It is first shown that the Dirac's equation in a relativistic frame could be modified to allow discrete time, in agreement to a recently published upper bound. Next, an exact self-adjoint 4 × 4 relativistic time operator for spin-1 2 particles is found and the time eigenstates for the non-relativistic case are obtained and discussed. Results confirm the quantum mechanical speculation that particles can indeed occupy negative energy levels with vanishingly small but non-zero probablity, contrary to the general expectation from classical physics. Hence, Wolfgang Pauli's objection regarding the existence of a self-adjoint time operator is fully resolved. It is shown that using the time operator, a bosonic field referred here to as energons may be created, whose number state representations in non-relativistic momentum space can be explicitly found.
TIME SPECTRAIn their recent paper, Faizal et al.[1] suggest that an operator for time could be defined and introduced to the non-relativistic Schrödinger's equation, which would recast it in the formwhere α with the dimension of inverse energy is introduced through appropriate deformed algebra. The resulting feature of (1) is that there will result two distinct energy eigenvalues, and thus the the time-coordinate would acquire a minimum time-step feature. While the subject of time has been quite controversial, as nicely summarized by Muller [2][3][4], the existence of a Hermitian timeoperator has been a subject of long debate. Pauli [5,6] was the first to point out that it was impossible to have such an operator of time. He did not present a well-founded proof, however, and his reason was that the time needed to be a continuous variable while energy eigenstates must be bounded from below [7]. This viewpoint has been followed in many of the later studies which have been discussed in several recent reviews of this subject [8-10]. However, it has been rigorously shown [11,12] that a self-adjoint Hermitian Timeof-Arrival operator can be indeed accurately defined and used. Also, in his comment [13] and earlier works [14], Sidharth also points out the possibility of discreteness at the Compton Scale to develop a consistent theoretical framework for cosmology. It is here shown that this is in fact quite possible in the fully relativistic picture of quantum mechanics, without retaining to such a non-standard algebra.The 4 × 4 Dirac's equation subject to a potential readswhere [V ± ] are appropriate perturbing spin-matrix potentials for particles and antiparticles, and |ψ ± are spinors. The vector σ is defined as σ = σ xx + σ yŷ + σ zẑ where σ j with j = x, y, z are 2 × 2 Pauli's spin matrices [5,7]. The 2 × 2 identity matrix [I] = σ 0 has not been shown for the convenience of notation. The above equation may be rearranged by taking time-derivatives from each row of (2) and straightforward substitution, to yield the modified 4 × 4 Schrödinger's equation of the typesimilar to (1) with α = 1/mc 2 . Curiously, this value of α satisfies the expected upper bound of 7.2 × 10 23 J −1 [1]...