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		<title>82.48.76.161: Creata pagina con &#039;===CURRICULUM===  *Education Ph.D. In Physics, Department of Astronomy, University of Trieste, 4/14/2005 Thesis title: Hydrodynamical Simulations of Galaxy Clusters: Thermodyn...&#039;</title>
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		<updated>2012-11-02T11:13:24Z</updated>

		<summary type="html">&lt;p&gt;Creata pagina con &amp;#039;===CURRICULUM===  *Education Ph.D. In Physics, Department of Astronomy, University of Trieste, 4/14/2005 Thesis title: Hydrodynamical Simulations of Galaxy Clusters: Thermodyn...&amp;#039;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;Nuova pagina&lt;/b&gt;&lt;/p&gt;&lt;div&gt;===CURRICULUM===&lt;br /&gt;
&lt;br /&gt;
*Education&lt;br /&gt;
Ph.D. In Physics, Department of Astronomy, University of Trieste, 4/14/2005&lt;br /&gt;
Thesis title:&lt;br /&gt;
Hydrodynamical Simulations of Galaxy Clusters: Thermodynamics and Chemical Enrichment.&lt;br /&gt;
Advisor:&lt;br /&gt;
Prof. Stefano Borgani&lt;br /&gt;
Graduation in Physics, Department of Physics, University of Padova, Italy, 12/21/1999.&lt;br /&gt;
Thesis title:&lt;br /&gt;
Effects of Radiative Cooling and Supernovae Heating on the Evolution of Intra-Cluster Medium&lt;br /&gt;
Advisor:&lt;br /&gt;
Dr. Ornella Pantano&lt;br /&gt;
&lt;br /&gt;
Other Education Experiences&lt;br /&gt;
Summer School on Parallel Computing, 1999,&lt;br /&gt;
held at supercomputing centre CINECA, Bologna&lt;br /&gt;
Positions held&lt;br /&gt;
May 2005 – May 2007 : post-doc at S.I.S.S.A, Trieste&lt;br /&gt;
June 2007 – April 2010: post-doc at Department of&lt;br /&gt;
Astronomy, University of Trieste&lt;br /&gt;
&lt;br /&gt;
*Research interests&lt;br /&gt;
Cosmology and Large Scale Structure of the Universe&lt;br /&gt;
Numerical Simulations of large-scale structure, IGM and Galaxy Clusters.&lt;br /&gt;
Physics of Intra-Cluster Medium in Galaxy Clusters and Galaxies-ICM interplay&lt;br /&gt;
Physics of Intergalactic Medium and Galaxies-IGM interplay&lt;br /&gt;
Chemical Enrichment of Intergalactic Medium and Intracluster Medium&lt;br /&gt;
The focus of the research activity is mainly on the chemo/thermodynamical properties of baryons in both gaseous and stellar&lt;br /&gt;
component, and on their evolution across the Universe history in different environments (voids, diffuse medium, collapsed objects).&lt;br /&gt;
Particularly, the interest is on the interplay between gas and galaxies in both Galaxy Clusters and IGM, on the galactic feedback mechanisms at different ages, and on the evolution of galactic properties and IGM properties at both low and high redshifts.&lt;br /&gt;
A specific attention is given to the chemical enrichment of the&lt;br /&gt;
universe.&lt;br /&gt;
&lt;br /&gt;
*Working experience&lt;br /&gt;
He has accumulated a significant experience in collaborative working within large international groups being&lt;br /&gt;
involved in large programs of numerical simulations and european networks.&lt;br /&gt;
In particular, he is actively developing the Gadget code widely used for cosmological and astrophysical simulations in&lt;br /&gt;
