- 51猎奇入口 Us
- People
- Undergrad
- Graduate
- Research
- News & Events
- Why Physics @SFU
- Equity
- _how-to
- Congratulations to our Class of 2021
- Archive
- AKCSE
- Atlas Tier 1 Data Centre
Colloquium
Cosmology, Galaxy Formation, and Planets with James Webb Space Telescope
Joel Primack, UC Santa Cruz
Location: C9000 & Online
*Register at the following link to join seminar:
Access link will be sent to your email address after registration
Synopsis
The modern standard cosmology 螞CDM describes almost perfectly the cosmic microwave background observations, but the resulting expansion rate of the universe (the Hubble parameter) is in serious disagreement with local measurements. This Hubble tension can perhaps be resolved by a brief episode of dark energy contributing about 10% of cosmic energy density for just a few thousand years about 50,000 years after the Big Bang. This high-redshift Early Dark Energy (EDE) scenario can be tested at lower redshifts, since new N-body simulations show that EDE predicts earlier structure formation than 螞CDM, for example 50% more clusters at redshift z 鈭� 1 and 10x more galaxies at z ~ 10. Such predictions are being tested by new observations, including by James Webb Space Telescope. JWST鈥檚 infrared capabilities allow its cameras to see starlight from even the highest-redshift galaxies. JWST鈥檚 better resolution than Hubble Space Telescope is also revealing new aspects of galaxy and planet formation. Earth is a Goldilocks planet, in the Sun鈥檚 habitable zone and also with just the right amount of radioactive heating by thorium and uranium for a long-lived magnetic field and plate tectonics 鈥� both of which may be necessary for the evolution of complex life. Such Goldilocks exoplanets, taking into account the abundance of Th and U deduced from the star鈥檚 spectrum, should be among the first planets to be searched by JWST for biosignatures.