Brief CV - Darklight Cosmology

Transcript

Carmelita Carbone
Curriculum vitæ et studiorum
Personal Data
Name: Carmelita Carbone
Status: Married
Nationality: Italian
Contacts
Work address: INAF – Osservatorio Astronomico di Brera
via Emilio Bianchi 46, I - 23807 Merate (LC), Italia.
Telephone: +39-02-723-204-55
Fax: +39-02-723-204-01
e-mail: [email protected]
Education
♦ October 2007: PhD at SISSA/ISAS, Trieste.
Title of PhD thesis: “Non-linear structure formation and cosmic radiation backgrounds”.
Supervisors: Prof. Carlo Baccigalupi (SISSA/ISAS, Trieste) and Prof. Sabino Matarrese
(University of Padova)
♦ July 2003: Degree in Physics at University of Padova with a mark of 110/110 cum laude.
Title of degree thesis: “Gravitational waves on large scales in the presence of Dark Matter
and Cosmological Constant”.
Supervisor: Prof. Sabino Matarrese (University of Padova)
Research Impact
H-index: 15.
36 publications with about 1573 citations (157 total normalised citations).
26 refereed publications with about 937 citations (154 total normalised citations).
13 first-author refereed publications with about 324 citations (102 total normalised citations).
Two famous papers (250+ citations).
Two very well-known papers (100+ citations), one of which with first-authorship.
http://adsabs.harvard.edu/cgi-bin/nph-abs connect?library&libname=Carmelita+Carbone+papers&libid=524848a566
C. Carbone, Curriculum Vitæ
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Awarded Research Activities
Awarded by the National ISCRA evaluation procedure as Principal Investigator of
• The class–A proposal entitled “The Dark-Energy and Massive-Neutrino Universe”, with
assigned budget of five million cpu-hrs (equivalent to a minimum amount of 50000 Euros1 )
on the Tier-0 machine IBM/BGQ Fermi at CINECA, Italy (January 2012).
• The class–B proposal entitled “The Dark-Energy and Massive-Neutrino Universe II”, with
assigned budget of eight million cpu-hrs (equivalent to a minimum amount of 80000 Euros)
on the Tier-0 machine IBM/BGQ Fermi at CINECA, Italy (November 2015).
Refereeing Activity
I am a reviewer for
⋆ Astronomy & Astrophysics
⋆ The Astrophysical Journal
⋆ Classical and Quantum Gravity
⋆ Monthly Notices of the Royal Astronomical Society
⋆ Nature Physics
⋆ Physical Review D
⋆ Physical Review Letters
⋆ Physics of the Dark Universe
⋆ Proceeding of the Royal Society A
⋆ Science
⋆ DECI/PRACE european HPC calls
⋆ ISCRA/CINECA national HPC calls
Experiment Membership
EUCLID (http://sci.esa.int/science-e/www/object/index.cfm?fobjectid=42266): this
is an M-class ESA mission within the Cosmic Vision 2015-2025 plan intended to map the geometry of the dark Universe. It combines weak gravitational lensing and baryon acoustic oscillations
measurements, and has been selected by ESA for implementation with launch planned for 2020.
The mission will investigate the distance-redshift relationship and the evolution of cosmic structures. It will achieve this goal by measuring shapes and redshifts of galaxies and clusters of
galaxies out to redshifts z ∼ 2, or equivalently up to a look-back time of 10 billion years. The
mission will therefore cover the entire period over which dark energy played a significant role in
accelerating the Universe expansion.
As member of the Euclid Consortium, I am involved in several Science Working Groups
(SWG) and Organisation Units (OU).
In particular, I am involved in
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The cost of 1 cpu-hr in Italy is between 0.01 and 0.05 Euros.
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• the CS-SWG (Cosmological simulations), in which I am lead of the Work-Packages WP1
(Initial Conditions) and co-lead of WP8 (Galaxy Clustering signal);
• the CMBX-SWG (LSS-CMB cross-correlation) in which I am co-lead of WP1 (CMB-XC
from N-body simulations);
• the IST (Inter-SWG Taskforces), in which I am co-lead of the Task-Group 3 (Galaxy
Clustering forecasts).
I am also an active member of the CS-WP4 (Lightcone generation), CS-WP9 (in which I
co-lead the sub-WP about Massive Neutrinos simulations), the GC-SWG (Galaxy Clustering),
and the CG-SWG (Clusters of Galaxies).
Professional Qualifications
∗ April 15th, 2014 – present: DARKLIGHT postdoctoral research fellow at INAF - National
Institute of Astrophysics, Astronomical Observatory of Brera, Milan/Merate, Italy
∗ June 1st, 2016: short-listed in the international competition for a permanent research
position in “Cosmology and Euclid”, at the CEA astrophysics division (Service dAstrophysique, SAp), Saclay, Paris.
∗ January 20th, 2016: qualified, at the fifth position, in the ranking list of the INAF–10RIC–
2015 national competition for researchers level-III on spectroscopic extragalactic surveys.
∗ November 13th, 2012: qualified, at the fourth position, in the ranking list of the INAF–
16RIC/MA1/OAMI–2012 national competition for researchers level-III.
∗ April 1st, 2011: recipient of a two-year fellowship within the programme “INAF POSTDOCTORAL FELLOWSHIPS 2010”, carried out at the Observatory of Bologna from
1 April 2012 to 31 January 2013, and at the Astronomy Observatory of Brera, from 1
February 2013 to 1 April 2014.
∗ December 31st, 2009: recipient of a two-year research grant for research activity on the
project “Cosmological Simulations for the ESA mission EUCLID”, which I have carried
out at the Department of Astronomy, Bologna University, from April 1st, 2010 to March
31st, 2012.
∗ March 12th, 2009: recipient of a one-year research grant for research activity on the project
“Dark-energy and cosmology with EUCLID and large galaxy surveys”, which I have carried
out at the Department of Astronomy, Bologna University, from April 1st, 2009 to March
31st, 2010.