collaboration with MPA group (Volker Springel, the developers&amp;#039;&lt;br /&gt;
In the framework of that involvement, he has been visiting MPA institute in Garching several times between 2003 and 2009, for a total period of about a year.&lt;br /&gt;
He has been involved in the large OWLS collaboration in Leiden, where he has been visiting in 2005 and 2007. Along with&lt;br /&gt;
collaborators Stefano Borgani and Matteo Viel has been involved in two Virgo consortium meetings (2007 at Leiden University, 2008 at Nottingham University) for setting up collaborations and projects.&lt;br /&gt;
He has been involved in the CosmoComp European network.&lt;br /&gt;
&lt;br /&gt;
*Reviewing Activity&lt;br /&gt;
He reviews papers for the following journals:&lt;br /&gt;
Astrophysical Journal&lt;br /&gt;
Monthly Notices of Royal Astronomical Society&lt;br /&gt;
Related Skills&lt;br /&gt;
Professional knowledge in scientific and non-scientific computer science nine-years experience in parallel computer programming and in developing massively parallel applications for cosmological simulations nine-year experience in international collaboration for co-developing segments of a worldwide-used parallel&lt;br /&gt;
code, and projecting and running very large numerical simulations on international facilities experience in developing massively parallel codes for analysis of large simulations and comparison with&lt;br /&gt;
&lt;br /&gt;
*Teaching Experiences&lt;br /&gt;
Introduction to programming / Numerical Methods&lt;br /&gt;
(partial) at S.I.S.S.A., Trieste,&lt;br /&gt;
2005-2006&lt;br /&gt;
2006-2007&lt;br /&gt;
&lt;br /&gt;
Lecture on advancend numerical methods in&lt;br /&gt;
astrophysics at the Advacend School on Parallel Computation, 2006, CINECA, Bologna&lt;br /&gt;
Co-supervision of undergraduate students at Department of Astronomy, Trieste&lt;br /&gt;
&lt;br /&gt;
Alexandro Saro 2005 now post-doc at the same Dep.&lt;br /&gt;
Dunja Fabjan 2006 now Ph.D. Student at the same Dep.&lt;br /&gt;
Massimo Viola 2008 now Ph.D. Student in Heidelberg&lt;br /&gt;
Filippo Bonaventura 2008&lt;br /&gt;
&lt;br /&gt;
Co-supervision of Ph.D. Students at Department of Astronomy, Trieste&lt;br /&gt;
Alexandro Saro 2006 – 2009 now post-doc at the same Dep.&lt;br /&gt;
Edoardo Tescari 2008 – 2009 (still in progress)&lt;br /&gt;
Dunja Fabjan 2007 – 2009 (still in progress)&lt;br /&gt;
at S.I.S.S.A., Trieste&lt;br /&gt;
Marco Valdes 2006-2009 now post-doc at IPMU, Tokio U.at MPA, Garching&lt;br /&gt;
Umberto Maio 2006-2009 now post-doc at MPE, garching&lt;br /&gt;
&lt;br /&gt;
*Publications on Refereed Journals&lt;br /&gt;
Tornatore, L., Borgani, S., Viel, M., Springel, V.&lt;br /&gt;
The impact of feedback on the low redshift Intergalactic medium&lt;br /&gt;
2009, MNRAS, Dayal, P.; Ferrara, A.; Saro, A.; Salvaterra, R.;&lt;br /&gt;
Borgani, S.; Tornatore, L&lt;br /&gt;
&lt;br /&gt;
Lyman Alpha emitter evolution in the reionization epoch&lt;br /&gt;
MNRAS, 2009, in press&lt;br /&gt;
Fabjan, D., Borgani, S., Tornatore, L., Saro, A., Murante, G., Dolag, K.&lt;br /&gt;
&lt;br /&gt;
Simulating the effect of AGN feedback on the metal enrichment of galaxy clusters&lt;br /&gt;
