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Puzzles of the New Cosmology: Expansion and smoothness of the Universe
Life and Matter Sciences Conference Tuesday, 5 April 2022, 19:00 hours Madrid
General information:
Venue: Fundación Ramón Areces - salón de actos. Calle Vitruvio, 5. 28006. Madrid.
Free admission. Necessary previous online registration. Limited capacity.
In cooperation with:
Real Academia de Ciencias and CIEMAT (Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas)
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Puzzles of the New Cosmology: Expansion and smoothness of the Universe
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- Description
- Programme
- Speaker/s
Description
The beginnings of the XXI century brought the development of the standard model of cosmology. The Universe is made of a 70% of dark energy, a 25% of dark matters and a 5% of ordinary matter. Even with a dark sector that still needs to be studied, this theory has had a brilliant success in the explanation of the cosmos. However, some new results obtained in the last few years could imply a new paradigm change. Some incompatible measurements of the expansion rate of the Universe and its smoothness place the standard model in tension. In this talk I will present a review of the new cosmology and the dark sector of the Universe, and of the tensions it faces and their possible consequences in our understanding of the cosmos.
Programme
Tuesday, 5 April
18:30 h.
Attendees check-in
19:00 h.
Puzzles of the New Cosmology: Expansion and smoothness of the Universe
Eusebio Sánchez
Departamento de Investigación Básica. CIEMAT.
Speaker/s
Eusebio Sánchez
Eusebio Sánchez has a PhD in physics and leads the cosmology group at CIEMAT. His current research area is the origin and evolution of the Universe. He holds responsibility positions in the most important international projects about cosmology. He is an author of more than 450 papers in scientific international journals and has worked in several laboratories of physics around the world, like CERN or Fermilab. His research covers a wide spectrum of scientific topics, from particle physics to the physical nature of dark matter and dark energy.
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