Skip to content

Cosmic Queries – Proving Einstein Right

StarTalk Podcast

Hosted by Neil deGrasse Tyson

52m
guest
1
Transcript

Original podcast

Summary

Written by a model from the transcript; not yet reviewed.

Neil deGrasse Tyson hosts a conversation with theoretical physicist Jim Gates, director of the Center for Theoretical Physics at Brown University, about Gates' 2019 book "Proving Einstein Right: The Daring Expeditions That Changed How We Look at the Universe." Gates explains how Einstein's general relativity, completed in 1915–16, required experimental verification through the bending of starlight during a solar eclipse, a concept that emerged from discussions with German astronomer Erwin Finlay-Foinlich around 1912.

The episode also covers the distinction between special and general relativity, the incompatibility of general relativity with quantum mechanics, the search for gravitons as the next major prediction to test, and string theory's potential to leave signatures in the cosmic microwave background. Gates emphasizes that Einstein was not a solitary genius but relied heavily on colleagues to refine his ideas, and that mathematics is the only human language that accurately describes nature.

The discussion touches on gravitational lensing, Einstein rings, and the possibility of a cosmic gravitational background, with Gates estimating 20 to 30 years before sufficient gravitational wave detectors exist to map it.

  • Einstein's general relativity took nearly a decade (1907–1915/16) to complete because he had to learn new mathematics to match his physical intuition. 9:54
  • The bending of starlight during a solar eclipse was the first experimental verification of general relativity, a concept that emerged from discussions with astronomer Erwin Finlay-Foinlich. 12:29
  • Detecting gravitons would be the next major prediction to test from general relativity, analogous to how photons are the particle form of light. 32:18
  • String theory may leave observable signatures in the cosmic microwave background, a concept Gates and colleagues called "Susy Reals." 39:47
  • There are currently about four gravitational wave detectors in the world, and Gates estimates 20 to 30 years before sufficient mapping of a gravitational background is possible. 46:45

Highlights

  • 8:47

    Einstein's Happiest Thoughtstory

    Einstein, still working at the patent office in 1907, watched a workman on a roof and realized that a falling person would feel weightless. He called this the happiest thought of his life, and it launched his decade-long path to general relativity.

  • 14:46

    Scientists Swim in Informationinsight

    Gates argues against the lone-genius stereotype, saying that being a scientist means swimming in a sea of information that comes from colleagues, and that Einstein himself worked out special relativity with a friend on a tram ride in Bern.

  • 17:49

    Mathematics as the Only Magicinsight

    Gates calls mathematics the only piece of magic he has ever experienced in reality, describing it as a third eye that lets scientists see things otherwise invisible, and the only human language that accurately describes nature.

  • 24:04

    Gravity Is Bending Spacetimestrategy

    Gates explains general relativity in a short course: gravity is not a force but the bending of spacetime itself, a concept that even Newton never answered. This contrasts with special relativity, which deals only with relative motion and the Doppler effect on light.

  • 31:16

    The Graviton as Next Frontierdata

    Gates identifies the quantization of energy carried by gravitational waves as the next big prediction to test. Detecting gravitons would move the concept from Star Trek science fiction into established physics, though no experiment currently exists to do so.

  • 39:47

    String Theory Signatures in the CMBinsight

    Gates describes a 2024 paper with colleagues at Brown showing that string theory could write observable structures called "Susy Reals" in the cosmic microwave background, meaning astrophysicists may be key to testing string theory.

  • 49:17

    Seeing Quasars Twice via Lensingdata

    Neil explains that gravitational lensing by galaxy clusters can produce multiple images of a quasar, and because the path lengths differ, the same brightness variation is observed at two different times, confirming the curvature of space.

  • 51:33

    Black Holes Are Not Blackinsight

    Gates notes that thanks to Hawking radiation, black holes are not truly black. He also states he has encountered no solid scientific arguments for the existence of white holes, and we see nothing in the universe that would match their predicted signature.

Guests

About this episode

Albert Einstein was, well, Albert Einstein. But was he right? Neil deGrasse Tyson and Chuck Nice investigate what it took to prove Einstein right, with theoretical physicist Dr. Jim Gates. Originally Aired October 19, 2020.

Transcript

0:00
52:57

8,889 words · 4 speakers

Speaker names marked are inferred from speaking time and the show’s known hosts — they are not voice-verified.

Topics

  • General Relativity
  • Quantum Mechanics
  • String Theory
  • Gravitational Waves
  • Theoretical Physics
  • Gravitational Lensing
  • Cosmology
  • Einstein

Page updated · transcript and summary are machine-generated