Reproducing gravity through spinor fields

M. Novello and M. Borba1

Abstract

We show how to mimic gravitational processes described by general relativity using self-interacting spinor fields as the basic fundamental entities to describe gravity.

References

  1. Maria Borba, MSci Thesis (in Portuguese) (2009).
  2. M. Novello, Phys. Rev. D 8 (8), 2398 (1973).
  3. M. Novello, gr-qc/0609033.
  4. M. Novello, arXiv: 0705.2692.
  5. M. Novello, JCAP 6, 18 (2007).
  6. W. Heisenberg, Rev. Mod. Phys. 29, 269 (1957).
  7. C. M. Will, gr-qc/9811036. We are using the terminology of what is usually called the Einstein Equivalence Principle as presented, for instance, in this article by Will.
  8. L. P. Grishchuk, Sov. Phys. Usp. 33 (8), 669 (1990). See also L. P. Grishchuk, A. N. Petrov and A. D. Popova. Commun. Math. Phys. 94, 379 (1984).
  9. E. Elbaz, The Quantum Theory of Particles, Fields and Cosmology (Springer, 1998). See also V. W. Kofink, Ann. der Phys., Band 30, 91 (1937).
  10. R. P. Feynman, Feynman Lectures on Gravitation, (Addison-Wesley Publ. Co., 1995).
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