Philip Mannheim: The Story of Conformal Gravity
Theories of Everything with Curt Jaimungal
Curt Jaimungal
4.6 • 616 Ratings
🗓️ 6 July 2026
⏱️ 155 minutes
🔗️ Recording | Apple Podcasts | RSS
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| 0:00.0 | The missing mass that we've defined as the art matter problem isn't missing. It's the rest of the |
| 0:06.4 | visible universe and it's been hiding in plain size. It's been there all along. Is the Graviton |
| 0:11.6 | then composite or fundamental? It's neither. It doesn't exist. Man, talk about fighting words. |
| 0:18.0 | Nature will keep you honest. This is the legendary Professor Philip Mannheim, |
| 0:22.8 | and today I'm excited to bring you his first ever podcast. |
| 0:26.5 | He's been working on a theory which solves dark matter and quantum gravity |
| 0:29.8 | simultaneously for literally decades. |
| 0:32.9 | You start out with a standard theory. |
| 0:35.0 | It doesn't work for galaxies, so you invent dark matter. It doesn't work for cosmology. You invent dark energy. It doesn't work for quantum theory, so you invent string theory. I haven't done that. I've just taken the theory and I've solved it. On this channel, I, Kurtzai Mungle, interview researchers regarding their theories of reality with rigor and technical depth. Today, what the professor argues is that we've been wrong about dark matter. |
| 0:56.9 | We also have no big bang in the universe, according to his theory. |
| 1:00.6 | Add further speculations on what collapses the wave function is a particle that we don't see. |
| 1:05.4 | It's one of the most startling discoveries in human history. |
| 1:08.6 | I can't describe it any other way. |
| 1:13.1 | Welcome to the story of conformal gravity. Professor, what precisely is Einstein's theory of gravity? Oh, well, I have to give you a |
| 1:20.5 | somewhat extensive answer to that. Einstein, in the early 20th century, developed what's called the special theory of relativity, |
| 1:29.6 | and he was dealing with a problem, and the problem was there was Newton's laws of motion, |
| 1:36.9 | and there were the Maxwell equations of electromagnetism, and they had different symmetries. |
| 1:42.9 | And what Einstein realized was there had to be a universal symmetry, |
| 1:46.0 | which we now call Lorentz invariance, |
| 1:49.0 | which meant modifying Newton's law. |
| 1:52.0 | And you can see this very simply, if you take Newton's law, |
| 1:55.0 | it just says you apply a force, you get an acceleration. |
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