
BY
In this address, a pioneering physicist looks back to the restless years when the puzzle of heat radiation first began to tease out a new fundamental constant. He walks the listener through the experimental clues—from Kirchhoff’s universal radiation law to Hertz’s resonators—that hinted at a deeper link between energy, temperature, and frequency, and describes his own early attempts to explain the black‑body spectrum using classical ideas. The narrative captures the mixture of optimism and frustration that drove the search for a reliable description of the energy distribution in radiant heat.
The speaker then outlines how a bold, quantitative step—introducing a discrete “quantum of action”—reoriented the whole field, setting the stage for a theory that would soon reshape atomic and molecular physics. By tracing this early development, the talk offers a clear picture of how a single insight blossomed into the quantum framework that underpins much of today’s science, inviting listeners to experience the intellectual adventure that launched modern physics.
Language
en
Duration
~36 minutes (34K characters)
Publisher of text edition
Project Gutenberg
Release date
2010-09-07
Rights
Public domain in the USA.
Subjects

1858–1947
A quiet, careful thinker who changed physics forever, he opened the door to quantum theory with his work on blackbody radiation and energy quanta. Awarded the 1918 Nobel Prize in Physics, he became one of the central figures in modern science.
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