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Normally one thinks of the observed cosmological constant as being so small that it can be utterly neglected on typical astrophysical scales, only affecting extremely large-scale cosmology at Gigaparsec scales.
1901
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Friedrich Kottler, “Über die physikalischen Grundlagen der Einsteinschen Relativitätstheorie”, Annalen der Physik 4 # 60
1918
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1979
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M. Visser and N. Yunes, “Power laws, scale invariance, and generalized Frobenius series: Applications to Newtonian and TOV stars near criticality”, Int. J. Mod. Phys. A 18
2003
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2005
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C. Cattöen and M. Visser, “Necessary and sufficient conditions for big bangs, bounces, crunches, rips, sudden singularities, and extremality events”, Class. Quant. Grav. 22
2005
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C. Barceló, S. Liberati and M. Visser, “Analogue gravity”, Living Rev. Rel. 8
2005
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C. Cattöen and M. Visser, “Cosmological milestones and energy conditions”, J. Phys. Conf. Ser. 68
2007
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2009
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2013
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2013
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2014
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T. Igata, “Stable bound orbits in six-dimensional Myers-Perry black holes”, Phys. Rev. D 92 # 2
2015
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2009
Cited alongside, same era.
T. Igata, H. Ishihara and Y. Takamori, “Stable bound orbits around black rings”, Phys. Rev. D 82
2010
Cited alongside, same era.
Z. Stuchlik and J Schee, “Influence of the cosmological constant on the motion of Magellanic Clouds in the gravitational field of Milky Way”, JCAP 9
2011
Cited alongside, same era.
See for instance https://en.wikipedia.org/wiki/Puiseux_series
Cited in the paper.
C. Cattöen and M. Visser, “Generalized Puiseux series expansion for cosmological milestones”, doi: 10.1142/9789812834300_0323 [arXiv: gr-qc/0609073]
Cited in the paper.
M. Visser, “Acoustic propagation in fluids: An unexpected example of Lorentzian geometry”, gr-qc/9311028
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2016
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2017
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