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A Day in the Half-Life - Energy storage: Save your electrons for a rainy day

Energy storage: Save your electrons for a rainy day

A Day in the Half-Life

09/23/21 • 47 min

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Have you ever wondered how electricity is available all the time? That’s the seemingly magical science of energy storage. In this episode, we speak to a policy leader and a researcher about the history of piggy-banking power to spend it later, and how this field is evolving to help us prevent extreme weather-related blackouts, adopt more renewable energy, and build bigger, better, more environmentally responsible batteries.
Featuring:
Noël Bakhtian, director of Berkeley Lab's Energy Storage Center. Noel formerly served as director of the Center for Advanced Energy Studies at Idaho National Laboratory and as a senior policy advisor for the White House Office of Science and Technology Policy. Before her shift into policy and leadership, she was an engineer at NASA Ames Research Center working on Mars landing projects.
Mike Gerhardt, research scientist at SINTEF Industry in Norway helping develop new battery and fuel cell technologies using experimentation and computer modeling. Before moving to SINTEF, he was a postdoc in the Energy Conversion Group at Berkeley Lab.
*Special thanks to The Apples in Stereo for use of their song*
This episode was hosted, produced, and edited by Aliyah Kovner. Art by Jenny Nuss.
Audio samples from Halleck, Joao_Janz, and philtre.

09/23/21 • 47 min

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A Day in the Half-Life - Energy storage: Save your electrons for a rainy day

Transcript

Aliyah:

Modern life is enabled by energy on demand. And we have instant power at our fingertips because scientists and engineers have devised many means of energy storage, which is simply taking energy that was gathered or generated previously, converting it to a stable form, and stashing it until we need it again. This is a massive industry, because our homes, businesses, and infrastructure rely on electricity and rely on it being available 24/7. In order to make this possible, energy p

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