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Find link is a tool written by Edward Betts.searching for Vacuum expectation value 23 found (98 total)
alternate case: vacuum expectation value
Goldberger–Wise mechanism
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on the Planck brane and TeV brane are different and causes the vacuum expectation value of the scalar field to change throughout the fifth dimension. ThisNext-to-Minimal Supersymmetric Standard Model (1,247 words) [view diff] no match in snippet view article find links to article
component of the singlet S^{\displaystyle {\hat {S}}} getting a vacuum-expectation value of ⟨S^⟩{\displaystyle \langle {\hat {S}}\rangle }; that is, weBumblebee models (3,093 words) [view diff] exact match in snippet view article find links to article
are effective field theories describing a vector field with a vacuum expectation value that spontaneously breaks Lorentz symmetry. A bumblebee model isDesert (particle physics) (1,274 words) [view diff] exact match in snippet view article
electroweak energy scale–conventionally defined as roughly the vacuum expectation value or VeV of the Higgs field (about 246 GeV)–and the GUT scale, inDoublet–triplet splitting problem (1,143 words) [view diff] exact match in snippet view article find links to article
SU(5) and is traceless. When Σ{\displaystyle \Sigma } acquires a vacuum expectation value ⟨Σ⟩=diag(2,2,2,−3,−3)f{\displaystyle \langle \Sigma \rangle ={\rmPhysics beyond the Standard Model (5,521 words) [view diff] exact match in snippet view article find links to article
Higgs vacuum expectation value. The sum of squares of boson masses (that is, W, Z, and Higgs bosons) is also very close to half of squared Higgs vacuum expectationTau function (integrable systems) (6,256 words) [view diff] exact match in snippet view article
of creation and annihilation operators) is defined so that its vacuum expectation value (VEV) vanishes ⟨0|:L1,⋯Lm:|0⟩=0.{\displaystyle \langle 0|:L_{1}Inflaton (926 words) [view diff] exact match in snippet view article find links to article
vacuum state with very large vacuum energy, caused by a non-zero vacuum expectation value of the inflaton field. Any region of space in this state will rapidlySoft SUSY breaking (514 words) [view diff] exact match in snippet view article find links to article
{\frac {|F|^{2}}{M^{3}}}}, where |F|{\displaystyle |F|} is the vacuum expectation value of the auxiliary field components of X{\displaystyle X} and M{\displaystyleGribov ambiguity (2,432 words) [view diff] exact match in snippet view article find links to article
order to do so, he considered the ghost propagator, which is the vacuum expectation value of the inverse of the Faddeev–Popov operator. If this operatorRiccardo Barbieri (844 words) [view diff] exact match in snippet view article find links to article
of a Dark Matter model based on a second Higgs doublet without vacuum expectation value. Having taught in Pisa for 30 years, Riccardo Barbieri is acclaimedR-parity (1,519 words) [view diff] exact match in snippet view article find links to article
partner of neutrino), which is odd under R-parity, develops a vacuum expectation value. It can be shown, on phenomenological grounds, that this cannotHierarchy problem (3,393 words) [view diff] exact match in snippet view article find links to article
recover the breaking of electroweak symmetry through a non-null vacuum expectation value. This can be obtained using the Weinberg–Coleman mechanism withPenrose–Hawking singularity theorems (3,121 words) [view diff] exact match in snippet view article find links to article
than the pressure. All ordinary matter, with the exception of a vacuum expectation value of a scalar field, obeys this condition. During inflation, theSuperselection (2,402 words) [view diff] exact match in snippet view article find links to article
the Higgs t parameter is varied so that it does not acquire a vacuum expectation value, the universe is now symmetric under an unbroken SU(2) and U(1)Fermi's interaction (3,718 words) [view diff] exact match in snippet view article find links to article
the Standard Model, the Fermi constant is related to the Higgs vacuum expectation value v=(2GF0)−1/2≃246.22GeV{\displaystyle v=\left({\sqrt {2}}\,G_{\rmLarge extra dimensions (3,362 words) [view diff] exact match in snippet view article find links to article
generate it, the Higgs must enter. But in the ADD model, the Higgs vacuum expectation value is comparable to the Planck scale, so the Higgs field can contributeSterile neutrino (4,402 words) [view diff] exact match in snippet view article find links to article
doublet Higgs field ϕ{\displaystyle \phi } acquires its non-zero vacuum expectation value, ν{\displaystyle \nu }, spontaneously breaking its SU(2)L × U(1)Chronology of the universe (13,846 words) [view diff] exact match in snippet view article find links to article
H0, H0⁎ scalar bosons (Higgs interaction). In this picture, the vacuum expectation value of the Higgs field is zero (therefore, all fermions are massless)Swampland (physics) (2,499 words) [view diff] exact match in snippet view article
infinite distance limit of the parameter space. If one takes the vacuum expectation value of the scalar fields to infinity, there exists a tower of lightComposite Higgs models (3,021 words) [view diff] exact match in snippet view article find links to article
{~v^{2}\ }{~f^{2}\ }}\ ,} where v = 246 GeV is the electro-weak vacuum expectation value. By construction these models approximate the SM to arbitrary precisionFamily symmetries (4,956 words) [view diff] exact match in snippet view article find links to article
complex scalar field called flavon ϕ{\displaystyle \phi } whose vacuum expectation value (VEV) ⟨ϕ⟩{\displaystyle \langle \phi \rangle } presumably breaksLight-front computational methods (10,679 words) [view diff] exact match in snippet view article find links to article
symmetry breaking in the vacuum of the theory. The usual Higgs vacuum expectation value in the instant form is replaced by k+=0{\displaystyle k^{+}=0}