∗ February 19th, 2009: offered a two-year IAP (France) postdoctoral position for research
activity on the project “Gravitational Lensing of the CMB: Preparation of the Planck
Mission”, declined.
∗ January 2008: recipient of a two-year postdoctoral grant within the Beatriu de Pinos 2007
programme, for research activity on the project “ Large scale structure and gravitational
wave emission”, which I have carried out at the Institut de Ciències de l’Espai (ICE –
IEEC/CSIC), Barcelona, in the period February 1st, 2008 – March 30th, 2009.
∗ February 13th, 2007: offered a two-year postdoctoral position funded by the Research
Council of Norway, for research activity on dark energy, at the Institutt for Teoretisk
Astrofysikk, Oslo University, declined.
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∗ December 15th, 2006: recipient of a two-year CSIC (Spain) research grant within the
“Dark Energy Survey” programme, for research activity on the project “Simulation and
study of the gravitational lensing effect on the cosmic radiation background”, which I have
carried out at the Institut de Ciències de l’Espai (ICE – IEEC/CSIC), Barcelona, in the
period November 1st, 2007 – January 31st, 2008.
∗ July 27th, 2006: recipient of a three-month Marie Curie grant within the EARA-EST
programme, for research activity on the project “Simulated all-sky lensed maps via the
Millennium Simulation”, which I have carried out at the Max-Planck-Institut für Astrophysik, Garching (Germany), under the supervision of Dr. Volker Springel, in the period
October 1st – December 31st, 2006.
∗ July 31st, 2003: recipient of a four-month grant within the PRIN 2002 programme, for
research activity on the project “Non-linear dynamics of Dark Matter and Dark Energy”,
which I have carried at the Physics Department, Padova University, under the supervision
of Prof. Sabino Matarrese, in the period September 1st – October 31st, 2003.
Visits to non-Italian scientific institutions
◦ October – December 2006: three-month Marie Curie grant within the EARA-EST programme, for research activity on the project “Simulated all-sky lensed maps via the Millennium Simulation”, which I have carried out at the Max-Planck-Institut für Astrophysik,
Garching (Germany), under the supervision of Dr. Volker Springel.
◦ July – September 2006: Three-month visit at the Max-Planck-Institut für Astrophysik,
Garching (Germany), for scientific collaboration with Dr. Volker Springel.
◦ March – April 2006: Two-month visit at the Max-Planck-Institut für Astrophysik, Garching (Germany), for scientific collaboration with Dr. Volker Springel.
◦ November 17th – December 17th, 2005: One-month visit at the Institut für Theoretische
Astrophysik (ITA), Heidelberg, hosted by Prof. Carlo Baccigalupi and Prof. Matthias
Bartelmann.
Student Supervision
• In collaboration with Prof. Lauro Moscardini, I have supervised the Master Degree thesis
of Camilla Penzo entitled “Cosmological models with scalar fields kinetically coupled to the
Einstein tensor”. She graduated in Astronomy at the Alma Mater Studiorium, University
of Bologna, on March 18th, 2011, with a mark of 109/110. She has been a PhD student
at the Max Planck Institute for Astronomy in Heidelberg, Germany, working in the group
led by Andrea Macciò, and is currently a postdoctoral researcher at the Observatoire de
Paris, Meudon.
• In collaboration with Prof. Moscardini and Dr. Federico Marulli, I have supervised the
Master Degree thesis of Linda Blot, concerning the effect of massive neutrinos on the
alignment profile of satellite galaxies in clusters. She graduated in Astronomy at the Alma
Mater Studiorium, University of Bologna, on July 20th, 2012, with a mark of 110/110. She
has been a PhD student in the COS group at LUTh (France) under the supervision of prof.
Pierstefano Corasaniti, and is currently a postdoc researcher at IEEC-UAB, Barcelona,
Spain.
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• In collaboration with Prof. Carlo Baccigalupi, I have supervised the PhD thesis of Matteo
Calabrese (SISSA, Trieste), entitled “The Universe in many nutshells: high resolution
simulations of CMB weak gravitational lensing ”. He is currently a fellow at Observatory
of Aosta Valley, Italy.
• In collaboration with Prof. Luigi Guzzo and Dr. Julien Bel, I have supervised the Master
Degree thesis of Matteo Zennaro entitled “Constraining neutrino mass from clustering
measurements at high redshift”. He graduated at Bicocca University in Milan, at the end of
October 2014, with a mark of 110/110 cum laude. He is currently a PhD student in Physics,
Astrophysics and Applied Physics at the University of Milan, under the supervision of Prof.
Davide Maino, Dr. Julien Bel and myself.
• In collaboration with Prof. Luigi Guzzo and Dr. Emiliano Sefusatti, I have supervised
the Master Degree thesis of Chiara Moretti entitled “Testing Non Linear Models for the
Galaxy Power Spectrum in Cosmologies with Massive Neutrinos”. She graduated at Bicocca University in Milan, at the end of June 2016 with a mark of 110/110.
Scientific Interests
⋆ Physics of the Early Universe, in particular:
– Cosmological perturbations
– Primordial non-Gaussianity
– Isocurvature initial conditions
⋆ Cosmic Microwave Background (CMB), in particular:
– Total intensity and polarisation anisotropies
– CMB weak gravitational lensing in different cosmologies from N-body simulation
data.
– ISW/Rees-Sciama effect with massive neutrinos from N-body simulation data.
– Massive neutrino effects on Sunyaev-Zeldovich and X-ray observables
⋆ Galaxy surveys, in particular:
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Baryon Acoustic Oscillations (BAOs)
Dark Energy and Dark Matter
Cosmological parameter measurements
Neutrino constraints
Redshift space distortions
⋆ Cosmological structure formation, in particular:
– Linear and non-linear regimes
– Large cosmological N-body simulations with dark-energy and massive neutrinos
– Gravitational waves from strongly non-linear structure evolution
⋆ Statistical Techniques for Data Analysis in Cosmology, in particular:
– Fisher Matrix analysis applied to galaxy/cluster clustering and CMB data
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Other
◦ Computational expertise: Fortran, IDL, C, HPC.
