Examples of using Electroweak in English and their translations into Vietnamese
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VELTMAN for elucidating the quantum structure of electroweak interactions in physics.
Indeed, in the electroweak theory, instantons trigger the violation of the conservation laws of baryons.
The grand unification epoch ends when theGUT forces further separate into the strong and electroweak forces.
The theory of strong and electroweak interactions at low and high energies and at high density or temperature.
Then physicists linked another force, the weak force, with that electromagnetic force,forming a theory of electroweak interactions.
It is natural to suspect that the electroweak forces and the strong forces should also be connected by gauge rotations.
In follow-up posts we will refine our Feynman rules to learn more about the nature of mass andthe phenomenon called electroweak symmetry breaking.
If the electroweak burning is efficient, it could consume enough mass to prevent what's left from ever becoming a black hole.
Starkman, together with former graduate and post-doctoral students, describe the electroweak star in a paper submitted to Physical Review Letters.
In the theory of electroweak interaction, the left-handed spin component of the electron forms a weak isospin doublet with the electron neutrino.
Just as electricity, magnetism,and the weak force were unified into the electroweak interaction, they work to unify all of the fundamental forces.
The gauge bosons in the electroweak force came about from this line of thought, as did the Higgs mechanism and, as was confirmed just a few years ago, the Higgs boson.
Starkman and his team theorize that at the extreme temperatures anddensities reached during stellar collapse could give rise to the electroweak phase of a star's life.
Most of the energy eventually emitted from electroweak stars is in the form of neutrinos, which are nearly without mass and hard to detect.
The Nobel prize winning work of Glashow, Salam, and Weinberg successfully showed that the electromagnetic andweak forces can be unified into a single electroweak force.
After electroweak symmetry breaking the Higgsino become a pair of neutral Majorana fermions called neutralinos and a charged Dirac fermion called a chargino.
The weak force has been unifiedtogether with the electromagnetic force as a single fundamental electroweak force, which manifests at high energy(such as those found within particle accelerators).
After electroweak symmetry breaking the Higgsino becomes a pair of neutral Majorana fermions called neutralinos and a charged Dirac fermion called a chargino(plus and minus).
Higgsino searches have been performed by both the ATLAS and CMS experiments at the Large Hadron Collider at CERN,where physicists have searched for the direct electroweak pair production of Higgsinos.
At temperatures below the electroweak scale their only interactions with standard model particles are weak interactions due to their mixing with ordinary neutrinos.
This unification work received the 1979 Nobel Prize in Physics,and further work on proving that the mathematical foundations of the electroweak force were renormalizable received the 1999 Nobel Prize in Physics.
It is a key element of the electroweak theory that forms part of the standard model of particle physics, and of many models, such as Grand Unified Theories.
In particle theory,supersymmetry is recognized as a way to stabilize the hierarchy between the unification scale and the electroweak scale(or the Higgs boson mass), and can also provide a natural dark matter candidate.
Finally, in the 20th century, Steven Weinberg, Abdus Salam and Sheldon Lee Glashow discovered that, at high energies, the electromagnetic and weak force- without which the sun wouldn't shine-merge into a single electroweak force.
Higgs is bestknown for his 1960s proposal of broken symmetry in electroweak theory, explaining the origin of mass of elementary particles in general and of the W and Z bosons in particular.
At ordinary temperatures it is so incredibly rare that it probably hasn't happened within the visible universe anytime in the last 10 billion years,except perhaps in the core of these electroweak stars and in the laboratories of some advanced alien civilizations.
Because of the high mass of the top quark, toponium does not exist,since the top quark decays through the electroweak interaction before a bound state can form(a rare example of a weak process proceeding more quickly than a strong process).
The weak nuclear force and the electromagnetic force were unified, in their quantized forms,into a single quantum field theory known as electroweak theory, by the physicists Abdus Salam, Sheldon Glashow and Steven Weinberg.
Some of the few loopholes allowing one to avoid theLee-Weinberg bound without introducing new forces below the electroweak scale have been ruled out by accelerator experiments(i.e. CERN, Tevatron), and in decays of B mesons.[3].