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  1.  11
    Contribution of Pressure to the Energy–Momentum Density in a Moving Perfect Fluid: A Physical Perspective.Ashok K. Singal - 2021 - Foundations of Physics 51 (1):1-20.
    In the energy–momentum density expressions for a relativistic perfect fluid with a bulk motion, one comes across a couple of pressure-dependent terms, which though well known, are to an extent, lacking in their conceptual basis and the ensuing physical interpretation. In the expression for the energy density, the rest mass density along with the kinetic energy density of the fluid constituents due to their random motion, which contributes to the pressure as well, are already included. However, in a fluid with (...)
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  2.  61
    Comment on “Exact Expression for Radiation of an Accelerated Charge in Classical Electrodynamics”.Ashok K. Singal - 2013 - Foundations of Physics 43 (2):267-270.
    It is shown that a newly derived “exact expression” for radiation of an accelerated charge in the recent literature is simply incorrect, having arisen because of a wrong relativistic transformation of the distance parameter. The ensuing claim that the newly derived expression alone satisfies the energy conservation for the electromagnetic radiation, is based on a wrong reasoning where a proper distinction between the time during which the radiation is received and the time for emission (retarded time of the charge) was (...)
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  3.  22
    Compatibility of Larmor’s Formula with Radiation Reaction for an Accelerated Charge.Ashok K. Singal - 2016 - Foundations of Physics 46 (5):554-574.
    It is shown that the well-known disparity in classical electrodynamics between the power losses calculated from the radiation reaction and that from Larmor’s formula, is succinctly understood when a proper distinction is made between quantities expressed in terms of a “real time” and those expressed in terms of a retarded time. It is explicitly shown that an accelerated charge, taken to be a sphere of vanishingly small radius \, experiences at any time a self-force proportional to the acceleration it had (...)
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  4.  11
    Implications of a Non-zero Poynting Flux at Infinity Sans Radiation Reaction for a Uniformly Accelerated Charge.Ashok K. Singal - 2021 - Foundations of Physics 51 (4):1-26.
    We investigate in detail the electromagnetic fields of a uniformly accelerated charge, in order to ascertain whether such a charge does ‘emit’ radiation, especially in view of the Poynting flow computed at large distances and taken as an evidence of radiation emitted by the charge. In this context, certain important aspects of the fields need to be taken into account. First and foremost is the fact that in the case of a uniformly accelerated charge, one cannot ignore the velocity fields. (...)
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