Dark Matter and Dark Energy

By Utpal Sarkar. Springer Theses, 2007

286 citations recorded by the source corpus.

The existence of Dark Matter would explain several astrophysical observations not covered by the Standard Model of particle physics. The chapter introduces the Standard Model of cosmology and the currently most favoured candidate for Dark Matter, the weakly interacting massive particle.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/17e7b15cf0ed8a8719c9b5972982d9b1bc59ba07

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In Astronomy and Astrophysics

1. R. Loll
2. J. Jurkiewicz
3. J. Ambjrn
4. M. Niedermaier
5. Gianluca Calcagni
6. Martin Reuter
7. J. Ambjørn
8. R. Gurau

In Nuclear and High Energy Physics

1. R. Loll
2. J. Jurkiewicz
3. J. Ambjrn
4. Gianluca Calcagni
5. R. Gurau

Citations in the corpus

• The universe from scratch (2005, methodology): “ constant G N, governing the strength of gravitational interactions, and the cosmological constant λ, another constant of nature, which may be responsible for the “dark energy” pervading our universe [26]. As mentioned in footnote 10, all simplices used in DT are equilateral14, and the path integral”