MNRAS, 2009, in press Wiersma, Robert P. C.; Schaye, Joop; Theuns, Tom;&lt;br /&gt;
Dalla Vecchia, Claudio; Tornatore, Luca&lt;br /&gt;
&lt;br /&gt;
Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations&lt;br /&gt;
MNRAS, 2009, 399, 574&lt;br /&gt;
Maio, U., Ciardi, B., Yoshida, N., Dolag, K., Tornatore, L.&lt;br /&gt;
&lt;br /&gt;
The onset of star formation in primordial halos&lt;br /&gt;
MNRAS, 2009, 503, 25&lt;br /&gt;
Tescari, E., Viel. M., Tornatore, L., Borgani, S.&lt;br /&gt;
&lt;br /&gt;
Dampde Lyman-alpha systems in high-resolution hydrodynamical simulations&lt;br /&gt;
MNRAS, 397, 411&lt;br /&gt;
Saro, A., Borgani, S., Tornatore, L., De Lucia, G., Dolag, K., Murante, G.&lt;br /&gt;
&lt;br /&gt;
Simulating the formation of a protocluster at z~2&lt;br /&gt;
MNRAS, 2009, 392, 795&lt;br /&gt;
Borgani, S., Fabjan, D., Tornatore, L., Schindler, S., Dolag, K., Diaferio, A.&lt;br /&gt;
&lt;br /&gt;
The chemical enrichment of the ICM frombhydrodynamical simulations&lt;br /&gt;
SSRV, 2008, 134, 379&lt;br /&gt;
Fabjan, D., Tornatore, L., Borgani, S., Saro, A., Dolag, K.&lt;br /&gt;
&lt;br /&gt;
Evolution of the metal content of the intra-cluster medium with hydrodynamical simulations&lt;br /&gt;
2008, MNRAS, in press&lt;br /&gt;
Cora, S. A., Tornatore, L., Tozzi, P., Dolag, K.&lt;br /&gt;
&lt;br /&gt;
On the dynamical origin of the ICM metallicity evolution&lt;br /&gt;
2008, MNRAS, in press&lt;br /&gt;
Rasia, E., Mazzotta, P., Bourdin, H., Borgani, S., Tornatore, L., Ettori, S., Dolag, K., Moscardini, L.&lt;br /&gt;
&lt;br /&gt;
X-Mas2 : study systematics on the ICM metallicity measurements&lt;br /&gt;
2008, ApJ, 674, 728&lt;br /&gt;
Viola, M., Monaco, P., Borgani, S., Murante, G.,&lt;br /&gt;
Tornatore, L., How does gas cool in dark matter haloes?&lt;br /&gt;
MNRAS, 2008, 383, 777&lt;br /&gt;
Tornatore, L., Borgani, S., Dolag, K., Matteucci, F.&lt;br /&gt;
&lt;br /&gt;
Chemical enrichment of galaxy clusters fromv hydrodynamical simulations&lt;br /&gt;
MNRAS, 2007, 382, 1050.&lt;br /&gt;
Tornatore, L., Ferrara, A., Schneider, R.&lt;br /&gt;
&lt;br /&gt;
Population III stars: hidden or disappeared?&lt;br /&gt;
MNRAS, 2007, 382 945.&lt;br /&gt;
Maio, U., Dolag, K., Ciardi, B., Tornatore L.&lt;br /&gt;
&lt;br /&gt;
Metal and molecule cooling in simulations of structure formation 2007, MNRAS, 379, 963.&lt;br /&gt;
Borgani, S., Dolag, K., Murante, G., Cheng, L.-M.,&lt;br /&gt;
Springel, V., Diaferio, A., Moscardini, L., Tormen, G.,&lt;br /&gt;
Tornatore, L., Tozzi, P. Hot and cooled baryons in smoothed particle hydrodynamic simulations of galaxy&lt;br /&gt;
&lt;br /&gt;
clusters: physics and numerics&lt;br /&gt;
2006, MNRAS, 367, 1641&lt;br /&gt;
Saro, A., Borgani, S., Tornatore, L., Dolag, K., Murante,&lt;br /&gt;
G., Biviano, A., Calura, F., Charlot, S.&lt;br /&gt;
&lt;br /&gt;
Properties of the galaxy population in hydrodynamical simulations of clusters&lt;br /&gt;
2006, MNRAS, 373, 397&lt;br /&gt;
Diaferio, A., Borgani, S., Moscardini, L., Murante, G., Dolag, K., Springel, V., Tormen, G., Tornatore, L., Tozzi, P.&lt;br /&gt;
2005, MNRAS, 356, 1477&lt;br /&gt;
