Author(s): Năstase, Horaţiu [UNESP]
Date: 2020
Persistent ID: http://hdl.handle.net/11449/200464
Origin: Oasisbr
Author(s): Năstase, Horaţiu [UNESP]
Date: 2020
Persistent ID: http://hdl.handle.net/11449/200464
Origin: Oasisbr
Made available in DSpace on 2020-12-12T02:07:22Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-01-01
In this chapter we will present the evidence for Dark Matter, and the resulting “Standard Model of Cosmology,” the Λ CDM model (cosmological constant plus cold dark matter). Dark Matter is what the name suggests, matter that is dark, i.e., non-luminous. That is, matter that we cannot detect from emitted light. I will present the evidences, then review the possible candidates for dark matter, and finish describing the Λ CDM model.
Instituto de Física Teórica UNESP
Instituto de Física Teórica UNESP