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Stefano Bovino

Associate Professor

Universidad de Concepción

Concepción, Chile

Líneas de Investigación


Astrochemistry, Computational Astrophysics, Laboratory Astrochemistry, Star formation, Galaxy formation and evolution, Quantum Chemistry, Physics of the Interstellar Medium

Educación

  •  PhD in Theoretical Chemistry, Sapienza University of Rome. Italia, 2011
  •  M.Sc. in Theoretical Chemistry, Sapienza University of Rome. Italia, 2008
  •  B.Sc. in Computational Chemistry, Sapienza University of Rome. Italia, 2005

Experiencia Académica

  •   DFG Postdoctoral Fellow Full Time

    Hamburg University

    Physics

    Hamburg, Alemania

    2015 - 2017

  •   Postdoc Full Time

    Göttingen University

    Physics

    Göttingen, Alemania

    2012 - 2015

  •   ISCRA Postdoc Fellow Full Time

    Sapienza University of Rome/CINECA

    Chemistry

    Rome, Italia

    2011 - 2012

  •   Short Term Scholar Full Time

    Harvard University

    Cambridge, Estados Unidos

    2008 - 2008

Experiencia Profesional

  •   Short-term scholar Full Time

    Harvard University

    Estados Unidos

    2008 - 2008

  •   ISCRA Postdoctoral Fellow Full Time

    Sapienza University of Rome

    Italia

    2011 - 2012

  •   Postdoc Full Time

    Göttingen University

    Alemania

    2012 - 2015

  •   DFG Postdoctoral Fellow Full Time

    Hamburg University

    Alemania

    2015 - 2017

  •   Associate Professor Full Time

    Universidad de Concepcion

    Chile

    2017 - At present

Premios y Distinciones

  •   Carla Roetti Medal

    Italian Chemical Society

    Italia, 2015

    Motivation: for his original contribution to the application of theoretical and computational chemistry methods to the astrophysics

  •   SAO Visiting Student Award

    Harvard Smithsonian Center for Astrophysics

    Estados Unidos, 2009

    Institute for Theoretical Atomic, Molecular, and Optical Physics (ITAMP), Harvard-Smithsonian Center for Astrophysics, Cambridge, USA. To work with Prof. Dalgarno on energy transfer processes relevant for planetary atmospheres evolution.

  •   SAO Visiting Student Award

    Harvard Smithsonian Center for Astrophysics

    Estados Unidos, 2010

    Institute for Theoretical Atomic, Molecular, and Optical Physics (ITAMP), Harvard-Smithsonian Center for Astrophysics, Cambridge, USA. To work with Prof. Dalgarno and Prof. Karchenko on energy transfer processes relevant for planetary atmospheres evolution.


 

Article (69)

