期刊
PHYSICS LETTERS B
卷 491, 期 1-2, 页码 203-206出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/S0370-2693(00)00966-7
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Heat kernel expansion coefficients are calculated for vacuum fluctuations with distributional background potentials and field strengths. Terms up to and including t(5/2) are presented. (C) 2000 Elsevier Science B.V. All rights reserved.
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