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Formation of wakes by chiral conducting cosmic strings
(World Scientific Publ Co Pte Ltd, 2004-10-20)
Chiral cosmic strings are naturally produced at the end of D-term inflation and they present very interesting cosmological consequences. In this work, we investigate the formation and evolution of wakes by a chiral string. ...
Formation of wakes by chiral conducting cosmic strings
(World Scientific Publ Co Pte Ltd, 2004-10-20)
Chiral cosmic strings are naturally produced at the end of D-term inflation and they present very interesting cosmological consequences. In this work, we investigate the formation and evolution of wakes by a chiral string. ...
An introduction to Large-scale Structure Formation
(Universidade Federal do Rio Grande do NorteBrasilUFRNFísica Bacharelado, 2019-12-05)
Formation of wakes by chiral conducting cosmic strings
(World Scientific Publ Co Pte Ltd, 2014)
Extended star formation history of the star cluster NGC 2154 in the Large Magellanic Cloud
(Wiley Blackwell Publishing, Inc, 2007-12)
The colour-magnitude diagram (CMD) of the intermediate-age Large Magellanic Cloud star cluster NGC 2154 and its adjacent field has been analysed using Padova stellar models to determine the cluster´s fundamental parameters ...
The origin of spin in galaxies: clues from simulations of atomic cooling haloes
(Oxford University Press, 2015)
In order to elucidate the origin of spin in both dark matter and baryons in galaxies, we have performed hydrodynamical simulations from cosmological initial conditions. We study atomic cooling haloes in the redshift range ...
Planet formation: statistics of spin rates and obliquities of extrasolar planets
(Oxford University Press, 2010-08)
We develop a simple model of planetary formation, focusing our attention on
those planets with masses less than 10M⊕ and studying particularly the primordial
spin parameters of planets resulting from the accretion of ...
Análisis estadísticos de superestructuras en el Universo /
(2011-02)
En esta tesis se presenta un nuevo método para determinar la probabilidad de encontrar eventos extremos en la distribución de materia oscura fría. En nuestra aproximación usamos un conjunto de simulaciones de N-Cuerpos ...