
The Life of Stars
The Controversial Inception and Emergence of the Theory of Stellar Structure
By: Giora Shaviv
Hardcover | 2 November 2009
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520 Pages
23.5 x 15.88 x 2.54
Hardcover
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Industry Reviews
From the reviews:
"The story of stellar structure is interwoven with the development of quantum mechanics and the determination that nuclear fusion reactions produce the energy emitted by stars. The author provides excellent coverage of those two developments. He also effectively notes that stellar theorists often had access, in principle, to information that would have allowed them to take giant leaps toward a solution." (Robert Deupree, Physics Today, November, 2010)
"For historians of science, Shaviv has done a considerable service by searching out many obscure or forgotten papers amongst the important and well-known ones, and he does give references to almost everything. He adds quite extensive footnotes as well." (Robert Connon Smith, The Observatory, Vol. 131 (1220), February, 2011)
"I thoroughly enjoyed this book. ... it especially enjoyable for me were the tiny snippets or anecdotes which appear quite liberally throughout the book, sometimes in the main text but more usually as a footnote. ... The author, Giora Shaviv, is a leading theoretical astrophysicist. ... The writing style is easy and the book is exceedingly well referenced." (Roger Pickard, Journal of the British Astronomical Association, Vol. 120 (5), 2010)
| The Controversy about the Age of the Earth | p. 1 |
| The Pre-Scientific Era | p. 1 |
| Charles Lyell and Jean Fourier | p. 3 |
| Energy Conservation: Helmholtz and Mayer | p. 9 |
| The Source of Solar Energy | p. 13 |
| Charles Darwin | p. 16 |
| Devout Criticism of Darwin | p. 21 |
| Scientific Criticism of Darwin | p. 23 |
| First Attempt to Quantify the Meteor Theory | p. 24 |
| Kelvin | p. 25 |
| The Darwin-Kelvin Controversy | p. 29 |
| The Birth of the Theory of Stellar Structure | p. 34 |
| Was Solar Contraction Observed? | p. 39 |
| Is the Sun Realty Liquid? | p. 44 |
| What Stellar Classification Tells Us | p. 45 |
| Secchi. The First Steps | p. 45 |
| Huggins and Lockyer. Scientific Astrophysical Spectroscopy | p. 47 |
| Is There a Universal Abundance? | p. 51 |
| Harvard and Potsdam | p. 52 |
| Vogel. The Helium Stars | p. 53 |
| The Henry Draper Project | p. 54 |
| Oh Be A Fine Girl Kiss Me | p. 55 |
| Anjar Hertzsprung. First Correlations | p. 58 |
| The 1910 Referendum: Science by Popular Vote? | p. 63 |
| Warning Signs | p. 66 |
| Henry Norris Russell | p. 67 |
| The Discussion on the Diagram | p. 70 |
| Summary for 1915 | p. 71 |
| The Dawn of a New Era | p. 75 |
| The Ultimate Answer to the Earth Age Problem: Radioactivity | p. 75 |
| The Complicated Structure of the Earth | p. 75 |
| The Invention of the Cathode Ray Tube | p. 76 |
| Dispersing Kelvin's Clouds. A New Horizon | p. 77 |
| Rutherford's 1907 Address | p. 96 |
| The Atom Is Mostly Empty | p. 99 |
| Science by Committee | p. 102 |
| New Elements or Misled by the Stars | p. 104 |
| The First Atomic Quantum Theory | p. 109 |
| Kelvin and the Age of the Earth. An Epilog | p. 111 |
| What We Know Today about the Age of the Earth | p. 112 |
