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Title: Entropic force and entanglement system

Abstract

We introduce the isothermal cavity, static holographic screen, and accelerating surface as holographic screen to study the entropic force in the presence of the Schwarzschild black hole. These may merge to provide a consistent holographic screen to define the entropic force on the stretched horizon near the event horizon. Considering the similarity between the stretched horizon of black hole and the entanglement system, we may define the entropic force in the entanglement system without referring to the source mass.

Authors:
;  [1]
  1. Institute of Basic Science and School of Computer Aided Science, Inje University, Gimhae 621-749 (Korea, Republic of)
Publication Date:
OSTI Identifier:
21409770
Resource Type:
Journal Article
Journal Name:
Physical Review. D, Particles Fields
Additional Journal Information:
Journal Volume: 81; Journal Issue: 10; Other Information: DOI: 10.1103/PhysRevD.81.105012; (c) 2010 The American Physical Society; Journal ID: ISSN 0556-2821
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; BLACK HOLES; CAVITIES; ENTROPY; HOLOGRAPHY; MASS; QUANTUM ENTANGLEMENT; SCHWARZSCHILD METRIC; SURFACES; METRICS; PHYSICAL PROPERTIES; THERMODYNAMIC PROPERTIES

Citation Formats

Myung, Yun Soo, and Kim, Yong-Wan. Entropic force and entanglement system. United States: N. p., 2010. Web. doi:10.1103/PHYSREVD.81.105012.
Myung, Yun Soo, & Kim, Yong-Wan. Entropic force and entanglement system. United States. https://doi.org/10.1103/PHYSREVD.81.105012
Myung, Yun Soo, and Kim, Yong-Wan. 2010. "Entropic force and entanglement system". United States. https://doi.org/10.1103/PHYSREVD.81.105012.
@article{osti_21409770,
title = {Entropic force and entanglement system},
author = {Myung, Yun Soo and Kim, Yong-Wan},
abstractNote = {We introduce the isothermal cavity, static holographic screen, and accelerating surface as holographic screen to study the entropic force in the presence of the Schwarzschild black hole. These may merge to provide a consistent holographic screen to define the entropic force on the stretched horizon near the event horizon. Considering the similarity between the stretched horizon of black hole and the entanglement system, we may define the entropic force in the entanglement system without referring to the source mass.},
doi = {10.1103/PHYSREVD.81.105012},
url = {https://www.osti.gov/biblio/21409770}, journal = {Physical Review. D, Particles Fields},
issn = {0556-2821},
number = 10,
volume = 81,
place = {United States},
year = {Sat May 15 00:00:00 EDT 2010},
month = {Sat May 15 00:00:00 EDT 2010}
}