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  2. ER = EPR - Wikipedia

    en.wikipedia.org/wiki/ER_=_EPR

    ER = EPR is a conjecture in physics stating that two entangled particles (a so-called Einstein–Podolsky–Rosen or EPR pair) are connected by a wormhole (or Einstein–Rosen bridge) [1] [2] and is thought by some to be a basis for unifying general relativity and quantum mechanics into a theory of everything. [1]

  3. Wormhole - Wikipedia

    en.wikipedia.org/wiki/Wormhole

    Einstein–Rosen bridges (or ER bridges), [20] named after Albert Einstein and Nathan Rosen, [21] are connections between areas of space that can be modeled as vacuum solutions to the Einstein field equations, and that are now understood to be intrinsic parts of the maximally extended version of the Schwarzschild metric describing an eternal ...

  4. Nathan Rosen - Wikipedia

    en.wikipedia.org/wiki/Nathan_Rosen

    In 1934 he became Albert Einstein's assistant at The Institute for Advanced Study in Princeton, New Jersey, and continued in that position until 1936. [1] In July 1935 [4] Einstein and Rosen published an article developing a concept of folded space time in parallel layers connected by a bridge, using only General Relativity and Maxwell's equations.

  5. Regge calculus - Wikipedia

    en.wikipedia.org/wiki/Regge_calculus

    Einstein–Rosen bridge; Equations; ... Regge calculus is a formalism for producing simplicial approximations of spacetimes that are solutions to the Einstein field ...

  6. Einstein field equations - Wikipedia

    en.wikipedia.org/wiki/Einstein_field_equations

    The Einstein field equations (EFE) may be written in the form: [5] [1] + = EFE on the wall of the Rijksmuseum Boerhaave in Leiden, Netherlands. where is the Einstein tensor, is the metric tensor, is the stress–energy tensor, is the cosmological constant and is the Einstein gravitational constant.

  7. Einstein–Rosen metric - Wikipedia

    en.wikipedia.org/wiki/EinsteinRosen_metric

    In general relativity, the Einstein–Rosen metric is an exact solution to the Einstein field equations derived in 1937 by Albert Einstein and Nathan Rosen. [1] It is the first exact solution to describe the propagation of a gravitational wave .

  8. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    Einstein's equations can also be solved on a computer using sophisticated numerical methods. [1] [2] [3] Given sufficient computer power, such solutions can be more accurate than post-Newtonian solutions. However, such calculations are demanding because the equations must generally be solved in a four-dimensional space.

  9. Penrose diagram - Wikipedia

    en.wikipedia.org/wiki/Penrose_diagram

    The Einstein–Rosen bridge closes off (forming "future" singularities) so rapidly that passage between the two asymptotically flat exterior regions would require faster-than-light velocity, and is therefore impossible. In addition, highly blue-shifted light rays (called a blue sheet) would make it impossible for anyone to pass through.