| Heat How | p. 113 |
| Towards a Complete Theory of Stellar Structure | p. 115 |
| Eddington. The First Stellar Model with Radiative Transfer | p. 115 |
| Stars Are Gaseous | p. 115 |
| Radiation Pressure Plays a Crucial Role in Stars | p. 116 |
| Basic Astrophysics: The Stars Obey Our Laws of Physics | p. 119 |
| Absorption of Radiation. A Key Issue | p. 119 |
| Two Logical Steps Leading to the Role of Radiation Pressure | p. 120 |
| Is the Contraction Energy Sufficient? | p. 121 |
| Some Surprising Expressions | p. 122 |
| Can We Model the Sun? | p. 122 |
| The Achilles Heel | p. 122 |
| The Second Paper | p. 123 |
| The Mean Molecular Weight | p. 123 |
| Why Is the Molecular Weight Important for a Star? | p. 124 |
| A New Phase of Matter | p. 125 |
| How Much Can a Star Radiate? | p. 127 |
| Variable Stars as Theory Testers | p. 129 |
| Leavitt's Cepheid Variable Observations | p. 130 |
| Some Time Perspectives | p. 132 |
| A Death Blow to the Binary Hypothesis | p. 133 |
| The Theory of Stellar Pulsation | p. 135 |
| Hertzsprung Again. A Small Digression | p. 138 |
| A Confusing Issue. The Bizarre White Dwarfs | p. 139 |
| Can We Already Guess What the Energy Source Might Be? | p. 142 |
| Eddington's Response to Russell | p. 143 |
| The Components of the Nucleus | p. 144 |
| Early Hints | p. 146 |
| Eddington's Presidential Address | p. 148 |
| Predicting Saturation in the Absorption | p. 149 |
| The Prediction of Nuclear Energy and Transmutation of the Elements | p. 151 |
| Chemical Elements in Equilibrium | p. 153 |
| Eddington Discovers Kramers' Law | p. 154 |
| The Universe Has Uniform Composition | p. 155 |
| Hertzsprung Once More. The Observed Mass-Luminosity Law | p. 157 |
| Kramers Discovers His Law | p. 159 |
| Absorption in Strong Radiation Fields | p. 160 |
| Subatomic Energy in Difficulty | p. 160 |
| Saha. Getting the Stellar State | p. 161 |
| The Theoretical Mass-Luminosity Law | p. 163 |
| Conceptual Difficulties | p. 166 |
| Objections to the Mass-Luminosity Law | p. 168 |
| The Writing Was on the Wall | p. 170 |
| The Russell-Vogt Theorem' | p. 171 |
| The Rosseland Mean: The Situation Worsens | p. 173 |
| Are the Stars Well Mixed? | p. 174 |
| The Absorption Coefficient Dispute and the Mass-Luminosity Relation | p. 178 |
| The Mass-Luminosity Relation Again | p. 179 |
| How Pristine the Stars Remain | p. 181 |
| A Devastating Argument | p. 182 |
| Reaching the Limits of Knowledge | p. 185 |
| Russell Again. Discovery of the Most Abundant Element in the Solar Atmosphere | p. 186 |
| Two Birds in a Single Shot | p. 189 |
| The Hydrogen in the Sun | p. 192 |
| First Signs of Finer Details | p. 194 |
| The Cowling Model | p. 195 |
| From Chemistry to Dying Stars | p. 197 |
| The Problem with the Existence of Different Atoms | p. 197 |
| The Road to the Pauli Principle. The Multi-Electron Atom | p. 197 |
| The Chemists Have It Differently | p. 198 |
| The Helium Atom | p. 200 |
| The Physicists' Approach. Was It Any Better? | p. 201 |
| Bohr and the Periodic Table | p. 203 |
| Stoner. Getting Closer | p. 204 |
| The Pauli Principle | p. 204 |
| The Unique Behavior of Particles | p. 208 |
| The Behavior of a Collection of Particles | p. 210 |