Cheng, L.M., Borgani, S., Tozzi, P., Tornatore, L., Diaferio, A., Dolag, K., He, X.T., Moscardini, L., Murante,  G., Tormen, G. 2005, A&amp;amp;A, 431, 405&lt;br /&gt;
Ettori, S., Borgani, S., Moscardini, L., Murante, G., Tozzi, P., Diaferio, A., Dolag, K., Springel, V., Tormen, G., Tornatore,L. 2004, MNRAS, 354, 111&lt;br /&gt;
Murante, G., Arnaboldi,M., Gerhard, O., Borgani, S., Cheng, L.M., Diaferio, A., Dolag, K., Moscardini, L.,&lt;br /&gt;
Tormen, G., Tornatore, L., Tozzi, P.&lt;br /&gt;
2004, ApJL, 607, 83&lt;br /&gt;
Tornatore, L., Borgani, S., Matteucci, F., Recchi, S., Tozzi, P.&lt;br /&gt;
2004, MNRAS, 349L, 19&lt;br /&gt;
Borgani, S., Murante, G., Springel, V., Diaferio, A., Dolag, K., Moscardini, L., Tormen, G., Tornatore, L., Tozzi, P.&lt;br /&gt;
2004, MNRAS, 348, 1078&lt;br /&gt;
Tornatore, L., Borgani, S., Springel, V., Matteucci, F., Menci, N., Murante, G.&lt;br /&gt;
2003, MNRAS, 342, 1025&lt;br /&gt;
Finoguenov, A., Borgani, S., Tornatore, L., Böhringer, H.&lt;br /&gt;
2003, A&amp;amp;A, 398L, 35&lt;br /&gt;
&lt;br /&gt;
Contributed talks in international conferences Tornatore, L., Borgani, S.&lt;br /&gt;
The Impact of Feedback on the Low-Redshift&lt;br /&gt;
Intergalactic Medium&lt;br /&gt;
2009, The Chemical Enrichment of the Intergalactic&lt;br /&gt;
Medium – Lorentz center, Leiden University&lt;br /&gt;
Tornatore, L., Borgani, S., Murante, G., Dolag, K., Saro,&lt;br /&gt;
A., Fabjan, D.&lt;br /&gt;
&lt;br /&gt;
Studying the chemical properties of ICM using numerical simulations&lt;br /&gt;
2007, Sesto 2007 – Tracing Cosmic Evolution with&lt;br /&gt;
&lt;br /&gt;
Galaxy Clusters&lt;br /&gt;
Tornatore, L., Borgani, S., Chemical enrichment of galaxy clusters in hydrodynamical simulations,&lt;br /&gt;
2006, in “CRAL-2006 – chemodynamics: from first stars to local galaxies,”EAS, 24, 2007 Tornatore, L., Borgani, S.&lt;br /&gt;
&lt;br /&gt;
The history of ICM&amp;#039;s enrichment in simulations&lt;br /&gt;
2005, Ringberg workshop M87, Distant Clusters of&lt;br /&gt;
Galaxies&lt;br /&gt;
Tornatore, L., Borani, S.&lt;br /&gt;
&lt;br /&gt;
Galaxy clusters chemodynamics in numerical simulations&lt;br /&gt;
2004, Turin, IAU Colloquium no. 195, “Outskirts of galaxy clusters: intense life in the suburbs”&lt;br /&gt;
Tornatore, L., Borgani, S., Recchi, S., Matteucci, F.&lt;br /&gt;
&lt;br /&gt;
ICM Chemodynamics in numerical simulations&lt;br /&gt;
2003, Vulcano, Chemical Enrichment of the ICM and IGM&lt;br /&gt;
Successful applications @ international facilities&lt;br /&gt;
Tornatore, L., Borgani, S., Matteucci, F.&lt;br /&gt;
&lt;br /&gt;
Simulating the effect of cooling and heating in the intra-cluster medium,&lt;br /&gt;
standard project CINECA SP4, 2002, 18000h&lt;br /&gt;
Tornatore, L., Borgani, S., Matteucci, F.&lt;br /&gt;
&lt;br /&gt;
Investiganting thermodynamics an chemistry of Galaxy Clusters, standard project CINECA SP4, 2003, 10000 h&lt;br /&gt;
Borgani, S., Diaferio, A., Dolag, K., Moscardini, L., Murante, G., Springel, Tormen, G., Tornatore, L., Tozzi, P.,&lt;br /&gt;
A Tree+SPH High-Resolution Simulation of Cosmic Web,&lt;br /&gt;
Key-Project CINECA, 2003, 50000h on IBM SP4.&lt;br /&gt;
Borgani, S., Tornatore, L.&lt;br /&gt;
&lt;br /&gt;
