Direct detection of universal expansion by holonomy in the McVittie spacetime
In general relativity, the parallel transfer of a vector around a closed curve in spacetime, or along two curves that together form a closed loop, usually results in a nonzero deficit angle between the vector’s initial and final positions. We show that such holonomy in the McVittie spacetime, which...
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Veröffentlicht in: | Physical review. D 2019-01, Vol.99 (2), p.024033, Article 024033 |
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Sprache: | eng |
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