| Why the Difference in Behavior? Why Does PEP Apply? | p. 211 |
| Why Is There Chemistry? Why Does Matter Have Its Bulky Form? | p. 212 |
| Observational Limits on the Pauli Principle | p. 214 |
| Eddington's White Dwarf Paradox | p. 215 |
| Cracking the Paradox: Ralph Fowler 1926 | p. 215 |
| Pokrowski. A Limit on the Mass of a Collapsed Star | p. 217 |
| Anderson Expands on Pokrowski's Idea, but Changes the Reasons | p. 218 |
| Stoner Again | p. 219 |
| Anderson | p. 220 |
| Stoner Responds | p. 221 |
| Chandrasekhar. The Final and Accurate Answer | p. 224 |
| What Determines Stellar Masses? | p. 227 |
| 1930. Milne's Attack on Eddington's Stellar Structure | p. 229 |
| Condensed Models | p. 232 |
| Independent Derivation of the Limiting Mass | p. 238 |
| Erupting Stars | p. 242 |
| The Observations of How Stars Perish | p. 243 |
| The Transformation of Matter into Neutrons | p. 254 |
| The Neutron Star | p. 256 |
| Oppenheimer: The Collapse to a Neutron Star | p. 257 |
| Back to Observations | p. 259 |
| Novas and Supernovas Are Not the Same Thing | p. 260 |
| Clinching the Identification | p. 260 |
| There Is More Than One Type of Supernova | p. 261 |
| Is There Any Remnant? | p. 262 |
| The Discovery of Neutron Stars | p. 263 |
| Eddington's Objection to the White Dwarf Theory | p. 264 |
| No Escape for Massive Stars | p. 267 |
| Newtonian Black Holes versus Einsteinian Black Holes | p. 268 |
| Schwarzschild. Solving the Einstein Equations | p. 268 |
| Einstein and Black Holes | p. 271 |
| Observations of Black Holes | p. 272 |
| The Solution to the Stellar Energy Problem | p. 275 |
| The Quantum Revolution | p. 276 |
| We Have Already Seen this Movie | p. 278 |
| Light at the End of the Tunnel | p. 278 |
| Tunneling: The Secret of Stellar and Biological Time Scales | p. 281 |
| Tunneling Under Stellar Conditions | p. 283 |
| The Paradox of the Giants | p. 284 |
| A Snag? | p. 285 |
| Creation and Annihilation of Matter in Stars. A Brief Comeback | p. 286 |
| The Masses of Nuclei | p. 289 |
| The Birth of Nuclear Astrophysics | p. 290 |
| The Idea of Regenerative Synthesis | p. 291 |
| The 8Be4 Barrier | p. 294 |
| The Discovery of the Neutron | p. 300 |
| New Horizons. Astrophysics | p. 301 |
| New Horizons. Nuclear Physics | p. 302 |
| Deuterium Exists and Is Stable | p. 303 |
| The Weak Force. Key to Stellar Longevity | p. 305 |
| The Return of Atkinson | p. 308 |
| The Last Paper on Liquid Stars | p. 310 |
| The Nuclear Dilemma: Equilibrium Versus Rate | p. 310 |
| At Last: A Fatal Blow to Classical Mass Annihilation | p. 313 |
| Back to the Nuclear Barrier | p. 315 |
| Weizsäcker | p. 317 |
| The First Paper | p. 317 |
| The Second Paper | p. 319 |
| Gamow Again | p. 325 |
| The Energy Source | p. 326 |
| A Problem of Stability | p. 327 |
| Hans Bethe | p. 328 |
| The First Calculation of the pp Reaction | p. 328 |
| Hans Bethe and the CN Cycle | p. 332 |
| Acceptance by the Community and New Puzzles | p. 336 |
| The Last Piece of Nuclear Data | p. 337 |
| The First Full Model of the Sun | p. 338 |
| The Fate of the Sun | p. 339 |
| Accretion: Revival of Helmholtz? | p. 339 |
| How the Low Mass Stars Perish | p. 341 |
| The Energy Source of White Dwarfs | p. 341 |
| The Central Stars of Planetary Nebulas | p. 346 |
