1982
DOI: 10.1007/978-94-015-7666-6
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General Relativity and Matter

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Cited by 65 publications
(81 citation statements)
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References 9 publications
(16 reference statements)
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“…We can see that the double Weiner process alluded is also connected with such an effect: The negative time derivative, which does not equal the positive time derivative in this case, represents negative energy states. However if we analyse the stochastic Schrodinger equation question further, and generalise the one dimensional case we consider to three dimensions, then as is well known [22], ı → σ, where σ are the Pauli matrices. In other words, we not only cross over to special relativity, but also recover the non commutative geometry (4) or Snyder's relations alluded to, at the Compton scale.…”
Section: Discussionmentioning
confidence: 99%
“…We can see that the double Weiner process alluded is also connected with such an effect: The negative time derivative, which does not equal the positive time derivative in this case, represents negative energy states. However if we analyse the stochastic Schrodinger equation question further, and generalise the one dimensional case we consider to three dimensions, then as is well known [22], ı → σ, where σ are the Pauli matrices. In other words, we not only cross over to special relativity, but also recover the non commutative geometry (4) or Snyder's relations alluded to, at the Compton scale.…”
Section: Discussionmentioning
confidence: 99%
“…Even-degree (integral-spin) polynomials build geometric fields; e.g. the tetrads, metric, and curvature tensors [1]. Odd-degree (half-integral-spin) polynomials represent the matter fields of Fermions.…”
Section: Introductionmentioning
confidence: 99%
“…Mendel Sachs' [1] dubbed this group of spin isometries the Einstein group, E. Van der Waerden had shown in 1933 [2] how to build all spin-vector.and spin-tensor representations of any isometry group as polynomials in the tensor products of irreducible left (L) chirality, of ( 89 and right (R) chirality, or (0, 89 spinors. Even-degree (integral-spin) polynomials build geometric fields; e.g.…”
Section: Introductionmentioning
confidence: 99%
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“…25 From the standpoint of general relativity, the excess energy from spacetime is freely allowed, since all EM energy moves in curved spacetime [33,36,37,[41][42][43]45,63] a priori, and simple conservation of EM energy as usually stated in classical equilibrium electrodynamics need not apply in a general relativistic situation [53,54].…”
Section: H Regauging Can Be Negentropic or Entropicmentioning
confidence: 99%