ABSTRACT
We prove that given an asymptotically flat (in a very weak sense) initial data set, there always exists a spinor field that satisfies Witten’s equation and that becomes constant at infinity. Thus we fill a gap in Witten’s arguments on the nonnegativity of the total mass of an isolated system, when measured at spatial infinity. We also include a review of Witten’s argument.
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- 18. With the adjoint given by one gets where is the spinor representation of the space‐time covariant derivative. Thus is the neutrino zero mode equation or Witten’s equation. Google Scholar
- 19. This identity is the spinorial version of the Green identity for scalars. Google Scholar
- 20. It is convenient for simplicity to use the second order equation (1.6) instead of Witten’s equation. In fact, they are equivalent, in the sense that every solution of (1.6) found in Sec. II satisfies Witten’s equation.25, Google Scholar
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- 26.To see this, note that for any of our solutions of (l.6), is square integrable. Thus, it suffices to show that the equation has no nontrivial solution in Assume, on the contrary, there exists one, Then, using identity (1.5) for and the local mass condition (1.9) we get
Here, with denotes a typical element of a one‐parameter family of nested surfaces (topologically ), and denotes the region enclosed by the The surfaces and the parameters are to be chosen so that Calling the left‐hand side of th expression above integrating it over and using the Hölder inequality, we get where But one can show there exists no function g which is positive, nondecreasing, and defined everywhere on and which satisfies the above inequality. - 27. It is immediate, from the form of that the volume integral in (1.7) is finite for any asymptotically flat initial data set, in the sense of Sec. II. Google Scholar
- 28. To see this, first note that T is diffeomorphic to The required flat metric on T is then chosen to agree with outside some compact set. Google Scholar
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