[Interview] Nobel Prize Winner Explains JWST vs The Crisis in Cosmology
Jan 29, 2024
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Dr. Adam Riess, Physics Nobel Prize laureate, discusses the Hubble Tension and the discrepancies in measuring the expansion of the Universe. They explore the significance of Cepheid variables, advancements in instruments like the James Webb Space Telescope, and the impact of dark energy. They also delve into measuring the cosmological constant and the challenges of finding supernovae. The concept of time dilation and the use of quasars as distance measuring tools are highlighted.
Cepheid variables are important distance indicators used to measure long-range distances in the universe.
The Hubble Space Telescope and the James Webb Space Telescope have played crucial roles in narrowing down the measurements of the Hubble constant.
Future telescopes like the James Webb Space Telescope have the potential to discover new objects for distance measurement and provide broader capabilities for understanding the universe.
Deep dives
Cepheid variables as a yardstick for measuring distance in the universe
Cepheid variables have been used for a century to measure long-range distances due to their tight relationship between period and luminosity. They are discrete objects and their specific mass and temperature make them excellent distance indicators. Cepheids are supergiant stars and their high luminosity allows them to be visible even in distant galaxies.
The role of Hubble Space Telescope in measuring the Hubble constant
The Hubble Space Telescope played a crucial role in measuring the Hubble constant by observing Cepheid variables in distant galaxies. Previous measurements were debated, but with the Hubble, the Hubble constant was narrowed down to 72-74 km/s/Mpc. Recent measurements from the James Webb Space Telescope have confirmed the accuracy of the Hubble measurements, ruling out errors in the imperfect sharpness of Hubble's images.
Challenges and future possibilities in measuring the expansion of the universe
The challenge lies in measuring the expansion rate of the universe beyond the Milky Way where individual motions and gravity of nearby objects dominate. New methods of measuring distance, such as using quasars or gravitational waves, are being explored, but they face difficulties due to the wide range of variation in these objects. Further progress is expected with future telescopes like the James Webb, which can cover larger areas and possibly discover new objects for distance measurement.
Challenges in Addressing the Hubble Tension
The podcast episode discusses the challenges in addressing the Hubble tension, which refers to the discrepancy in measurement results of the Hubble constant. The speaker emphasizes the need for thorough checks and improved telescopes to validate the measurements and minimize error bars. While new data collection and increased sample sizes may help reduce error bars, there are limitations to improving the precision of the Hubble constant using the current methods. However, independent measurements from other experiments like LIGO and new cosmic microwave background experiments may reveal new insights and exciting possibilities.
Exploring Potential Observations with James Webb Space Telescope
The podcast episode highlights the potential capabilities of the James Webb Space Telescope (JWST) and the observations it could make. One possibility is using tools like Cepheid variables to further simplify the measurement process and potentially improve precision. The speaker mentions the challenges of standardizing quasars and galaxies as distance indicators due to their range and inhomogeneity. However, they mention ongoing promising work with red giant stars and asymptotic giant branch stars that could be observed with JWST. The speaker also emphasizes the need for interdisciplinary approaches and new theories to better understand dark matter and dark energy, as well as the importance of future telescopes with broader capabilities to tackle unanswered questions.
The Hubble Tension is one of the most exciting mysteries in modern day science. Different methods give different results for the expansion of the Universe. So, how can we solve this and can James Webb help us with that? Or will it make things even worse? Finding out with Physics Nobel Prize laureate, Dr Adam Riess.