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Luciano Casarini

Picture




interests
research: dark energy, structure formation, weak lensing, n-body & hydro simulations, data science
teaching: physics. math, stats, distance learning

experience
Visiting professor, UFES-DFIS, Brazil, 2014-present

Postdoctoral research assistant, FAPES/CNPq,  Brazil 2011-2014
Postdoctoral research assistant, UniMiB-DFO, Italy, 2007-2011
Research assistant, UniMiB-DFO, Italy, 2005-2006
Research assistant, CNR/IASF-BO, Italy, 2003-2005
Research assistant, UniFI, Italy, 2002-2003


cv: free (en), lattes (pt)
publications: inspire HEP, NASA-ADS & astroph
public codes: github

links
projects: Euclid, J-PAS, DEUS, EDECS, SPOrt, BaR-SPOrt
boltzmann: CAMB, CLASS
fisher: CosmicFish
mcmc: CosmoMC, Montepython, NumCosmo
n-body: PKDGRAV, Gasoline, RAMSES
forums: CosmoCoffee
group: Vox Charta

data science: Talking Machines, reddit

images & movies


Does a generalized Chaplygin gas correctly describe the cosmological dark sector?
R.F. vom Marttens, L. Casarini, W. Zimdahl, W.S. Hipólito-Ricaldi & D.F. Mota
accepted by Phys. Dark Univ.
generalized chaplygin model: variation of CMB power spectrum
generalized chaplygin model: variation of Tf(k) and P(k)
CMB and matter power spectra with non-linear dark-sector interactions
R.F. vom Marttens, L. Casarini, W.S. Hipólito-Ricaldi & W. Zimdahl
JCAP 1701, 50 (2017) [ADS]

scaling model: variation of CMB power spectrum
scaling model: variation of transfer function and matter power spectrum
Effects of coupled dark energy on the Milky Way and its satellites
C. Penzo, A. V. Macció, M. Baldi, L. Casarini & J. Oñorbe
Mon. Not. Roy. Astron. Soc. 461, 2490 (2016) [ADS]
Picture
Density maps at=0. From first row to last : halo alpha, halo beta, halo gamma, halo delta. From first column to last:  LCDM model, EXP003, EXP008e3 and EXP006 coupled models.
Picture
Density maps for halo epsilon in LCDM (upper panel),
and in EXP006 coupled cosmology (lower panel).
Dark MaGICC: the effect of dark energy on disc galaxy formation. Cosmology does matter
C. Penzo, A. V. Macció, L. Casarini, G. S. Stinson & J. Wadsley
Mon. Not. Roy. Astron. Soc. 442, 176 (2014) [ADS]
SUCDM model : gas + star (galaxy gamma)
SUCDM model : gas + star (galaxy gamma)
waCDM model : gas + star (galaxy gamma)
waCDM model : gas + star (galaxy gamma)
SUCDM model : star only (galaxy gamma)
SUCDM model : metals galaxy (gamma)
waCDM model : star only (galaxy gamma)
 waCDM model : metals (galaxy gamma)

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Website administrators:  DC. Rodrigues, V. Marra & OF. Piattella. Contributions: several students and postdocs have helped to expand and maintain the content that can be found here, specially in the organization of the events section, where their corresponding names can be found. Disclamer: Cosmo-ufes is a center ("núcleo") from UFES; this website is maintained by Cosmo-ufes members.