This paper primarily addresses the question of whether recent lensing observations probing the small-scale structure in the universe are consistent with the ACDM model. A conservative approach is taken, in which only the most difficult to explain cases of image flux anomalies in strong lenses are considered. Numerical simulations are performed to compare predictions for the ACDM small-scale mass function with observed flux ratios. By simulating several representative cases, it is found that all the cusp caustic lens anomalies and the disagreements between monochromatic flux ratios and simple lens models can be explained without any substructure in the primary lenses' dark matter halos. Intergalactic ACDM halos are enough to naturally explain these cases. However, thus far, spectroscopic gravitational lensing observations require more small-mass halos (∼106 M⊙) than are expected in the ACDM model © 2005. The American Astronomical Society. All rights reserved.
Metcalf, R.B. (2005). Testing ACDM with gravitational lensing constraints on small-scale structure. THE ASTROPHYSICAL JOURNAL, 622(1 I), 72-80 [10.1086/427864].
Testing ACDM with gravitational lensing constraints on small-scale structure
METCALF, ROBERT BENTON
2005
Abstract
This paper primarily addresses the question of whether recent lensing observations probing the small-scale structure in the universe are consistent with the ACDM model. A conservative approach is taken, in which only the most difficult to explain cases of image flux anomalies in strong lenses are considered. Numerical simulations are performed to compare predictions for the ACDM small-scale mass function with observed flux ratios. By simulating several representative cases, it is found that all the cusp caustic lens anomalies and the disagreements between monochromatic flux ratios and simple lens models can be explained without any substructure in the primary lenses' dark matter halos. Intergalactic ACDM halos are enough to naturally explain these cases. However, thus far, spectroscopic gravitational lensing observations require more small-mass halos (∼106 M⊙) than are expected in the ACDM model © 2005. The American Astronomical Society. All rights reserved.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.