Origins of Heavy Elements and Neutrinos in Supernovae

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This chapter explores the role of neutrinos in the formation of heavy elements in supernovae and discusses the origins of heavy elements in the universe. It delves into the processes involved in the creation of heavy elements, such as the S-process and the R-process, as well as the importance of core collapse supernovae and neutron star mergers. The rates of these events and their impact on the abundances of heavy elements are also discussed.

In mid-20th-century cosmology, there was a debate over the origin of the chemical elements. Some thought that they could be produced in the Big Bang, while others argued that they were made inside stars. The truth turns out to be a combination of both, with additional complications layered in. Some of the elements of the periodic table come all the way from the Big Bang, but others are made inside stars or in stellar explosions. But still others are made by cosmic rays or when neutron stars and black holes merge together. We talk to nuclear astrophysicist Sanjana Curtis about all the different ways that the universe is cleverly able to produce various elements.

Blog post with transcript: https://www.preposterousuniverse.com/podcast/2024/01/08/261-sanjana-curtis-on-the-origins-of-the-elements/

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Sanjana Curtis received her Ph.D. in physics from North Carolina State University. She is currently a National Science Foundation postdoctoral fellow at the University of California, Berkeley. Her research involves nuclear astrophysics, especially the production of heavier elements in supernova explosions and neutron-star/black-hole collisions. She is also active in science communication, including at her TikTok channel.

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