TY - JOUR
T1 - The dark side of cosmology
T2 - Dark matter and dark energy
AU - Spergel, David N.
PY - 2015/3/6
Y1 - 2015/3/6
N2 - A simple model with only six parameters (the age of the universe, the density of atoms, the density of matter, the amplitude of the initial fluctuations, the scale dependence of this amplitude, and the epoch of first star formation) fits all of our cosmological data . Although simple, this standard model is strange. The model implies that most of the matter in our Galaxy is in the form of "dark matter," a new type of particle not yet detected in the laboratory, and most of the energy in the universe is in the form of "dark energy," energy associated with empty space. Both dark matter and dark energy require extensions to our current understanding of particle physics or point toward a breakdown of general relativity on cosmological scales.
AB - A simple model with only six parameters (the age of the universe, the density of atoms, the density of matter, the amplitude of the initial fluctuations, the scale dependence of this amplitude, and the epoch of first star formation) fits all of our cosmological data . Although simple, this standard model is strange. The model implies that most of the matter in our Galaxy is in the form of "dark matter," a new type of particle not yet detected in the laboratory, and most of the energy in the universe is in the form of "dark energy," energy associated with empty space. Both dark matter and dark energy require extensions to our current understanding of particle physics or point toward a breakdown of general relativity on cosmological scales.
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U2 - 10.1126/science.aaa0980
DO - 10.1126/science.aaa0980
M3 - Review article
C2 - 25745164
AN - SCOPUS:84924426882
SN - 0036-8075
VL - 347
SP - 1100
EP - 1102
JO - Science
JF - Science
IS - 6226
ER -