The sources of the vacuumC-metric

Bonnor, W. B.

doi:10.1007/bf00759569

Cited by 97 publications

(130 citation statements)

References 18 publications

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“…It is known that semi-infinite line source and finite line source with mass density 1 2 are associated, through the Weyl solutions, to Rindler and Schwarzschild spacetimes respectively [32] [20]. Thus, if the cubic (2) has three distinct real roots, the roots of F will be associated to the line sources and the roots of G will be associated to pieces of the z-axis.…”

Section: Metric and Weyl Coordinatesmentioning

confidence: 99%

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Uniformly accelerated black holes

Letelier

Oliveira

2001

Phys. Rev. D

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The static and stationary C-metric are revisited in a generic framework and their interpretations studied in some detail. Specially those with two event horizons, one for the black hole and another for the acceleration. We found that: i) The spacetime of an accelerated static black hole is plagued by either conical singularities or lack of smoothness and compactness of the black hole horizon; ii) By using standard black hole thermodynamics we show that accelerated black holes have higher Hawking temperature than Unruh temperature of the accelerated frame; iii) The usual upper bound on the product of the mass and acceleration parameters (< 1/ √ 27) is just a coordinate artifact. The main results are extended to accelerated rotating black holes with no significant changes.

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Section: Metric and Weyl Coordinatesmentioning

confidence: 99%

“…The charged C-metric is interpreted as the solution for Einstein-Maxwell equations for a charged particle moving with uniform acceleration [16]. Another possible interpretation is the spacetime of two Schwarzschild-type particles joined by a spring moving with uniform acceleration [20].…”

Section: Introductionmentioning

confidence: 99%

Uniformly accelerated black holes

Letelier

Oliveira

2001

Phys. Rev. D

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“…3 Spherical prolate coordinates are a special case of C-metric coordinates; see [29,30] and references therein. Our spherical prolate diagrams are analogs of C-metric diagrams in [31].…”

Section: Singularity Locus and Affine Coordinatesmentioning

confidence: 99%

How to stop (worrying and love) the bubble: boundary changing solutions

Jones

Wang

2007

J. High Energy Phys.

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We discover that a class of bubbles of nothing are embedded as time dependent scaling limits of previous spacelike-brane solutions. With the right initial conditions, a near-bubble solution can relax its expansion and open the compact circle. Thermodynamics of the new class of solutions is discussed and the relationships between brane/flux transitions, tachyon condensation and imaginary D-branes are outlined. Finally, a related class of simultaneous connected S-branes are also examined.

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“…Geometrical and asymptotic properties were subsequently studied in [5], [6]. Bonnor [7] found a transformation of the C-metric into the boost-rotational canonical form. However, the explicit metric functions are somewhat complicated and depend on specific ranges of the initial "static" coordinates [7]- [10].…”

Section: Introductionmentioning

confidence: 99%

“…Bonnor [7] found a transformation of the C-metric into the boost-rotational canonical form. However, the explicit metric functions are somewhat complicated and depend on specific ranges of the initial "static" coordinates [7]- [10]. Recently the limit of unbounded acceleration A → ∞ was investigated [11].…”

Section: Introductionmentioning

confidence: 99%