◦ Languages: Italian (native), English (fluent), Spanish (good)
Contributions to conferences and meetings
∗ Invited talk on “Clustering and lensing from the DEMNUni neutrino simulations”, Theoretical challenges for precision galaxy clustering, 11-15 July 2016, Sexten Center for
Astrophysics, Italy (declined).
∗ Invited talk on “Clustering and lensing from the DEMNUni neutrino simulations”, BAO
& RSD: Dark Light on Obscure Acronyms, 05-09 July 2016, Sexten Center for Astrophysics, Italy (declined).
∗ Talk on “Clustering and weak-lensing in the presence of massive neutrinos”, CS-SWG
splinter, Euclid Consortium Meeting, May 31–June 3 2016, Lisbon, Portugal.
∗ Invited talk on “Clustering, lensing and ISW-RS from very large simulations with massive
neutrinos”, Nonlinear Large Scale Structure: Theory Meets Expectations, 24-26 May 2016,
IAP, Paris
∗ Invited talk on “Clustering, lensing and ISW-RS from the DEMNUni neutrino simulations”, 28th Texas Symposium on Relativistic Astrophysics, 13-18 December 2015, Geneva
∗ Invited talk on “Lensing and ISW/RS from the DEMNUni simulations”, From Inflation
to Galaxies: a workshop in honor of Sabino Matarrese, 31 August–3 September, 2015,
Castiglioncello, Italy (declined)
∗ Invited talk on “Lensing and ISW/RS from the DEMNUni simulations”, CMBX-SWG
splinter, Euclid Consortium Meeting, 8–12 June 2015, Lausanne, Switzerland.
∗ Talk on “Photometric Clustering in Euclid-GCSWG”, GC-SWG splinter, Euclid Consortium Meeting, 8–12 June 2015, Lausanne, Switzerland.
∗ Invited talk on “Clustering, lensing and ISW/RS effects from the DEMNUni simulations”, Advanced Workshop on Cosmological Structures from Reionization to Galaxies:
Combining Efforts from Analytical and Numerical Methods, ICTP, 12–15 May 2015, Trieste, Italy.
∗ Invited talk on “CMB-lensing and ISW/RS effects from the largest cosmological simulations with massive neutrinos”, 100th National Congress of the Italian Physics Society,
22–26 September 2014, Pisa, Italy.
∗ Invited talk on “LSS, lensing, ISW/RS and respective cross-correlations from the largest
cosmological simulations with massive neutrino particles”, Cosmology after Planck, 25
Aug.–19 Sept. 2014, MIAPP, Garching bei Muenchen, Germany.
∗ Invited talk on “LSS from the Dark Energy & Massive Neutrino Universe simulations”,
Measuring and Modelling RSD in Galaxy Surveys, 21–25 July 2014, Sexten CfA, Italy.
∗ Talk on “Lensing and ISW/RS from the DEMNUni simulations”, Cross-correlations in the
high-redshift sky, UCL, 18–20 June 2014 , London, UK.
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∗ Talk on “The Dark Energy and Massive Neutrino Universe simulations”, CS-SWG splinter,
Euclid Consortium Meeting, 5 May, 2014, Marseille, France.
∗ Invited talk on “Neutrino constraints from future surveys”, Darklight Project Meeting,
17–19 June 2013, Varenna, Italy.
∗ Talk on “Neutrino constraints from the Euclid galaxy-clustering“, Euclid GC-SWG splinter, Euclid Consortium meeting, 14 May 2013, Leiden, The Netherlands.
∗ Talk on “CMB deflection maps from N-body simulations in Coupled Dark Energy cosmologies“, CMBX-SWG splinter, Euclid Consortium meeting, 13 May 2013, Leiden, The
Netherlands.
∗ Invited talk on “CMB lensing and N-body simulations”, Big Bang, Big Data, Big Computers, 19–21 September 2012, AstroParticule et Cosmologie (APC) Laboratory, Paris,
France.
∗ Invited talk on “Neutrino mass from cosmological observations: galaxy-clustering”, Neutrino Oscillation Workshop, 9–16 September 2012, Conca Specchiulla (Otranto, Lecce),
Italy.
∗ Invited talk on “Isocurvature perturbations with Euclid”, TH-SWG splinter, Euclid Consortium meeting, 17 May 2012, Copenhagen, Denmark.
∗ Invited talk on “CMB lensing in N-body simulations”, CMBX-SWG splinter, Euclid
Consortium meeting, 14 May 2012, Copenhagen, Denmark.
∗ Talk on “Lensed CMB from the Millennium Simulation”, Planck Joint Core Team meeting,
30 April 2009, LAL (Orsay), France.
∗ Talk on “The properties of the dark matter halo distribution in non-Gaussian scenarios”,
Dark Matter conference, Galileo Galilei Institute for Theoretical Physics, February 2009,
Arcetri, Florence, Italy.
∗ Talk on “Lensed CMB from the Millennium Simulation”, New Horizons for Modern Cosmology workshop, Galileo Galilei Institute for Theoretical Physics, February 2009, Arcetri,
Florence, Italy.
∗ Talk on “Lensed B-modes from N-body simulations”, Planck Technical Working Group 5
meeting, May 2008, Paris, France.
∗ Poster on “All-sky lensed CMB maps via the via the Millennium Simulation”, Planck
Consortium meeting 2007, June 2007, Toulouse, France.
∗ Talk on “Simulating CMB lensing with the Millennium Run”, Gravitational Lensing Workshop, August 2006, Leiden, The Netherlands.
∗ Poster on “The stochastic gravitational-wave background from cold dark matter halos”,
International Astrophysics Conference, “Relativistic Astrophysics and Cosmology - Einstein’s Legacy -”, November 2005, Munich, Germany.