Chemical analysis of prestellar cores in Ophiuchus yields short timescales and rapid collapse
Chemical post-processing of magneto-hydrodynamical simulations of star-forming regions: robustness and pitfalls
Establishing the evolutionary timescales of the massive star formation process through chemistry,
Identification of prestellar cores in high-mass star forming clumps via H2D+ observations with ALMA
On the low ortho-to-para H2 ratio in star-forming filaments
Presence of water on exomoons orbiting free-floating planets: a case study,
A new proxy to estimate the cosmic ray ionization rate in dense cores
A novel framework for studying the impact of binding energy distributions on the chemistry of dust grains
High level ab initio binding energy distribution of molecules on interstellar ices: Hydrogen fluoride
Predicting FIR lines from simulated galaxies
Survey of ortho-H2D+ in high-mass star-forming regions
The [C II]-SFR correlation in dwarf galaxies across cosmic time
The [CII]-SFR correlation in dwarf galaxies across cosmic time
A timeline for massive star-forming regions via combined observation of o-H2D+ and N2D+
Black hole formation in the context of dissipative dark matter
First molecule still animates astronomers
High-redshift quasars and their host galaxies - I. Kinematical and dynamical properties and their tracers
On the size of the CO-depletion radius in the IRDC G351.77-0.51
The 3D Structure of CO Depletion in High-mass Prestellar Regions
Fast deuterium fractionation in magnetized and turbulent filaments
Massive black holes from dissipative dark matter
The effect of non-equilibrium metal cooling on the interstellar medium
The formation of protostellar binaries in primordial minihaloes
The natural emergence of the correlation between H-2 and star formation rate surface densities in galaxy simulations
A detailed framework to incorporate dust in hydrodynamical simulations
Deuterium fractionation and H2D+ evolution in turbulent and magnetized cloud cores
H-2 Ortho-to-para Conversion on Grains: A Route to Fast Deuterium Fractionation in Dense Cloud Cores?
The impact of chemistry on the structure of high-z galaxies
A chemical model for the interstellar medium in galaxies
The chemical evolution of self-gravitating primordial disks
THE FORMATION OF THE PRIMITIVE STAR SDSS J102915+172927: EFFECT OF THE DUST MASS AND THE GRAIN-SIZE DISTRIBUTION
CH + Destruction by Reaction with H: Computing Quantum Rates To Model Different Molecular Regions in the Interstellar Medium
How realistic UV spectra and X-rays suppress the abundance of direct collapse black holes
Saturation of the turbulent dynamo
A UV flux constraint on the formation of direct collapse black holes
Dark-matter halo mergers as a fertile environment for low-mass Population III star formation
Effects of turbulence and rotation on protostar formation as a precursor of massive black holes
FORMATION OF CARBON-ENHANCED METAL-POOR STARS IN THE PRESENCE OF FAR-ULTRAVIOLET RADIATION
KROME - a package to embed chemistry in astrophysical simulations
Primordial star formation: relative impact of H-2 three-body rates and initial conditions
THE FORMATION OF MASSIVE PRIMORDIAL STARS IN THE PRESENCE OF MODERATE UV BACKGROUNDS
THE TURBULENT DYNAMO IN HIGHLY COMPRESSIBLE SUPERSONIC PLASMAS
Chemical complexity in astrophysical simulations: optimization and reduction techniques
Impact of an accurate modelling of primordial chemistry in high-resolution studies
Mg+(2S) and Mg+(2P) in reaction with H2(): A description of the energy surfaces explaining the mechanisms
The small-scale dynamo: breaking universality at high Mach numbers
Turbulent magnetic field amplification from the smallest to the largest magnetic Prandtl numbers
Chemical destruction of rotationally ?hot? HeH+: Quantum cross sections and mechanisms of its reaction with H
Complexity reduction of astrochemical networks
Direct and inverse reactions of LiH + with He( 1 S) from quantum calculations: mechanisms and rates
LiHe + IN THE EARLY UNIVERSE: A FULL ASSESSMENT OF ITS REACTION NETWORK AND FINAL ABUNDANCES
Small-scale dynamo at low magnetic Prandtl numbers
Cold Chemistry with Ionic Partners: Quantum Features of HeH + ( 1 ?) with H( 1 S) at Ultralow Energies
Energy transfer in O collisions with He isotopes and Helium escape from Mars
Ion chemistry in the early universe
LiH destruction by protons: a comparison of quantum models for an important astrochemical process
ON THE RELATIVE ABUNDANCE OF LiH AND LiH + MOLECULES IN THE EARLY UNIVERSE: NEW RESULTS FROM QUANTUM REACTIONS
PHOTON-INDUCED EVOLUTIONARY RATES OF LiHe + ( 1 Σ + ) IN EARLY UNIVERSE FROM ACCURATE QUANTUM COMPUTATIONS
Quenching vibrations of cesium dimers by He at low and ultralow temperatures: quantum dynamical calculations
Relaxation of energetic S( 1 D) atoms in Xe gas: Comparison of ab initio calculations with experimental data
Testing the lithium chemistry for early universe models with a quantum reactive method
IS H + AN EFFICIENT DESTROYER OF LiH MOLECULES? A QUANTUM INVESTIGATION AT EARLY UNIVERSE CONDITIONS
THE IONIC PATHWAYS OF LITHIUM CHEMISTRY IN THE EARLY UNIVERSE: QUANTUM CALCULATIONS FOR LiH + REACTING WITH H
FAST LiH DESTRUCTION IN REACTION WITH H: QUANTUM CALCULATIONS AND ASTROPHYSICAL CONSEQUENCES
Spin-driven structural effects in alkali doped H4e clusters from quantum calculations
Trapping hydrogen atoms from a neon-gas matrix: A theoretical simulation
Ultralow-energy vibrational quenching in ionic collisions: Isotope effects in Li++D2 encounters
Vibrational cooling of spin-stretched dimer states by He buffer gas: Quantum calculations for Li2(a?u+3) at ultralow energies
Collisional quenching at ultralow energies: Controlling efficiency with internal state selection

Proyecto (6)

Millennium Nucleus on Transversal Research and Technology to explore Supermassive Black Holes
Deuteration chemistry: a tool to determine timescales during star formation
First Computational Astrochemistry Laboratory Using the Largest Shared Memory Computer in Chile
Formation and Growth of Supermasssive Black Holes
La química del deuterio como diagnostico de las condiciones físicas en regiones de formacion estelar
The low-metallicity ISM=> From high redshift to the local Universe
74
Stefano Bovino

Associate Professor

Department of Astronomy

Universidad de Concepción

Concepción, Chile

27
Dominik Schleicher

Associate Professor

Astronomia

UNIVERSIDAD DE CONCEPCION

Concepcion, Chile

2
Giovanni Sabatini

PhD student

Astronomia

Universidad de Concepción

Concepción, Chile

1
Joaquin Prieto

Investigador CATA

Astronomia

Universidad de Chile

Santiago, Chile

1
Amelia Stutz

Associate Professor

Astronomy

UNIVERSIDAD DE CONCEPCION

Concepcion, Chile