Examples of using Electroweak in English and their translations into Slovak
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This is called the electroweak theory.
Electroweak theory, Fermi theory of beta decay, Weak hypercharge, Weak isospin.
Electromagnetic and weak interactions into the electroweak.
Electroweak theory is very important for modern cosmology, particularly on how the universe evolved.
For elucidating the quantum structure of electroweak interactions in physics".
The electroweak theory of particle physics is a unification of the electromagnetic and weak interactions.
Hooft, Gerardus't Netherlands study of the quantum structure of electroweak interactions.
In inflationary cosmology, the electroweak epoch ends when the inflationary epoch begins, at roughly 10- 32 second.
At high energies electromagnetic andweak forces are described as a unified electroweak force.
Any introduction of particle masses would break the electroweak symmetry and render the theory unpredictable.
At high energy the weak force andelectromagnetic force are unified as a single electroweak force.
The inflationary epoch comprises the first part of the electroweak epoch following the grand unification epoch.
The soft supersymmetry breaking terms shouldalso be of the same order of magnitude as the electroweak scale.
In inflationary cosmology, the electroweak epoch began when the inflationary epoch ended, at roughly 10- 32 second.
Gerard't Hooft Netherlands"for elucidating the quantum structure of electroweak interactions in physics".
In the theory of the electroweak interaction, the carriers of the weak force are the massive gauge bosons called the W and Z bosons.
Gerardus't Hooft Netherlands"for elucidating the quantum structure of electroweak interactions in physics"[94].
In other models, the electroweak epoch is said to begin after the inflationary epoch ended, at roughly 10- 32 seconds.
If supersymmetry is a property of our universe, then it must bebroken at an energy as low as 1 TeV, the electroweak symmetry scale.
Beyond the Standard Model, some theorists work to unite the electroweak and strong interactions within a Grand Unified Theory[12](GUT).
If supersymmetry is a property of our universe, then it must be broken at anenergy that is no lower than 1 TeV, the electroweak scale.
The analogy between the Skyrme field and the Higgs field of the electroweak sector has been used to postulate that all fermions are skyrmions.
If supersymmetry is a property of our universe, then it must bebroken at an energy as low as 1 TeV, the electroweak symmetry scale.
Precision measurements of electroweak parameters, such as the Fermi constant and masses of W/Z bosons, can be used to calculate constraints on the mass of the Higgs.
If supersymmetry is a property of our universe, then it must be broken at anenergy that is no lower than 1 TeV, the electroweak symmetry scale.
It should have the same order of magnitude as the electroweak scale, many orders of magnitude smaller than that of the Planck scale, which is the natural cutoff scale.
The focus of the High-Energy Physics Group lies in phenomenology of the Standard model of electroweak interactions and beyond. Particularly, the models of electroweak symmetry breaking are studied.