Dark Matter and Dark Energy
By M. Kamionkowski. 2007
255 citations recorded by the source corpus.
This is a short review, aimed at a general audience, of several current subjects of research in cosmology. The topics discussed include the cosmic microwave background (CMB), with particular emphasis on its relevance for testing inflation; dark matter, with a brief review of astrophysical evidence and more emphasis on particle candidates; and cosmic acceleration and some of the ideas that have been put forward to explain it. A glossary of technical terms and acronyms is provided.
Subfields: Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/88fc59e4216ed6202be74273409b97b341376261
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Citations in the corpus
- Search for axion-like dark matter with ferromagnets (2020, methodology): “With azimuthal field B0 inside the magnetized toroid, the second term on the right-hand side of equation (1) represents the effective current density, Jeff 1⁄4 ωagaγa0 cosðωatÞB0=ðμ0cÞ I , as sourced by the axion-like dark matter field.”
- Bulk viscosity driving the acceleration of the Universe (2005, unknown): “ar X iv :a st ro -p h/ 05 03 36 2v 1 1 6 M ar 2 00 5”
- Smoothing supernova data to reconstruct the expansion history of the universe (2005, unknown): “The nature of dark energy has been the subject of much debate over the past decade (for reviews see Sahni & Starobinsky (2000); Carroll (2001); Peebles & Ratra (2003); Padmanabhan (2003); Sahni (2004)).”