| The Harman-Seaton Sequence | p. 354 |
| Stellar Evolution to PN Formation | p. 362 |
| Some of the Remaining Problems with the White Dwarfs | p. 364 |
| Masses of the Central Stars | p. 364 |
| Shaping the PN | p. 365 |
| A Few Present Day Challenges for Understanding PNs | p. 366 |
| From the Vantage Point of Time | p. 366 |
| The Life and Death of Massive Stars | p. 369 |
| New Physics: A Prelude | p. 369 |
| The Creation of the Weak Interaction Theory | p. 373 |
| The Evolution of Massive Stars | p. 374 |
| The Explosive Climax: Properties of the 'Classical' Supernovas | p. 378 |
| Supernova Theory | p. 383 |
| The Trigger | p. 385 |
| The Explosion. A History of Unsubstantiated Proclamations | p. 397 |
| Type II SNs | p. 398 |
| Type I SNs | p. 403 |
| Esoteric Mechanisms? | p. 404 |
| Peculiar SNs. An Example | p. 405 |
| Obstacles to Understanding the SN Phenomenon and the Formation of the Elements Beyond C and O | p. 408 |
| The Light Curve | p. 409 |
| The Tale of a Recent Supernova. What One Good Case Can Tell Us | p. 413 |
| Identification and Scattered Records | p. 415 |
| Neutrinos | p. 418 |
| The Detection of Gamma Ray Line Emission | p. 420 |
| The SN 1987 A Light Curve | p. 425 |
| The Rings that Rang the Bell | p. 431 |
| The Progenitor and the Ring Structure | p. 433 |
| Single Star Evolution | p. 435 |
| Binary Star Evolution | p. 436 |
| The Binary Merged | p. 436 |
| A Few of the Remaining Unsolved Questions | p. 438 |
| The Latest Images | p. 440 |
| Life and Death Under Supernova Control | p. 440 |
| Recent News: Ultra-Powerful Supernovas | p. 449 |
| Provisional Summary | p. 452 |
| The Sun | p. 455 |
| How Come Life Survives on the Earth | p. 455 |
| Victory for Stellar Structure Theory. The Solar Neutrino | p. 458 |
| How the Solar Neutrino Problem Came into Being | p. 459 |
| Doubts and Possible Implications | p. 462 |
| The Most Energetic Solar Neutrino Source Identified | p. 464 |
| The Neutrino Confusion | p. 466 |
| The Pioneer in Solar Neutrino Experiments | p. 468 |
| Suggested Astrophysical Solutions | p. 470 |
| Is the Sun a Perfect Sphere? | p. 472 |
| Is Statistical Mechanics Defective in the Sun? | p. 474 |
| A Unique Mode of Formation? | p. 475 |
| New Astrophysical Processes | p. 476 |
| Astrophysical Summary | p. 476 |
| Suggested Elementary Particle Solutions | p. 477 |
| Have All Neutrino Types been Discovered? | p. 481 |
| A New Generation of Neutrino Detectors | p. 483 |
| The Soviet-American Gallium Solar Neutrino Experiment (SAGE) | p. 483 |
| GALLEX | p. 484 |
| Super-Kamiokande | p. 485 |
| Sudbury Neutrino Observatory (SNO) | p. 487 |
| Summary of Solar Neutrino Experiments | p. 488 |
| Helioseismology: Independent Confirmation of Stellar Structure | p. 490 |
| Some Reflections | p. 491 |
| Further Implications | p. 493 |
| Closing the Circle: Neutrino Geology | p. 493 |
| Index | p. 495 |
| Table of Contents provided by Ingram. All Rights Reserved. |
ISBN: 9783642020872
ISBN-10: 3642020879
Published: 2nd November 2009
Format: Hardcover
Language: English
Number of Pages: 520
Audience: General Adult
Publisher: Springer Nature B.V.
Country of Publication: DE
Dimensions (cm): 23.5 x 15.88 x 2.54
Weight (kg): 0.86
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