Autor(es): Năstase, Horaţiu [UNESP]
Data: 2020
Identificador Persistente: http://hdl.handle.net/11449/200469
Origem: Oasisbr
Autor(es): Năstase, Horaţiu [UNESP]
Data: 2020
Identificador Persistente: http://hdl.handle.net/11449/200469
Origem: Oasisbr
Made available in DSpace on 2020-12-12T02:07:29Z (GMT). No. of bitstreams: 0 Previous issue date: 2019-01-01
In this chapter we will describe the Cosmic Microwave Background Radiation and its anisotropy. After describing the CMBR kinematics, we will see how primordial perturbations, in particular curvature perturbations, that were already observed, are described and propagate, and how they influence the CMBR.
Instituto de Física Teórica UNESP
Instituto de Física Teórica UNESP