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Иш: Signature flips in time-varying $\Lambda (t)$ cosmological models with observational data
<tt>emcee</tt>: The MCMC Hammer
Daniel Foreman-Mackey, David W. Hogg, Dustin Lang +1
Мақола2013108 иқтибосABIMeasurements of Ω and Λ from 42 High‐Redshift Supernovae
S. Perlmutter, G. Aldering, G. Goldhaber +30
Мақола1999103 иқтибосABICoincident general relativity
Jose Beltrán Jiménez, Lavinia Heisenberg, Tomi Koivisto
Мақола201837 иқтибосABIAn alternative to quintessence
Alexander Yu. Kamenshchik, Ugo Moschella, Vincent Pasquier
Мақола200134 иқтибосABIStatefinder—A new geometrical diagnostic of dark energy
Varun Sahni, Tarun Deep Saini, Alexei A. Starobinsky +1
Мақола200329 иқтибосABITwo new diagnostics of dark energy
Varun Sahni, Arman Shafieloo, Alexei A. Starobinsky
Мақола200826 иқтибосABIAnisotropic nature of space–time in <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline" id="d1e1494" altimg="si9.svg"> <mml:mrow> <mml:mi>f</mml:mi> <mml:mfenced open="(" close=")"> <mml:mrow> <mml:mi>Q</mml:mi> </mml:mrow> </mml:mfenced> </mml:mrow> </mml:math> gravity
M. Koussour, S. H. Shekh, М. Беннаи
Мақола202220 иқтибосABICosmological consequences of a rolling homogeneous scalar field
Bharat Ratra, P. J. E. Peebles
Мақола198818 иқтибосABI