Metric-sign qualification. With this paper's metric signature, b gives
The minus sign in the printed Larmor formula would therefore make a positive radiative loss negative. A concrete counterexample is an instant of rest with nonzero acceleration: , so the printed expression is . That sign is appropriate for the opposite metric signature. With the convention already fixed in question 1, positive emitted power instead is
Alternatively the printed negative quantity can be interpreted as the particle's signed radiative energy change, rather than the positive loss magnitude.
For fixed rest mass, resolve the acceleration parallel and perpendicular to the velocity, as in b. This gives
Writing , the Liénard radiated-power formula becomes . For uniform circular motion, the acceleration is perpendicular to the velocity; for straight-line motion it is parallel. Comparing the same particle at equal relativistic energy and equal laboratory acceleration magnitude therefore gives
This particular comparison makes the linear loss larger. The familiar larger loss from bending applies to a different comparison: at equal applied laboratory force magnitude , and , giving and . Stating which quantity is held fixed is essential.
Both the muon and electron have the same electric charge magnitude. At equal kinetic energy per particle, their Lorentz factors are , so the heavier muon has the smaller Lorentz factor. At equal total relativistic energy the same ordering follows from , provided that energy is large enough to create either particle.
If the equal-acceleration comparison of c is retained, . Thus the four-way instantaneous comparison selects
For positive , its smaller Lorentz factor reduces the power relative to an electron, and transverse acceleration reduces the power relative to longitudinal acceleration of the same magnitude. This conclusion follows from the constraint actually stated in c.
For the customary engineering comparison at equal applied force, the result changes. From c,
Under that comparison the choice is
Its longitudinal radiative power is smaller than an electron's by , while avoiding bending removes the extra factor. At a fixed bend radius , the circular loss is , giving the familiar suppression at fixed ultrarelativistic energy and .
An energy budget alone does not specify a unique optimization. The force, acceleration, bend radius, acceleration time, and length are otherwise unrestricted. For example, in a linear accelerator a constant small force gives radiative power proportional to , and reaching a specified final three-momentum takes time proportional to ; the total radiated energy therefore tends to zero as . One cannot infer a unique accelerator choice without an additional constraint. The standard practical preference is the second boxed answer, with its stated comparison. Muon decay introduces a separate lifetime constraint if slow acceleration is contemplated, but it was not part of the specified radiative-loss calculation.