desy.de/record/153707/files/DESY-2013-00673.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000153707 8564_ $$uhttps://bib-pubdb1.desy.de/record/153707/files/DESY-2013-00673.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000153707 8564_ $$uhttps://bib-pubdb1.desy.de/record/153707/files/DESY-2013-00673.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000153707 909CO $$ooai:bib-pubdb1.desy.de:153707$$pdriver$$pVDB$$popen_access$$popenaire
000153707 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1003770$$aExternes Institut$$b0$$kExtern
000153707 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1003770$$aExternes Institut$$b0$$kExtern
000153707 9131_ $$0G:(DE-HGF)POF2-514$$1G:(DE-HGF)POF2-510$$2G:(DE-HGF)POF2-500$$3G:(DE-HGF)POF2$$4G:(DE-HGF)POF$$aDE-HGF$$bStruktur der Materie$$lElementarteilchenphysik$$vTheoretical Particle Physics$$x0
000153707 9141_ $$y2013
000153707 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000153707 9201_ $$0I:(DE-H253)ZNP_-2012_-20130307$$kZNP(-2012)$$lStandort Zeuthen$$x0
000153707 9201_ $$0I:(DE-H253)ZEU-THEO-20120731$$kZEU-THEO$$lTheorie$$x1
000153707 980__ $$aintrep
000153707 980__ $$aVDB
000153707 980__ $$aUNRESTRICTED
000153707 980__ $$aFullTexts
000153707 980__ $$aI:(DE-H253)ZNP_-2012_-20130307
000153707 980__ $$aI:(DE-H253)ZEU-THEO-20120731
000153707 9801_ $$aFullTexts