Exact Solutions of Einstein's Field Equations: List of tables

By H. Stephani, D. Kramer, M. MacCallum, C. Hoenselaers, E. Herlt. 2003

1,952 citations recorded by the source corpus.

Subfields: Artificial Intelligence, Astronomy and Astrophysics, Oceanography

View Paper: https://www.semanticscholar.org/paper/ccc1e637f00d7c77fa6688d52d35234155e6f2aa

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Artificial Intelligence

1. M. Blau
2. Andrew Strominger
3. C. Lammerzahl

In Astronomy and Astrophysics

1. Jorge E Santos
2. Ó. J. Dias
3. V. Perlick
4. Benson Way
5. A. Luna
6. D. O’Connell
7. Isobel Nicholson
8. R. Monteiro

In Oceanography

1. J. Ovalle
2. M. O'loughlin
3. D. O’Connell
4. A. Luna
5. V. Lysov
6. M. Blau
7. Andrew Strominger
8. Alan Coley

Citations in the corpus

• Type D spacetimes and the Weyl double copy (2018, background): “15) 3See [84] or [85] for more details on this classification.”
• SEARCHING EXACT SOLUTIONS FOR COMPACT STARS IN BRANEWORLD: A CONJECTURE (2007, background): “2 lutions in general relativity [ 44 ]. Even for the simple case of a static perfect fluid, only very few reported exact solutions are of physical interest [45].”
• Geometrothermodynamics of black holes (2007, background): “In general relativity, the gravitational field of the most general black hole is described by the Kerr–Newman [ 24 ] solution that corresponds to a rotating, charged black hole.”
• Photon regions and shadows of accelerated black holes (2015, methodology): “gion. Evaluating PTfor rh1 and rh2 yields by (31) the horizontal angular diameter hof the shadow. The vertical angular radius corresponds to those boundary points where the tangent is horizontal. By (32) we have f(rv) := sin2 %v = 1 P2(rv) T2(r v), so the tangent is horizontal if df dr v (rv) = 0. T”
• From Navier-Stokes to Einstein (2011, methodology): “We consider the case of p = 2 to connect to the well-studied Petrov classification of spacetimes [37]).”
• Vanishing scalar invariant spacetimes in higher dimensions (2004, background): “All of these spacetimes belong to Kundt’s class, and hence the metric of these spacetimes can be expressed in an appropriate form in adapted coordinates [ 2 , 3]. VSI spacetimes can be classified according to their Petrovtype, Segre type and the vanishing or non-vanishing of the quantity τ . This le”
• Numerical methods for finding stationary gravitational solutions (2015, methodology): “These include inverse scattering methods, algebraically special solutions, Kerr-Schild techniques, applications of supersymmetry and generalised Harrison transformations [17, 30].”