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Scientific seminars
♦ Invited talk on “The effect of massive neutrinos on the large scale structure of the Universe”, to be held on 9 December 2016 at CERN, Geneve.
♦ Talk on “Clustering, lensing and ISW-RS from the neutrino DEMNUni simulations”, 19
May 2016, CEA, Saclay.
♦ Seminar on “Lensing and ISW/RS from the DEMNUni simulations”, LSS-CMB workshop,
23 September 2015, Merate, Italy.
♦ Seminar on “Clustering, lensing and ISW/RS effects from the DEMNUni simulations”,
May 14th 2015, SISSA/ISAS, Trieste.
♦ Seminar on “The BICEP2 results on primordial gravitational waves”, April 10th 2014,
Astronomical Observatory of Brera, Merate (LC), Italy
♦ Seminar on “Baryon acoustic oscillations in different cosmologies”, Department of Astronomy, University of Bologna, February 2012.
♦ Seminar on “The properties of the dark matter halo distribution in non-Gaussian scenarios”, Department of Astronomy, University of Bologna, May 2009
♦ Seminar on “All-sky lensed CMB maps via the via the Millennium Simulation”, Physics
Department, Milano University, November 2008
♦ Seminar on “Non-linear structure formation and cosmic radiation backgrounds”, ICE,
Barcelona, November 2007
♦ Seminar on “All-sky lensed CMB maps via N-body simulations”, ICE, Barcelona, December 2006
♦ Seminar on “All-sky lensed CMB maps via N-body simulations”, Astrophysics Department, Oxford University, Oxford, January 2007
♦ Seminar on “Cosmological perturbations and stochastic gravitational-wave background
from dark matter halos”, ITA, Heidelberg, December 2005
♦ Seminar on “Gravitational waves from dark matter halos”, SISSA, Trieste, May 2005
♦ Seminar on “Cosmic microwave fluctuations from gravitational-waves”, SISSA, Trieste,
February 2005
Popular conferences
• Talk on “L’inflazione cosmologica: modelli a confronto”, “L’universo in fiore” lectures,
INAF–Astronomical Observatory of Brera, April 1st 2015 and February 3rd 2016, Milan,
Italy
• Talk on “L’Universo primordiale”, SISSA Open-Day, September 2004, Trieste, Italy
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Participation to other meetings and schools
· Euclid Consortium Meeting, 31 May – 3 June 2016, Lisbon, Portugal.
· Euclid Cosmological-Simulations SWG Meeting, 18–19 November 2015, Barcelona, Spain.
· Euclid Galaxy-Clustering SWG Meeting, 18–19 February 2015, London, UK.
· Joint Euclid Theory and Simulations SWG meeting, 12–13 January 2015, Oslo, Norway.
· Euclid Cosmological Simulations SWG Meeting, 4–5 December 2014, Barcelona, Spain.
· Prospects in Neutrino Physiscs, 19–20 December 2013, London, UK.
· Euclid OU-LE3 meeting, 17–19 December 2013, Nice, France.
· Workshop “Origin of cosmic structures : numerical and theoretical approaches”, 25–29
November, 2013, Paris, France.
· Euclid National Day, 8 November 2013, Italy.
· Pontecorvo100 - Symposium in honour of Bruno Pontecorvo for the centennial of the birth,
18–20 September 2013, Pisa, Italy.
· Synergistic Science with Euclid and the Square Kilometre Array, 16–18 September 2013,
Oxford, UK.
· Cosmo Probes 2013, 24–26 June 2013, Lausanne, Switzerland.
· Euclid Mission Consortium meeting, 15–16 May 2012, Copenhagen, Denmark
· The Dark Universe Conference, 4–7 October 2011, Heidelberg, Germany.
· The Euclid Mission Meeting, 7-8 September 2011, Bologna, Italy.
· Joint Euclid Meeting for all the Euclid Science Working Groups, 24–25 January 2011,
Garching bei Muenchen, Munich, Germany.
· Euclid Consortium Meeting, IAP, 25–26 May 2010, Paris, France.
· “Observing the Dark Universe with Euclid”, 17–18 November 2009, Space Expo Noordwijk,
The Netherlands.
· BPol Workshop, 25–27 October 2006, Orsay-Paris, France.
· Conference on Computational Cosmology, International Center for Theoretical Physics
(ICTP), , June 2005, Trieste, Italy.
· National School of Astrophysics, September 2004, Asiago (VI), Italy.
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Publications
1. Carbone, Carmelita; Petkova, Margarita; Dolag, Klaus, “DEMNUni: ISW, Rees-Sciama,
and weak-lensing in the presence of massive neutrinos”, Journal of Cosmology and Astroparticle Physics, Issue 07, article id. 034 (2016).
http://iopscience.iop.org/article/10.1088/1475-7516/2016/07/034/pdf
2. Amendola et al 2016, “Cosmology and Fundamental Physics with the Euclid Satellite”,
eprint arXiv:1606.00180
http://arxiv.org/abs/1606.00180
3. Zennaro, Matteo; Bel, Julien; Villaescusa-Navarro, Francisco; Carbone, Carmelita; Sefusatti, Emiliano; Guzzo, Luigi, “Initial Conditions for Accurate N-Body Simulations of
Massive Neutrino Cosmologies”, eprint arXiv:1605.05283
4. Petracca, Fernanda; Marulli, Federico; Moscardini, Lauro; Cimatti, Andrea; Carbone,
Carmelita; Angulo, Raul E., “Forecasts on neutrino mass constraints from the redshiftspace two-point correlation function”, MNRAS accepted, eprint arXiv:1512.06139.
http://adsabs.harvard.edu/abs/2015arXiv151206139P
5. Castorina, Emanuele; Carbone, Carmelita; Bel, Julien; Sefusatti, Emiliano; Dolag,
Klaus, “DEMNUni: The clustering of large-scale structures in the presence of massive
neutrinos”, Journal of Cosmology and Astroparticle Physics, Issue 07, article id. 043,
(2015).
http://adsabs.harvard.edu/abs/2015JCAP...07..043C
6. Wolk, M.; Szapudi, I.; Bel, J.; Carbone, C.; Carron, J.,“Improving constraints on the
neutrino mass using sufficient statistics”, eprint arXiv:1504.00069.