Simulating the chemo-thermodynamics of intra-cluster medium,&lt;br /&gt;
NERSC (National Energy Research Scientific Computing Center),&lt;br /&gt;
2004, 20000h, Seaborg facility&lt;br /&gt;
Tornatore, L., Borgani, S., Murante, G., Ling-Mei, C., Tozzi, P.&lt;br /&gt;
&lt;br /&gt;
Simulating the heating and metal enrichment of the intra-cluster medium,&lt;br /&gt;
standard project CINECA, 2004, 10000 h&lt;br /&gt;
Murante, G., Borgani, S., Chen, L.M., Diaferio, A., Dolag, K., Moscardini, L., Springel, V., Tormen, G., Tornatore, L., Tozzi, P.,&lt;br /&gt;
&lt;br /&gt;
A Tree+SPH Hih-Resolution Resimulation of a Galaxy Cluster,&lt;br /&gt;
Key-Project CINECA, 2004, 40000h on IBM SP4&lt;br /&gt;
Tornatore, L., Borgani, S., Murante, G., Ling-Mei, C., Tozzi, P.&lt;br /&gt;
&lt;br /&gt;
Simulating the heating and metal enrichment of the intra-cluster medium,&lt;br /&gt;
standard project CINECA, 2005, 7000 h&lt;br /&gt;
Tornatore, L., Dolag, K., Murante, G., Moscardini, L.&lt;br /&gt;
&lt;br /&gt;
Tree+SPH Simulations of the Chemical Enrichment of the Intra-Cluster Medium, standard project CINECA, 2006, 5000h&lt;br /&gt;
Murante, G., Borgani, S., Dolag, K., Tornatore, L., Saro, A.,&lt;br /&gt;
&lt;br /&gt;
Properties of the Galaxy Population in High-Resolution Cluster Simulations, standard project CINECA, 2006, 15000h on IBM SP5&lt;br /&gt;
Tornatore, L., Ferrara, A., Schneider R.,&lt;br /&gt;
Simulating the fading of the first stars,&lt;br /&gt;
SISSA internal project, 2006, 50000h @ CINECA&lt;br /&gt;
Borgani, S., Murante, G., Saro, A., Tornatore, L., Dola, K.,&lt;br /&gt;
Simulations of Galaxy Clusters with AGN feedback,&lt;br /&gt;
standard project CINECA, 2007, 20000h&lt;br /&gt;
Viel, M., Borgani, S., Tornatore, L.,&lt;br /&gt;
&lt;br /&gt;
The Galaxy-Intergalactic Medium Interplay,&lt;br /&gt;
key-project CINECA, 2007, 200000h&lt;br /&gt;
Ferrara, A., Tornatore, L., Schneider R.,&lt;br /&gt;
&lt;br /&gt;
Where are the first stars?,&lt;br /&gt;
SISSA internal project, 2007, 50000h @ CINECA&lt;br /&gt;
Tornatore, L., Borgani, S., Murante, G., Viel, M.,&lt;br /&gt;
&lt;br /&gt;
Simulating the impact of galactic outflows on the IGM,&lt;br /&gt;
standard project CINECA, 2008, 300000h&lt;br /&gt;
Borgani, S., Moscardini, L., Murante, L., Tornatore, L., Viel, M.,&lt;br /&gt;
&lt;br /&gt;
High-resolution simulations of the Warm-Hot Universe,&lt;br /&gt;
Key-project CINECA, 2008, 400000h&lt;br /&gt;
Valdes, M., Ferrara, A., Tornatore, L.&lt;br /&gt;
&lt;br /&gt;
Simulating the impact of DM-decay on the hydrogen temperature at very hugh redshifts,&lt;br /&gt;
SISSA intenal project, 2008, 30000h @ CINECA&lt;br /&gt;
Viel, M., Borgani, S., Tornatore, L.,&lt;br /&gt;
&lt;br /&gt;
The Galaxy-Intergalactic Medium Interplay and the role of galactic winds at z~2-4,&lt;br /&gt;
standard project CINECA, 2009, 50000h&lt;br /&gt;
Fabjan, D., Borgani, S., Dolag, K., Murante, G., Tornatore, L.,&lt;br /&gt;
&lt;br /&gt;
Simulations of feedback effects on the properties of galaxy clusters,&lt;br /&gt;
standard project CINECA, 2009, 50000h&lt;/div&gt;</summary>
		<author><name>82.48.76.161</name></author>
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