Book contents
- Frontmatter
- Contents
- Foreword
- Preface
- I Survey of the Problem
- II Thermodynamics of Radiation
- III Quantum Theory
- IV Polytropic Gas Spheres
- V Radiative Equilibrium
- VI Solution of the Equations
- VII The Mass-Luminosity Relation
- VIII Variable Stars
- IX The Coefficient of Opacity
- X Ionisation, Diffusion, Rotation
- XI The Source of Stellar Energy
- XII The Outside of a Star
- XIII Diffuse Matter in Space
- APP. I Physical and Astronomical Constants
- APP. II References
- INDEX
II - Thermodynamics of Radiation
Published online by Cambridge University Press: 01 June 2011
- Frontmatter
- Contents
- Foreword
- Preface
- I Survey of the Problem
- II Thermodynamics of Radiation
- III Quantum Theory
- IV Polytropic Gas Spheres
- V Radiative Equilibrium
- VI Solution of the Equations
- VII The Mass-Luminosity Relation
- VIII Variable Stars
- IX The Coefficient of Opacity
- X Ionisation, Diffusion, Rotation
- XI The Source of Stellar Energy
- XII The Outside of a Star
- XIII Diffuse Matter in Space
- APP. I Physical and Astronomical Constants
- APP. II References
- INDEX
Summary
Radiation Pressure.
21. Radiant energy or radiation consists of electromagnetic waves in the aether. Maxwell's electromagnetic theory showed that these waves possess momentum. If E is the energy of the waves, c the velocity of light, the momentum is E/c in the direction in which the waves are travelling.
According to the modern view energy and mass are inseparable, c2 ergs corresponding to 1 gm. This leads immediately to the same result. For the energy E ergs indicates a mass E/c2 gm., and since the velocity is c the momentum is (E/c2) × c = E/c.
A material screen which absorbs the waves absorbs also their momentum. Thus the momentum of the screen changes, which is another way of saying that it is acted on by a force. Suppose that waves containing E ergs per cu. cm. impinge normally on a perfectly absorbing surface. A column of radiation of height c passes into and is absorbed by each sq. cm. of the surface per sec.; this column contains Ec ergs and the momentum is thus Ec/c or E units. The force on the screen is thus E dynes per sq. cm.
For imperfect absorbers we must deduct the proportion of the momentum which is not passed on to the material screen, viz. that of the transmitted, scattered or reflected waves. For example, a perfect reflector would experience a pressure 2E; half of this is due to its stoppage of the incident waves and half is the recoil due to the projection of the train of reflected waves.
- Type
- Chapter
- Information
- The Internal Constitution of the Stars , pp. 27 - 43Publisher: Cambridge University PressPrint publication year: 1988