7. Calabrese, Matteo; Carbone, Carmelita; Fabbian Giulio; Baldi Marco; Baccigalupi,
Carlo, “Multiple Lensing of the Cosmic Microwave Background anisotropies”, Journal of
Cosmology and Astroparticle Physics, Issue 03, article id. 049, pp. (2015).
http://iopscience.iop.org/1475-7516/2015/03/049/
8. Camera, Stefano; Carbone, Carmelita; Fedeli, Cosimo; Moscardini, Lauro, “Neglecting
Primordial non-Gaussianity Threatens Future Cosmological Experiment Accuracy”, Physical Review D, Volume 91, Issue 4, id.043533 (2015).
http://journals.aps.org/prd/abstract/10.1103/PhysRevD.91.043533
9. Roncarelli, Mauro; Carbone, Carmelita; Moscardini, Lauro, “The effect of massive
neutrinos on the SZ and X-ray observables of galaxy clusters”, Monthly Notices of the
Royal Astronomical Society, Volume 447, Issue 2, p.1761-1773.
http://mnras.oxfordjournals.org/content/447/2/1761
10. Antolini, Claudia; Fantaye, Yabebal; Martinelli, Matteo; Carbone, Carmelita; Baccigalupi, Carlo, “N-body lensed CMB maps: lensing extraction and characterization”,
Journal of Cosmology and Astroparticle Physics, Issue 02, article id. 039, pp. (2014).
11. Carbone, Carmelita; Baldi, Marco; Pettorino, Valeria; Baccigalupi, Carlo, “Maps of
CMB lensing deflection from N-body simulations in Coupled Dark Energy Cosmologies”,
Journal of Cosmology and Astroparticle Physics, Issue 09, article id. 004, pp. (2013).
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12. Luca Amendola, Stephen Appleby, David Bacon, Tessa Baker, Marco Baldi, Nicola Bartolo, Alain Blanchard, Camille Bonvin, Stefano Borgani, Enzo Branchini, Clare Burrage,
Stefano Camera, Carmelita Carbone, Luciano Casarini, Mark Cropper, Claudia deRham, Cinzia di Porto, Anne Ealet, Pedro G. Ferreira, Fabio Finelli, Juan Garcia-Bellido,
Tommaso Giannantonio, Luigi Guzzo, Alan Heavens, Lavinia Heisenberg, Catherine Heymans, Henk Hoekstra, Lukas Hollenstein, Rory Holmes, Ole Horst, Knud Jahnke, Thomas
D. Kitching, Tomi Koivisto, Martin Kunz, Giuseppe La Vacca, Marisa March, Elisabetta
Majerotto, Katarina Markovic, David Marsh, Federico Marulli, Richard Massey, Yannick
Mellier, David F. Mota, Nelson Nunes, Will Percival, Valeria Pettorino, Cristiano Porciani,
Claudia Quercellini, Justin Read, Massimiliano Rinaldi, et al., “Cosmology and fundamental physics with the Euclid satellite”, Living Reviews in Relativity, vol. 16, no. 6 (2013).
http://adsabs.harvard.edu/cgi-bin/bib query?arXiv:1206.1225
13. Elisabetta Majerotto, Luigi Guzzo, Lado Samushia, Will J. Percival, Yun Wang, Sylvain de
la Torre, Bianca Garilli, Paolo Franzetti, Emanuel Rossetti, Andrea Cimatti, Carmelita
Carbone, Nathan Roche, Giovanni Zamorani, “Probing deviations from General Relativity with the Euclid spectroscopic survey”, Mon. Not. R. Astron. Soc. 424, 1392-1408
(2012).
http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2012.21323.x/pdf
14. Stefano Camera, Carmelita Carbone, Lauro Moscardini, “Inclusive constraints on unified dark matter models from future large-scale surveys”, Journal of Cosmology and Astroparticle Physics, Issue 03, pp. 039 (2012).
15. Carmelita Carbone, Cosimo Fedeli, Lauro Moscardini, Andrea Cimatti, “Measuring
the neutrino mass from future wide galaxy cluster catalogues”, Journal of Cosmology and
Astroparticle Physics, Issue 03, pp. 023 (2012).
16. R. Laureijs, J. Amiaux, S. Arduini, J.-L. Augures, J. Brinchmann, R. Cole, M. Cropper,
C. Dabin, L. Duvet, A. Ealet, B. Garilli, P. Gondoin, L. Guzzo, J. Hoar, H. Hoekstra,
R. Holmes, T. Kitching, T. Maciaszek, Y. Mellier, F. Pasian, W. Percival, J. Rhodes,
G. Saavedra Criado, M. Sauvage, R. Scaramella, L. Valenziano, S. Warren, R. Bender,
F. Castander, A. Cimatti, O. Le Fvre, H. Kurki-Suonio, M. Levi, P. Lilje, G. Meylan, R.
Nichol, K. Pedersen, V. Popa, R. Rebolo Lopez, H.-W. Rix, H. Rottgering, W. Zeilinger, F.
Grupp, P. Hudelot, R. Massey, M. Meneghetti, L. Miller, S. Paltani, S. Paulin-Henriksson,
S. Pires, C. Saxton, T. Schrabback, G. Seidel, J. Walsh, N. Aghanim, L. Amendola, J.
Bartlett, C. Baccigalupi, J.-P. Beaulieu, K. Benabed, J.-G. Cuby, D. Elbaz, P. Fosalba, G.
Gavazzi, et al., “Euclid Definition Study Report”.
17. Federico Marulli, Carmelita Carbone, Matteo Viel, Lauro Moscardini, Andrea Cimatti,
“Effects of massive neutrinos on the large-scale structure of the Universe”, Mon. Not. R.
