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The thermodynamic quantities of massless scalar, neutrino, electromagnetic, massless Rarita-Schwinger and gravitational fields near the general spherically symmetric static black holes are investigated by using the modified equation of state density due to the generalized uncertainty relation. It is shown that the thermodynamic quantities depend not only on the characteristic of the black hole but also on the spin of the fields and the size of minimal length.
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Keywords:
- generalized uncertainty relation /
- general spherically symmetric static black hole /
- thermodynamic quantity
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