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1
On the Relation between the Expansion and the Mean Density of the Universe.
Proc Natl Acad Sci U S A. 1932 Mar;18(3):213-4. doi: 10.1073/pnas.18.3.213.
2
A lightweight universe?
Proc Natl Acad Sci U S A. 1998 May 26;95(11):5956-9. doi: 10.1073/pnas.95.11.5956.
3
The past and the future fate of the universe and the formation of structure in it.
Proc Natl Acad Sci U S A. 1999 Jul 20;96(15):8334-5. doi: 10.1073/pnas.96.15.8334.
5
Sequestration of vacuum energy and the end of the universe.
Phys Rev Lett. 2015 Mar 13;114(10):101302. doi: 10.1103/PhysRevLett.114.101302. Epub 2015 Mar 10.
6
Value of H(0) in the inhomogeneous universe.
Phys Rev Lett. 2014 Jun 6;112(22):221301. doi: 10.1103/PhysRevLett.112.221301.
7
A flat Universe from high-resolution maps of the cosmic microwave background radiation.
Nature. 2000 Apr 27;404(6781):955-9. doi: 10.1038/35010035.
8
Age estimates of globular clusters in the Milky Way: constraints on cosmology.
Science. 2003 Jan 3;299(5603):65-9. doi: 10.1126/science.1075631.
9
Size and age of the universe.
Science. 1981 Aug 21;213(4510):825-30. doi: 10.1126/science.213.4510.825.

引用本文的文献

1
100 years of mathematical cosmology: Models, theories, and problems, Part A.
Philos Trans A Math Phys Eng Sci. 2022 May 2;380(2222):20210191. doi: 10.1098/rsta.2021.0191. Epub 2022 Mar 14.
2
Chaotic universe model.
Sci Rep. 2018 Jan 15;8(1):721. doi: 10.1038/s41598-017-18681-4.
3
Cosmic vacuum energy decay and creation of cosmic matter.
Naturwissenschaften. 2007 Sep;94(9):709-24. doi: 10.1007/s00114-007-0235-1. Epub 2007 Apr 25.
4
Hubble's diagram and cosmic expansion.
Proc Natl Acad Sci U S A. 2004 Jan 6;101(1):8-13. doi: 10.1073/pnas.2536799100. Epub 2003 Dec 26.

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