Astron. Soc. 418, 346-356 (2011).
http://adsabs.harvard.edu/abs/2011MNRAS.418..346M
18. Carmelita Carbone, Anna Mangilli, Licia Verde,“Isocurvature modes and Baryon Acoustic Oscillations II: gains from combining CMB and Large Scale Structure”, Journal of
Cosmology and Astroparticle Physics, Issue 09, pp. 028 (2011).
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19. Carmelita Carbone, Licia Verde, Yun Wang, Andrea Cimatti, “Neutrino constraints
from future nearly all-sky spectroscopic galaxy surveys”, Journal of Cosmology and Astroparticle Physics, Issue 03, pp. 030 (2011).
20. Cosimo Fedeli, Carmelita Carbone, Lauro Moscardini, Andrea Cimatti, “The clustering
of galaxies and galaxy clusters: constraints on primordial non-Gaussianity from future
wide-field surveys”, Mon. Not. R. Astron. Soc. 414, 1545-1559 (2011).
http://adsabs.harvard.edu/abs/2011MNRAS.414.1545F
21. Y. Wang, W. Percival, A. Cimatti, P. Mukherjee, L. Guzzo, C. M. Baugh, C. Carbone,
P. Franzetti, B. Garilli, J. E. Geach, C. G. Lacey, E. Majerotto, A. Orsi, P. Rosati, L.
Samushia, G. Zamorani, “Designing a space-based galaxy redshift survey to probe dark
energy”, Mon. Not. R. Astron. Soc. 409, 737-749 (2010).
http://adsabs.harvard.edu/abs/2010MNRAS.409..737W
22. Carmelita Carbone, Olga Mena, Licia Verde, “Cosmological Parameters Degeneracies
and Non-Gaussian Halo Bias”, Journal of Cosmology and Astroparticle Physics, Issue 07,
pp. 020 (2010).
23. James Aguirre, Alexandre Amblard, Amjad Ashoorioon, Carlo Baccigalupi, Amedeo Balbi,
James Bartlett, Nicola Bartolo, Dominic Benford, Mark Birkinshaw, Jamie Bock, Dick
Bond, Julian Borrill, Franois Bouchet, Michael Bridges, Emory Bunn, Erminia Calabrese,
Christopher Cantalupo, Ana Caramete, Carmelita Carbone, Suchetana Chatterjee,
Sarah Church, David Chuss, Carlo Contaldi, Asantha Cooray, Sudeep Das, Francesco
De Bernardis, Paolo De Bernardis, Gianfranco De Zotti, Jacques Delabrouille, F.-Xavier
Dsert, Mark Devlin, Clive Dickinson, Simon Dicker, Matt Dobbs, Scott Dodelson, Olivier
Dore, Jessie Dotson, Joanna Dunkley, Maria Cristina Falvella, Dale Fixsen, Pablo Fosalba,
Joseph Fowler, Evalyn Gates, Walter Gear, Sunil Golwala, Krzysztof Gorski, Alessandro
Gruppuso, Josh Gundersen, Mark Halpern, et al., “Observing the Evolution of the Universe”.
24. S. Dodelson, R. Easther, S. Hanany, L. McAllister, S. Meyer, L. Page, P. Ade, A. Amblard,
A. Ashoorioon, C. Baccigalupi, A. Balbi, J. Bartlett, N. Bartolo, D. Baumann, M. Beltran,
D. Benford, M. Birkinshaw, J. Bock, D. Bond, J. Borrill, F. Bouchet, M. Bridges, E. Bunn,
E. Calabrese, C. Cantalupo, A. Caramete, C. Carbone, S. Carroll, S. Chatterjee, X. Chen,
S. Church, D. Chuss, C. Contaldi, A. Cooray, P. Creminelli, S. Das, F. De Bernardis, P. de
Bernardis, J. Delabrouille, F.-X. Desert, M. Devlin, C. Dickinson, S. Dicker, M. DiPirro,
M. Dobbs, O. Dore, J. Dotson, J. Dunkley, C. Dvorkin, H. K. Eriksen, M. Cristina Falvella,
D. Finley, D. Finkbeiner, D. Fixsen, R. Flauger, P. Fosalba, J. Fowler, S. Galli, E. Gates,
W. Gear, Y. Giraud-Heraud, K. Gorski, B. Greene, A. Gruppuso, et al., “The Origin of the
Universe as Revealed Through the Polarization of the Cosmic Microwave Background”.
25. C. Carbone, E. Branchini, K. Dolag, M. Grossi, F. Iannuzzi, S. Matarrese, L. Moscardini,
L. Verde, “The properties of the dark matter halo distribution in non-Gaussian scenarios”,
Nuclear Physics B Proceedings Supplements, Volume 194, p. 22 (2009).
http://adsabs.harvard.edu/abs/2009NuPhS.194...22C
26. M. Grossi, L. Verde,C. Carbone, K. Dolag, E. Branchini, F. Iannuzzi, S. Matarrese,
L. Moscardini, “Large-scale non-Gaussian mass function and halo bias: tests on N-body
13
simulations”, Mon. Not. R. Astron. Soc. 398, 321-332 (2009).
http://adsabs.harvard.edu/abs/2009MNRAS.398..321G
27. Carmelita Carbone, Carlo Baccigalupi, Matthias Bartelmann, Sabino Matarrese and
Volker Springel, “Lensed CMB temperature and polarization maps from the Millennium
Simulation”, Mon. Not. R. Astron. Soc. 396, 668-679 (2009).
http://adsabs.harvard.edu/abs/2009MNRAS.396..668C
28. Carmelita Carbone, Licia Verde, Sabino Matarrese, “Non-Gaussian halo bias and future
galaxy surveys”, The Astrophysical Journal, 684, L1-L4 (2008).
http://adsabs.harvard.edu/abs/2008ApJ...684L...1C
29. Carmelita Carbone, Volker Springel, Carlo Baccigalupi, Matthias Bartelmann, Sabino
Matarrese, “Full-sky maps for gravitational lensing of the CMB”, Mon. Not. Roy. Astron.
