These tools will no longer be maintained as of December 31, 2024. Archived website can be found here. PubMed4Hh GitHub repository can be found here. Contact NLM Customer Service if you have questions.
6. Why there is something rather than nothing: cosmological constant from summing over everything in lorentzian quantum gravity. Barvinsky AO Phys Rev Lett; 2007 Aug; 99(7):071301. PubMed ID: 17930882 [TBL] [Abstract][Full Text] [Related]
7. Can all cosmological observations be accurately interpreted with a unique geometry? Fleury P; Dupuy H; Uzan JP Phys Rev Lett; 2013 Aug; 111(9):091302. PubMed ID: 24033020 [TBL] [Abstract][Full Text] [Related]
9. First cosmological constraints on dark energy from the radial baryon acoustic scale. Gaztañaga E; Miquel R; Sánchez E Phys Rev Lett; 2009 Aug; 103(9):091302. PubMed ID: 19792779 [TBL] [Abstract][Full Text] [Related]
10. Exact solution to the averaging problem in cosmology. Wiltshire DL Phys Rev Lett; 2007 Dec; 99(25):251101. PubMed ID: 18233512 [TBL] [Abstract][Full Text] [Related]
12. Evolution of cosmological perturbations in a brane-universe. Langlois D Phys Rev Lett; 2001 Mar; 86(11):2212-5. PubMed ID: 11289892 [TBL] [Abstract][Full Text] [Related]
13. Why the cosmological constant is small and positive. Steinhardt PJ; Turok N Science; 2006 May; 312(5777):1180-3. PubMed ID: 16675662 [TBL] [Abstract][Full Text] [Related]
14. Producing a scale-invariant spectrum of perturbations in a Hagedorn phase of string cosmology. Nayeri A; Brandenberger RH; Vafa C Phys Rev Lett; 2006 Jul; 97(2):021302. PubMed ID: 16907429 [TBL] [Abstract][Full Text] [Related]
15. Value of H(0) in the inhomogeneous universe. Ben-Dayan I; Durrer R; Marozzi G; Schwarz DJ Phys Rev Lett; 2014 Jun; 112(22):221301. PubMed ID: 24949753 [TBL] [Abstract][Full Text] [Related]
16. Diamagnetic field states in cosmological plasmas. Asenjo FA; Mahajan SM Phys Rev E; 2019 May; 99(5-1):053204. PubMed ID: 31212428 [TBL] [Abstract][Full Text] [Related]