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A method for computing the stress-energy tensor for the quantized, massless,spin 1/2 field in a general static spherically symmetric spacetime ispresented. The field can be in a zero temperature state or a non-zerotemperature thermal state. An expression for the full renormalizedstress-energy tensor is derived. It consists of a sum of two tensors both ofwhich are conserved. One tensor is written in terms of the modes of thequantized field and has zero trace. In most cases it must be computednumerically. The other tensor does not explicitly depend on the modes and has atrace equal to the trace anomaly. It can be used as an analytic approximationfor the stress-energy tensor and is equivalent to other approximations thathave been made for the stress-energy tensor of the massless spin 1/2 field instatic spherically symmetric spacetimes.Comment: 34 pages, no figure

physical review. d. particles, fields, gravitation, and cosmology/physical review. d. particles and fields

Method to compute the stress-energy tensor for the massless spin<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mfrac><mml:mrow><mml:mn>1</mml:mn></mml:mrow><mml:mrow><mml:mn>2</mml:mn></mml:mrow></mml:mfrac></mml:math>field in a general static spherically symmetric spacetime

Method to compute the stress-energy tensor for the massless spin12field in a general static spherically symmetric spacetime