Soc. 388, 1618-1626 (2008).
http://adsabs.harvard.edu/abs/2008MNRAS.388.1618C
30. Carmelita Carbone, Carlo Baccigalupi, and Sabino Matarrese, “Stochastic gravitational
wave background from cold dark matter halos”, Physical Review D 73, 063503 (2006).
http://adsabs.harvard.edu/abs/2006PhRvD..73f3503C
31. Carmelita Carbone, Sabino Matarrese, “Unified treatment of cosmological perturbations from super-horizon to small scales”, Physical Review D 71 043508 (2005)
http://adsabs.harvard.edu/abs/2005PhRvD..71d3508C
32. Carmelita Carbone, “CMB-lensing and ISW/RS effects from the largest cosmological
simulations with massive neutrinos”, Book of Abstracts, 100th National Congress of The
Italian Physics Society, September 22-26, 2014, Pisa, Italy, ISBN 978-88-7438-088-6.
http://www.sif.it/attivita/congresso/100/invito
33. Carmelita Carbone, “Neutrino mass from future large scale structure surveys”, Nuclear
Physics B (Proceedings Supplements), Volume 237, p. 50-53 (2013).
http://www.sciencedirect.com/science/article/pii/S0920563213001771
34. Carbone C.,Proceedings of “Big Bang, Big Data, Big Computers” (Big3). September
19-21, 2012. Laboratoire Astroparticule et Cosmologie, 10 rue A. Domon et L. Duquet,
75205 Paris 13, France.
http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=165
35. C. Carbone, C. Baccigalupi, S. Matarrese, “The stochastic gravitational-wave background from cold dark matter halos”, Relativistic Astrophysics Legacy and Cosmology
- Einstein’s, ESO Astrophysics Symposia, Volume . ISBN 978-3-540-74712-3. SpringerVerlag Berlin Heidelberg, 2007, p. 75 (2007)
http://adsabs.harvard.edu/abs/2007ralc.book...75C
36. PhD thesis entitled “Non-linear structure formation and cosmic radiation backgrounds”,
October 23rd, 2007.
http://www.sissa.it/ap/PhD/Theses/carbone.pdf
Referees (names and addresses)
Here below you can find the names and addresses of my potential referees.
• Prof. Carlo Baccigalupi
Scuola Internazionale Superiore di Studi Avanzati (SISSA/ISAS)
via Bonomea 265, I-34136 Trieste, Italy
phone : +39 040 3787475
fax: +39 040 3787528
• Prof. Matthias Bartelmann
Universität Heidelberg
Zentrum für Astronomie
Institut für Theoretische Astrophysik
Philosophenweg 12, D-69120 Heidelberg, Germany
phone: +49 (0) 6221 54 4817
fax: +49 (0) 6221 54 4221
• Prof. Andrea Cimatti
ALMA MATER STUDIORUM – Universitá di Bologna
Dipartimento di Fisica e Astronomia
Viale Berti Pichat 6/2, I-40126 Bologna, Italy
phone: +39 051 20 9 5817 fax: +39 051 20 9 5700
• Prof. Luigi Guzzo
INAF - Osservatorio Astronomico di Brera
Via Bianchi 46, I-23807 Merate (LC), Italy
phone.: +39 039 5971 025
fax: +39 039 5971 000
• Prof. Sabino Matarrese
Dipartimento di Fisica e Astronomia ”Galileo Galilei”
Universita’ degli Studi di Padova
via Marzolo 8, I-35131 Padova, Italy
phone : +39 049 8277120
fax: +39 049 8277112
• Prof. Licia Verde
Institute of Cosmological Sciences (ICC) UB-IEEC
Facultad de Fisica
Marti’ i Franques 1, E-08028 Barcelona, Spain
phone: +34 934031328
fax: +34 934021588
14
15
Research Interests
I am a cosmologist, interested in the theoretical interpretation of different cosmological data,
from the Cosmic Microwave Background (CMB) to Large Scale Structures (LSS), on both the
weak-lensing and galaxy-clustering sides. In particular I am interested in the analysis and
modellisation of massive neutrinos effects on different cosmological observables.
I started my cosmological studies from a very theoretical point of view, with my Master
Degree Thesis at Padua University, developing a perturbation approach, able to deal, on the
same footing, with second-order and post-Newtonian cosmological perturbations, and providing
a unified description of their evolution from the linear to the highly non-linear regime [1].
During my PhD in SISSA (Trieste), I moved to a more numerical approach, focussing on
ray-tracing studies and CMB lensing analyses, via N-body simulations such as the Millennium
Run, and producing the first all-sky maps of convergence and lensed CMB temperature and
polarisation from LSS in the fully non-linear regime [2, 3]. Recently, the same map-making
procedure has been modified by Dr. Matteo Calabrese, who I have been supervising during
his PhD, to account for multiple lens-plane effects beyond the Born approximation. This has
allowed to simulate second-order effects as the so-called antisymmetric “rotation”, but also to
detect the impact of often used approximations on very large scales, as the usual 3D→2D gradient
approximation, which produces an artificial excess of power at large angular separations. These
codes are part of the code comparison within the CS-WP4 (Lightcone generation) in Euclid.
For my first postdoc I moved to UAB, Barcelona, where I had the possibility to approach
galaxy-clustering and forecasting analyses for present and future surveys, in particular concerning massive neutrinos and primordial non-Gaussianity constraints [4, 5]. As regards primordial
non-Gaussianity, I also gave an important contribution to the correction of theoretical predictions of the halo mass function and halo bias, when compared to N-body simulation outputs.
In fact, I identified the theoretical reason for correction factors introduced ad hoc to recover
simulation measurements, i.e. the need to account for the ellipsoidal collapse model (as opposed
to spherical collapse theory) also in primordial non-Gaussian scenarios [6].
