By NelmaS on Qui, 06/07/2017 - 23:06
Morgan Le Delliou
Instituto de Fısica Teorica, Universidade Estadual de Sao Paulo, Brazil
I will discuss our paper that extends past works of Del Popolo that obtained a high precision mass function using the excursion set approach and an improved barrier, taking implicitly into account a non-zero cosmological constant, the angular momentum acquired by tidal interaction of proto-structures and dynamical friction. In the ΛCDM paradigm, we found that our MF is in agreement at the 3% level to Klypin’s Bolshoi simulation, in the mass range Mvir = 5 X 109 h−1 Msun — 5 X 1014 h−1 Msun and redshift range 0 < z < 10. For z = 0 we also compared our MF to several fitting formulae, and found in particular agreement with Bhattacharya’s within 3% in the mass range 1012 − 1016 h−1 Msun.
10 de julho de 2017 | 12:00
Faculdade de Ciências da Universidade de Lisboa (C6.2.51)
Campo Grande, 1749-016 Lisboa