dc.contributor.author |
Germani, C |
en |
dc.contributor.author |
Kehagias, A |
en |
dc.date.accessioned |
2014-03-01T01:33:55Z |
|
dc.date.available |
2014-03-01T01:33:55Z |
|
dc.date.issued |
2010 |
en |
dc.identifier.issn |
0031-9007 |
en |
dc.identifier.uri |
https://dspace.lib.ntua.gr/xmlui/handle/123456789/20616 |
|
dc.subject |
Degree of Freedom |
en |
dc.subject |
General Relativity |
en |
dc.subject |
Higgs Boson |
en |
dc.subject |
Quantum Correction |
en |
dc.subject |
Scalar Field |
en |
dc.subject |
Standard Model |
en |
dc.subject.classification |
Physics, Multidisciplinary |
en |
dc.subject.other |
Degrees of freedom |
en |
dc.subject.other |
General Relativity |
en |
dc.subject.other |
New model |
en |
dc.subject.other |
Quantum correction |
en |
dc.subject.other |
Scalar fields |
en |
dc.subject.other |
Standard-model Higgs bosons |
en |
dc.subject.other |
The standard model |
en |
dc.subject.other |
Standards |
en |
dc.subject.other |
Bosons |
en |
dc.title |
New model of inflation with nonminimal derivative coupling of standard model higgs boson to gravity |
en |
heal.type |
journalArticle |
en |
heal.identifier.primary |
10.1103/PhysRevLett.105.011302 |
en |
heal.identifier.secondary |
http://dx.doi.org/10.1103/PhysRevLett.105.011302 |
en |
heal.identifier.secondary |
011302 |
en |
heal.language |
English |
en |
heal.publicationDate |
2010 |
en |
heal.abstract |
In this Letter we show that there is a unique nonminimal derivative coupling of the standard model Higgs boson to gravity such that it propagates no more degrees of freedom than general relativity sourced by a scalar field, reproduces a successful inflating background within the standard model Higgs parameters, and finally does not suffer from dangerous quantum corrections. © 2010 The American Physical Society. |
en |
heal.publisher |
AMER PHYSICAL SOC |
en |
heal.journalName |
Physical Review Letters |
en |
dc.identifier.doi |
10.1103/PhysRevLett.105.011302 |
en |
dc.identifier.isi |
ISI:000279483900002 |
en |
dc.identifier.volume |
105 |
en |
dc.identifier.issue |
1 |
en |