English (United Kingdom)

https://curated-unify.zendy.io/wp-json/zendy-region/v1/featured_content/oa?rat=en

https://curated-unify.zendy.io/wp-json/zendy-region/v1/highlighted_journal/

Global: Zendy Plus annual

Presents the access of premium content as premium feature

Premium Content

Presents the keyphrase highlighting as premium feature

Keyphrase Highlighting

Presents the summarisation as premium feature

Summarisation

Insights

Presents the pdf analysis as premium feature

PDF Analysis

Presents the zaia usage as premium feature

ZAIA

Global: Zendy Tools annual

Global: Zendy Free Plan

Global: Zendy Tools monthly

Global: Zendy Plus monthly

The stress-energy tensor of a quantized scalar field is computed in thereduced two-dimensional charged dilatonic black hole spacetime of Garfinkle,Horowitz, and Strominger. In order for the stress-energy of quantized fields tobe regular on the event horizon in both the extreme string metric and theconformally associated physical metric, it is necessary to assign a nonzerotemperature, T = (8 pi e^{phi_0} M)^{-1}, to the extreme string metric,contrary to the expectation that this horizonless spacetime would have anatural temperature of zero.Comment: 10 page, ReVTe

Quantized fields and temperature in charged dilatonic black hole spacetimes