Conservation laws, consisting of the existence of quantities
which do not change in time, independent
of the dynamical evolution of a system, are crucial and
vital for the construction of any dynamical
system theory. The basic properties such as
conservation of energy, momentum, angular momentum,
charge, isospin, or generalization thereof are
fundamental and must be guaranteed by a physical
system, if it is to give a valid description of nature.
One persistent objection against the concept
of superluminal entities is based on the anticipation
of fast energy loss which could be incurred
under Vavilov-Cherenkov radiation, with the consequent
prediction that no such particles could be
detected. Yet presently, no theoretical or experimental
explication exists which justifies this claim.
Here we show, in the limit of a kinematically
permissible and non-dispersive medium, that energy
conservation is feasible. Corresponding to radiation
intensities from large energy-momentum transfer,
when the parameter k of the
generalized linear velocity of the superluminal free spin-half field is made
sufficiently large, Cherenkov cone becomes flattened at
90o with direction of motion, bringing the
radiated energy to merge with the circulating energy
flow in the wave field of the particle.
Author(s) Details
Emmanuel D. K. Gazoya
National Nuclear Research
Institute (NNRI) / ARC, Ghana Atomic Energy Commission, Accra, Box LG 80,
Ghana.
View Book :- https://bp.bookpi.org/index.php/bpi/catalog/book/245
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