Quantum entanglement in Plebański-Demiański spacetimes

Hugo García-Compeán, Felipe Robledo-Padilla

Resultado de la investigaciónrevisión exhaustiva

3 Citas (Scopus)


For an Einstein-Podolsky-Rosen pair of spin-1/2 particles in circular orbits in a general axially symmetric spacetime, the spin precession angle is obtained. Hovering observers are introduced for ensuring fixed reference frames to perform suitable reliable measurements. Frame-dragging of spinning holes is explicitly incorporated relative to hovering observers. The spin-singlet state is found to be mixed with the spin-triplet by acceleration and gravity effects, which deteriorate the perfect anti-correlation of an entangled pair of spins measured by hovering observers. Finally, an algorithm to calculate spin precession for a general axially symmetric spacetime is proposed. This algorithm is applied to study the complete list of expanding and twisting Type-D Plebański-Demiański black holes and their descendent limiting solutions with lower parameters.

Idioma originalEnglish
Número de artículo235012
PublicaciónClassical and Quantum Gravity
EstadoPublished - 7 dic 2013

All Science Journal Classification (ASJC) codes

  • Física y astronomía (miscelánea)


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