Section I comprises questions 1–4; Section II comprises questions 5–8. Numbered subdivisions below retain the successive unlettered source blocks; letters retain the source's actual letters. The Symmetry and Relativity 2011 Exam Solution Notes answer much of Section II. Covered requests are linked to their precise pages; supplements below fill requests omitted or only referred elsewhere. These page references describe coverage, not an independent certification of every calculation in the notes.
Covered by the official notes: comparison with a 200 keV neutrino mass (PDF p. 12; handwritten p. 7).[ref]
The notes stop at “no change”; the experimental implication is that this is a poorly conditioned neutrino mass measurement. In relativistic two-body decay, the corrections to the rest-frame energy and momentum enter through the square of the daughter rest mass, while the Lorentz transformation boosts both the massless value and its small correction. A measured laboratory energy or angle must therefore resolve a very small change against beam-energy spread, decay-angle uncertainty and detector resolution. No visible change at the quoted precision does not establish zero neutrino mass.
Covered by the official notes: definition of a pure force via constant rest mass (PDF p. 13; handwritten p. 8).[ref]
The page labels as a proper force; that is the four-force. The requested proper force is the three-force measured in the instantaneous rest frame of the object. For a pure force its magnitude is times the proper acceleration, and in that frame the four-force has components .
Covered by the official notes: definitions of four-force and four-velocity and the vanishing antisymmetric contraction (PDF p. 15; handwritten p. 10).[ref]
To make the necessity statement precise, mass preservation must hold for every allowed timelike four-velocity, with the same field tensor and nonzero charge. It is not necessary for one prescribed trajectory alone. Use metric signature , so . Put . The mass-preservation condition requires the quadratic form for every timelike . Every timelike vector can be rescaled to a physical four-velocity; by homogeneity the quadratic form vanishes on the open timelike cone. A polynomial vanishing on an open set is identically zero, so . Thus the electromagnetic field tensor must be antisymmetric under this universal quantifier. For a single velocity, the scalar contraction can vanish even for a nonzero symmetric part, which is why the quantifier is essential.