Rujukan Tenaga_gelap

  1. ↑ Peebles, P. J. E. dan Ratra, Bharat (2003). "The cosmological constant and dark energy". Reviews of Modern Physics. 75 (2): 559–606. arXiv:astro-ph/0207347. Bibcode:2003RvMP...75..559P. doi:10.1103/RevModPhys.75.559.Selenggaraan CS1: pelbagai nama: senarai pengarang (link)
  2. ↑ Ade, P. A. R.; Aghanim, N.; Armitage-Caplan, C.; et al. (Planck Collaboration) (22 Mac 2013). "Planck 2013 results. I. Overview of products and scientific results – Table 9" (PDF). Astronomy and Astrophysics (diserahkan). arXiv:1303.5062. Bibcode:2013arXiv1303.5062P. Tanda italik atau tebal tidak dibenarkan dalam: |journal= (bantuan)
  3. ↑ Ade, P. A. R.; Aghanim, N.; Armitage-Caplan, C.; et al. (Planck Collaboration) (31 March 2013). "Planck 2013 Results Papers". Astronomy and Astrophysics (diserahkan). arXiv:1303.5062. Bibcode:2013arXiv1303.5062P. Tanda italik atau tebal tidak dibenarkan dalam: |journal= (bantuan)
  4. ↑ "First Planck results: the Universe is still weird and interesting".
  5. ↑ Sean Carroll, Ph.D., Cal Tech, 2007, The Teaching Company, Dark Matter, Dark Energy: The Dark Side of the Universe, Guidebook Part 2 halaman 46, dicapai pada 7 Oktober 2013, "...dark energy: A smooth, persistent component of invisible energy, thought to make up about 70 percent of the current energy density of the universe. Dark energy is known to be smooth because it doesn't accumulate preferentially in galaxies and clusters..."
  6. ↑ http://hyperphysics.phy-astr.gsu.edu/hbase/astro/dareng.html

Rujukan

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