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A curved static de Sitter-like metric is analyzed. The source of curvature isrooted from a constant stress tensor with positive energy density and negativepressures. All the curvature invariants are constant everywhere and thegeometry is conformally flat. The horizon surface gravity equals the parameter$\omega$ from the metric that is also interpreted as an angular velocity. TheTolman-Komar gravitational energy is investigated. One finds that the horizonentropy satisfies the relation $S = A_{H}/4$, as for the black hole horizon.

On a de Sitter-like spacetime with cylindrical symmetry