The expertise developed on cosmological parameter forecasts from galaxy-clustering data,
allowed me to become a Euclid member in the galaxy clustering Science Working Group (SWG),
and approach the fields of Baryon Acoustic Oscillations (BAO) and Redshift Space Distortions
(RSD), when I moved to Bologna for my second postdoc. I developed the so called “P (k)shape+BAO+RSD” fisher code in massive neutrino scenarios [7], whose predictions were used
in the Euclid-RedBook as forecasts on the neutrino mass from the spectroscopic Euclid survey.
Thanks to the acquired expertise, I am now co-lead of the Task-Group 3 (Galaxy Clustering
forecasts) in the IST (Inter-SWG Taskforces) of Euclid.
Working in different topics, from galaxy-clustering to CMB-lensing, at both theoretical and
numerical levels, has allowed me to gain a broad knowledge about different cosmological aspects
and probes, also in view of possible cross-correlation and probe-combination analyses.
This, together with my involvement in various Euclid SWGs, and my interest in neutrino
physics, has led me to submit HPC proposals for the production of large cosmological N-body
simulations in scenarios with massive neutrinos and evolving dark energy.
I am currently the principal investigator awarded by the Italian ISCRA/CINECA evaluation
procedure for the class-B project entitled “The Dark-Energy and Massive-Neutrino Universe
II (DEMNUni-II)” simulations, with assigned budget of eight million cpu-hours on the Tier-0
IBM-BG/Q FERMI cluster at CINECA. This proposal is the continuation of the DEMNUni
project with assigned budget of five million cpu-hours on IBM-BG/Q [8, 9], and concerns the
production of a very large set of N-body neutrino simulations, characterised by a box side size
of L = 2 Gpc/h, Npart = 2 × (2048)3 , a baseline Planck cosmology, and based on a modified
version of code Gadget-III which includes a massive neutrino component.
16
Given the size of the DEMNuni simulations, they are suited for different applications, that
span from BAO, to non-linear LSS clustering properties with statistics at different orders, to
the distribution of large voids in the presence of massive neutrinos, to weak-lensing, Sunyaev
Zel’dovich effects [10], and CMB secondary anisotropies analyses. I am pursuing these studies
in collaboration with the numerous members of the project.
The first DEMNUni simulation set has been characterised by a baseline ΛCDM-Planck cosmology, and four different total neutrino masses, Mν = 0, 0.17, 0.3, 0.53 eV, in the form of a
particle-component with a degenerate mass spectrum. The DEMNUni-II project includes both
massive neutrinos and the equation of state parameters of an evolving dark energy (DE) background. This project is of great importance for the study of the degeneracy at the non-linear
level between the neutrino mass and the DE parameters, especially in view of future large sky
surveys as Euclid and LSST. In fact, it is well known that neutrino effects decrease by 15%–20%
the figure of merit for dark-energy from future probes as Euclid, undermining therefore the accuracy with which dark-energy parameters can be constrained. Studying and modelling the LSS
non-linear evolution with simulated data that include dark-energy and neutrino effects will help
in adding information to data analyses, and therefore minimise/break degeneracies especially
via the combination of different probes.
In addition, one of the aim of the DEMNUni project is the realisation of end-to-end simulations in the presence of a massive neutrinos and DE, to study simultaneously weak-lensing/galaxyclustering/CMB simulated signals and their cross-correlations. In fact, end-to-end simulations
for future cosmological probes need to be based on realistic mock catalogues/maps which cannot neglect neutrino masses and evolving DE, and, at the same time, which are large enough
to simulate the nearly full-sky area probed by future surveys. Accounting for neutrino masses
and DE will help not to introduce systematic effects in statistical measurements and/or bias the
best-fit values of cosmological parameters.
The expertise developed in the cosmological simulation field, during my latest years as a
DARKLIGHT postdoc fellow in the group of Prof. Luigi Guzzo in Milan, has allowed me to be
appointed as lead of WP1 (Initial Conditions) and co-lead of WP8 (Galaxy Clustering signal)
in the Cosmological-Simulation SWG, and co-lead of WP1 (CMB-XC from N-body simulations)
in the LSS-CMB cross-correlation SWG of Euclid.
This work will be of extreme importance for the preparation of Euclid data analysis and theoretical interpretation, to which I plan to contribute with cosmological parameters extraction
via likelihood analyses applied to the combination of internal and external Euclid probes.
References
[1] Carbone C., Matarrese S., 2005, Phys. Rev. D 71, 043508-1
[2] Carbone C., Springel V., Baccigalupi C., Bartelmann M., Matarrese S., 2008, MNRAS 388,
1618
[3] Carbone C., Baccigalupi C., Bartelmann M., Matarrese S., Springel V., 2008, Mon. Not.
R. Astron. Soc. 396, 668-679 (2009)
[4] Carbone C., Verde L., Matarrese S., 2008, Astrophys. J. Lett. 684, L1
[5] Carbone C., Mena O. and Verde L., 2010, JCAP, 07, 020
[6] Grossi M., Verde L., Carbone C., Dolag K., Branchini E., Iannuzzi F., Matarrese S., Moscardini L., 2009, Mon. Not. Roy. Astron. Soc., 398, 321
17
[7] Carbone C., Verde L., Wang Y. and Cimatti A., Journal of Cosmology and Astroparticle
Physics, Issue 03, pp. 030 (2011)
[8] Castorina E., Carbone C., Bel J., Sefusatti E., Dolag K., 2015 Journal of Cosmology and
Astroparticle Physics, Issue 07, article id. 043, pp. (2015)
[9] Carbone, Carmelita; Petkova, Margarita; Dolag, Klaus, “DEMNUni: ISW, Rees-Sciama,
and weak-lensing in the presence of massive neutrinos”, eprint arXiv:1605.02024
[10] Roncarelli, Mauro; Carbone, Carmelita; Moscardini, Lauro, Monthly Notices of the Royal
Astronomical Society, Volume 447, Issue 2, p.1761-1773

Brief CV - Darklight Cosmology

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