GALACTIC NONLINEAR DYNAMIC MODEL


Autoria(s): De Melo, C. A. M.; Resende, S. T.
Contribuinte(s)

Universidade Estadual Paulista (UNESP)

Data(s)

30/09/2013

20/05/2014

30/09/2013

20/05/2014

10/04/2009

Resumo

We develop a model for spiral galaxies based on a nonlinear realization of the Newtonian dynamics starting from the momentum and mass conservations in the phase space. The radial solution exhibits a rotation curve in qualitative accordance with the observational data.

Formato

1669-1673

Identificador

International Journal of Modern Physics A. Singapore: World Scientific Publ Co Pte Ltd, v. 24, n. 8-9, p. 1669-1673, 2009.

0217-751X

http://hdl.handle.net/11449/24275

WOS:000265092600040

Idioma(s)

eng

Publicador

World Scientific Publ Co Pte Ltd

Relação

International Journal of Modern Physics A

Direitos

closedAccess

Palavras-Chave #Galactic rotation curves #dark matter #mathematical modeling
Tipo

info:eu-repo/semantics/article