CALCULATION OF THE a3 COEFFICIENT FOR SPINOR FIELD BY PROPER TIME EXPANSION METHOD
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Abstract
The a3 coefficient is an important and useful quantity from which one can evaluate the vacuum polarization energy-momentum tensors and revise Einstein's classical gravitational field equation to a semiclassical level. The a3 coefficient of spinor field is calculated by proper time expansion method in this article.
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Cite this article:
XU Dianyan. CALCULATION OF THE a3 COEFFICIENT FOR SPINOR FIELD BY PROPER TIME EXPANSION METHOD[J]. Chin. Phys. Lett., 1987, 4(1): 41-43.
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XU Dianyan. CALCULATION OF THE a3 COEFFICIENT FOR SPINOR FIELD BY PROPER TIME EXPANSION METHOD[J]. Chin. Phys. Lett., 1987, 4(1): 41-43.
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XU Dianyan. CALCULATION OF THE a3 COEFFICIENT FOR SPINOR FIELD BY PROPER TIME EXPANSION METHOD[J]. Chin. Phys. Lett., 1987, 4(1): 41-43.
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XU Dianyan. CALCULATION OF THE a3 COEFFICIENT FOR SPINOR FIELD BY PROPER TIME EXPANSION METHOD[J]. Chin. Phys. Lett., 1987, 4(1): 41-43.
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