Licia Verde | |
---|---|
Born | 14 October 1971 53) Venice, Italy | (age
Alma mater | University of Padua University of Edinburgh |
Known for | Cosmic microwave background large-scale structure |
Awards | Gruber Prize in Cosmology (2012) ISI highly cited researcher (2015) European Research Council award (2009 & 2016) Narcis Monturiol Medal (2018) Breakthrough Prize in Fundamental Physics (2018) National Research Award of Catalonia (2018) European Astronomical Society Lodewijk Woltjer Lecture (2019) Rey Jaime I Awards (2021) Medalla de la Real Sociedad Española de Física (2024) |
Scientific career | |
Fields | Cosmology, physics, astrophysics |
Institutions | University of Edinburgh Princeton University University of Pennsylvania University of Barcelona University of Oslo Radcliffe Institute for Advanced Study |
Doctoral advisor | Alan F. Heavens |
Other academic advisors | Sabino Matarrese |
Licia Verde (born 14 October 1971, Venice, Italy) is an Italian cosmologist and theoretical physicist and currently ICREA [1] Professor of Physics and Astronomy at the University of Barcelona. [2] Her research interests include large-scale structure, dark matter, dark energy, inflation and the cosmic microwave background.
She received a Laurea degree in 1996 from University of Padua and a PhD in 2000 from the University of Edinburgh, working with Sabino Matarrese and Alan F. Heavens. She did postdoctoral study at Princeton University and joined the faculty of The University of Pennsylvania in 2003. From September 2007, Verde is an ICREA Professor at the ICCUB of the University of Barcelona. She was a Professor II at the University of Oslo during 2013 to 2016. [3] Verde was editor of the Physics of the Dark Universe Journal [4] and is currently scientific director of the Journal of Cosmology and Astroparticle Physics. [5] As of 1 January 2019 she is the chair of the science advisory board of the arXiv.
She is known primarily for work on large-scale structure, analysis of the WMAP data and development of rigorous statistical tools to analyse surveys of the universe. She is a highly cited author. [6] [7] [8]
She appeared in the movie The Laws of Thermodynamics and is featured in the PBS show Closer to Truth in its 2020 season.
Licia Verde was born in Venice, Italy where she grew up. She attended the Liceo classico Marco Polo before she started her undergraduate studies at the University of Padua. She moved to the University of Edinburgh in the fall of 1994, first as an Erasmus and later as a PhD student.[ citation needed ]
Verde was a research associate at the Dept. of Astrophysical Sciences, Princeton University during 2000 to 2003. In 2003, she joined the faculty of the Physics and Astronomy Dept. of the University of Pennsylvania [9] and remained there until the end of 2007. Since 2008, she is ICREA Professor of Cosmology at the University of Barcelona [10] in Spain. She has also held several faculty visiting positions: Visiting Scholar at the IAS in Princeton, USA (2005); [11] Visiting Senior Research Fellow at the Dept. of Astrophysical Sciences of Princeton University (2007-2009); Scientific Associate at CERN (2012-2013); Professor II of Physics and Astronomy at the University of Oslo (2013-2016) and Radcliffe Fellow at the Radcliffe Institute for Advanced Study, Harvard University (2015-2016). [12] In 2019 she was appointed chair of the science advisory board of the arXiv and in 2020 scientific director of the Journal of Cosmology and Astroparticle Physics . [5]
Verde analyzed a powerful but challenging statistical property of galaxy surveys related to higher-order correlations. She showed that the galaxy redshift survey conducted with the Anglo-Australian Telescope trace the distribution of dark matter; this result indicated that the galaxy distribution can be used to study the dark matter one. [27]
After she joined the science team of the Microwave Anisotropy Probe, a NASA space mission to map the full sky at radio waves, Verde participated in analysis and interpretation of the Cosmic Microwave Background data from the WMAP satellite. [28]
Thanks to two ERC grants: Cosmological Physics with future large-scale structure surveys (Phys.LSS), [17] and Beyond Precision Cosmology: dealing with Systematic Errors (BePreSyE) [20] Verde has established a research group in physical cosmology at the University of Barcelona. Under her lead, the group has contributed to results from the Baryon Acoustic Oscillations Survey part of the Sloan Digital Sky Survey: measurements of the expansion history of the universe and the formation of cosmological structures as well as constraint on cosmological parameters describing structure and detailed composition of the cosmos.[ citation needed ]
The other recent direction of Verde's research is on dark energy. She has developed a model-independent way to study the Universe's expansion history and infer from there the physical properties of dark energy. [29]
The Big Bang is a physical theory that describes how the universe expanded from an initial state of high density and temperature. The notion of an expanding universe was first scientifically originated by physicist Alexander Friedmann in 1922 with the mathematical derivation of the Friedmann equations.
The cosmic microwave background, or relic radiation, is microwave radiation that fills all space in the observable universe. With a standard optical telescope, the background space between stars and galaxies is almost completely dark. However, a sufficiently sensitive radio telescope detects a faint background glow that is almost uniform and is not associated with any star, galaxy, or other object. This glow is strongest in the microwave region of the radio spectrum. The accidental discovery of the CMB in 1965 by American radio astronomers Arno Penzias and Robert Wilson was the culmination of work initiated in the 1940s.
The Wilkinson Microwave Anisotropy Probe (WMAP), originally known as the Microwave Anisotropy Probe, was a NASA spacecraft operating from 2001 to 2010 which measured temperature differences across the sky in the cosmic microwave background (CMB) – the radiant heat remaining from the Big Bang. Headed by Professor Charles L. Bennett of Johns Hopkins University, the mission was developed in a joint partnership between the NASA Goddard Space Flight Center and Princeton University. The WMAP spacecraft was launched on 30 June 2001 from Florida. The WMAP mission succeeded the COBE space mission and was the second medium-class (MIDEX) spacecraft in the NASA Explorer program. In 2003, MAP was renamed WMAP in honor of cosmologist David Todd Wilkinson (1935–2002), who had been a member of the mission's science team. After nine years of operations, WMAP was switched off in 2010, following the launch of the more advanced Planck spacecraft by European Space Agency (ESA) in 2009.
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