335 | Andrew Jaffe on Models, Probability, and the Universe
Episode
77 min
Read time
2 min
Topics
Software Development, Psychology & Behavior, Philosophy & Wisdom
AI-Generated Summary
Key Takeaways
- ✓Models as fundamental tools: Scientific understanding requires models at every level, from children building causal maps of their environment to cosmologists analyzing CMB data. Models are stories about the world that help navigate it, whether mathematical equations or mental frameworks, and no knowledge exists without them.
- ✓Bayesian probability in practice: Bayesian methods answer the question "what is the Hubble constant" directly with probability distributions (67±1 km/s/Mpc from CMB), while frequentist methods make complex statements about repeated experiments. Bayesian approaches allow marginalization over unknown parameters, making them superior for one-off astronomical events.
- ✓The Hubble tension problem: Current measurements show a significant discrepancy between CMB-derived values (67 km/s/Mpc) and supernova-based measurements (72 km/s/Mpc), separated by four to six error bars. This represents either systematic errors in observations or potentially new physics connecting early and late universe.
- ✓Entropy as knowledge-dependent: Statistical mechanics reveals that entropy and available work depend on what you know about a system. With complete information about 10^23 gas particles, you could extract more work than thermodynamic laws suggest, demonstrating that physical laws encode probabilistic statements about knowledge.
- ✓Quantum probabilities as Bayesian: Quantum mechanics provides only probabilistic predictions, whether interpreted through many worlds or QBism (quantum Bayesianism). Both frameworks treat quantum uncertainties as Bayesian probabilities about measurement outcomes rather than frequentist statements, eliminating the need for consciousness-based collapse mechanisms.
What It Covers
Andrew Jaffe explains how scientific knowledge relies on probabilistic models rather than certainty, covering Bayesian versus frequentist approaches, quantum mechanics interpretations, statistical mechanics, and measuring cosmological parameters like the Hubble constant from cosmic microwave background data.
Key Questions Answered
- •Models as fundamental tools: Scientific understanding requires models at every level, from children building causal maps of their environment to cosmologists analyzing CMB data. Models are stories about the world that help navigate it, whether mathematical equations or mental frameworks, and no knowledge exists without them.
- •Bayesian probability in practice: Bayesian methods answer the question "what is the Hubble constant" directly with probability distributions (67±1 km/s/Mpc from CMB), while frequentist methods make complex statements about repeated experiments. Bayesian approaches allow marginalization over unknown parameters, making them superior for one-off astronomical events.
- •The Hubble tension problem: Current measurements show a significant discrepancy between CMB-derived values (67 km/s/Mpc) and supernova-based measurements (72 km/s/Mpc), separated by four to six error bars. This represents either systematic errors in observations or potentially new physics connecting early and late universe.
- •Entropy as knowledge-dependent: Statistical mechanics reveals that entropy and available work depend on what you know about a system. With complete information about 10^23 gas particles, you could extract more work than thermodynamic laws suggest, demonstrating that physical laws encode probabilistic statements about knowledge.
- •Quantum probabilities as Bayesian: Quantum mechanics provides only probabilistic predictions, whether interpreted through many worlds or QBism (quantum Bayesianism). Both frameworks treat quantum uncertainties as Bayesian probabilities about measurement outcomes rather than frequentist statements, eliminating the need for consciousness-based collapse mechanisms.
Notable Moment
Jaffe describes how Einstein's general relativity predicted gravitational lensing during solar eclipses with a value exactly double Newton's prediction. Eddington's 1919 measurements during an eclipse, enabled by his Quaker pacifist exemption from World War One service, confirmed Einstein's theory within error bars while ruling out Newton.
Episode Transcript
Hey, Zach. Are you smiling at my gorgeous canyon view? No, Donald. I'm smiling because I've got something I wanna tell the whole world. Well, do it. Shout it out. T Mobile's got home Internet. Home Internet. Woah. I love that echo. T Mobile's got home internet. Internet. How much is it? Look at that, Zach. We got the neighbor's attention. Just $35 a month a month. And you love a great deal, Denise. Plus, they've got a five year price guarantee. That's five whole trips around the sun. Time switching. Boom. Yes. T Mobile home Internet for the neighborhood. Donald, you still haven't returned my weed whacker. Carl, don't you embarrass me like this, please. What's everyone yelling about? T Mobile's got home Internet. And Donald's got my weed whacker. Yes. T Mobile's got home Internet. Just $35 a month with autopay and any voice line. And it's guaranteed for five years. Yodeling. Beautiful yodeling, Carl. Taxes will be supplied. Ctmobile.com/isp for details and exclusions. Hello, everyone. Welcome to the Mindscape podcast. I'm your host, Sean Carroll. One of the ideas that has been very common in intellectual history, at least the parts of intellectual history that I know about in the world, is the search for certainty in knowledge. Rock bottom, 100% reliable knowledge of something along the lines of a proof in geometry or logic or other areas of mathematics. It turns out it took the human race a long time to learn this lesson, but it turns out that scientific knowledge, empirical knowledge about the actual world in which we live is not like that. That's not achievable in the world of the scientific exploration of the world because there's a lot of different ideas you might have about the world. There's no a priori way to reason your way into figuring out which one is the right one. And what you have to do is propose lots of different possibilities and sift through them, trying to fit them through the data and understanding that some of them fit better, some of them fit worse, some of them don't fit yet but still have a chance, and all that messy reality of the situation. We call these theories, if you wanna be a little bit less grandiose about it, models of the world. And scientists use models all the time, but it's not something you need to be grown up sophisticated scientists to do. Little children model the world, almost as soon as they're born. We mentioned this both in the podcast with Alison Gopnik and with Judea Pearl. Little kids touch things and try to build a causal map of the world around them. Scientists just do the same thing in a more sophisticated way. But like many things, the philosophical underpinnings of an idea, like the fact that scientific knowledge is provisional and probabilistic rather than certain and foundational, means that we can update our way of thinking about it, our actual technical tools …
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