Hubble tension as a hint for new models of dark energy

Abdolali Banihashemi

Department of Physics, Shahid Beheshti University;

Department of Physics, Sharif University of Technology

Hubble tension as a hint for new models of dark energy

سمینار به صورت هیبریدی (حضوری و مجازی) برگزار می شود

Abstract: There is a ~5sigma discrepancy between the value of H0 measured from local standard candles and the one inferred from CMB in a LCDM-dependent way. In light of this so-called Hubble tension, many models have been proposed as alternatives to the standard model of cosmology; many of which are concerned with the physics of dark energy. In this session, we will have a review of the Hubble tension and then I’ll talk about Ginzburg-Landau theory of dark energy, which is based on the physics of critical phenomena.

یکشنبه 29 آبان 1401، ساعت 17:00

Sunday 20 November 2022 – 17:00 Tehran Time

Hybrid Seminar

دانشکده فیزیک-اتاق 626–Physics department Room 626  /

https://vc.sharif.edu/ch/cosmology

گزینه ورود به صورت مهمان – Enter as a Guest

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