The mutual interaction terms of the SM Higgs, left-handed leptons, the extra
scalar, and fermions are given by
On the other hand,
scalars of mass ~1 TeV decaying into diphotons, which is a typical signature of many models, are still allowed by the LHC data.
"We do not know what dark matter is, but if it has anything to do with any
scalar particles, it may be older than the Big Bang.
Yale, "Exact Hawking radiation of
scalars, fermions, and bosons using the tunneling method without back-reaction," Physics Letters B, vol.
Our findings suggest rumen-reticulum fill
scalars vary on an intraspecific basis.
where a, b, c, d are
scalars of which b [not equal to] 0, c = 0, d [not equal to] 0 and A, B are two non-zero 1-forms such that A(X) = g(X,U) and B(X) = g(X, V); U, V being mutually orthogonal unit vector fields and D is a symmetric (0, 2) type tensor field with zero trace which satisfies the condition D(X, U) = 0, [for all]X.
The Clebsch parametrization consists of the following very general representation of arbitrary vector fields with three
scalars in the form
Thus, it has been rigorously shown for the first time in this manner (to the author's knowledge) that the
scalars [C.sub.n] appearing in the potential formulation do not contribute to the fields and consequently ensures a unique field representation.
Abstract: We address the problem of loop invariant generation of programs over
scalars and unbounded data structures.
where A is a nowhere vanishing 1-form and [a.sub.1], [a.sub.2] are
scalars of which [a.sub.2] [not equal to] 0.
As the editors note, the three topics are conceptually connected: implicatures (
scalars at least) are sensitive to negative polarity items and presupposition, unlike entailment, is typically invariant under negation.
