ASTRONOMICAL SPECTROSCOPY This page intentionally left blank Imperial College Press Advanced Physics Texts – Vol. 2 ASTRONOMICAL SPECTROSCOPY An Introduction to the Atomic and Molecular Physics of Astronomical Spectra by JONATHAN TENNYSON University College Londomn, UK PressImperial College Published by Imperial College Press 57 Shelton Street Covent Garden London WC2H 9HE Distributed by World Scientific Publishing Co. Pte. Ltd. 5 Toh Tuck Link, Singapore 596224 USA office: 27 Warren Street, Suite 401-402, Hackensack, NJ 07601 UK office: 57 Shelton Street, Covent Garden, London WC2H 9HE British Library Cataloguing-in-Publication Data A catalogue record for this book is available from the British Library. ASTRONOMICAL SPECTROSCOPY An Introduction to the Atomic and Molecular Physics of Astronomical Spectra Copyright © 2005 by Imperial College Press All rights reserved. This book, or parts thereof, may not be reproduced in any form or by any means, electronic or mechanical, including photocopying, recording or any information storage and retrieval system now known or to be invented, without written permission from the Publisher. For photocopying of material in this volume, please pay a copying fee through the Copyright Clearance Center, Inc., 222 Rosewood Drive, Danvers, MA 01923, USA. In this case permission to photocopy is not required from the publisher. ISBN 1-86094-513-9 ISBN 1-86094-529-5 (pbk) Typeset by Stallion Press Email: [email protected] Printed in Singapore. May18,2005 12:24 WSPC/SPI-B267:AstronomicalSpectroscopy fm PREFACE This book follows closely a lecture course I gave entitled ‘Astronomical Spectroscopy’tothird-yearundergraduatestudentsatUniversityCollege London between 1998 and 2003. The students who attended had done a prior introductory course on Quantum Mechanics which covered the hydrogen atom but no further atomic physics or spectroscopy. A similar levelofpriorknowledgeisassumedinthecurrentwork. Therearemanypeoplewhosehelphavebeenessentialforthecomple- tion of this book. First I must thank BillSomerville who inaugurated the courseAstronomicalSpectroscopyandtaughtitfortwoyearsbeforeme. Heselflesslysharedhislecturenotesandothermaterialswithme.Iwould like to thank Ceinwen Sanderson for turning my hand-scrawled lecture A notesintoLTEX,andmycolleaguesTonyLynas-Gray,BillSomerville,Peter Storeyand JeremyYatesfor their extensivecomments on the draftof the book. I owe a debtof gratitude to my graduatestudents Bob Barberand Natasha Doss who checked all the problems and found many errors. I thankallofthemforthecorrections;anyerrorsthatremainareallmine. I must alsothankthe studentswho attendedmyAstronomicalSpec- troscopy course. It was great fun to teach, not least because the latest developments in astrophysics often fed straight into the lectures. Partic- ular thanks are due to the class of 2003 who made a number of helpful commentsandsuggestionsonthecontentsofthebook. A book on spectroscopy thrives on good illustrations and I have shamelesslyplunderedtheliteratureandothersourcesforspectratoillus- trate this one. I must thank Xiaowei Liu for help with digitising many of the published spectra, my student Iryna Rozum, my son Matthew, and especially David Rage for their help with the other illustrations. v May18,2005 12:24 WSPC/SPI-B267:AstronomicalSpectroscopy fm vi AstronomicalSpectroscopy I thank the journal publishers and the many authors who greeted my requests to reproduce their work with prompt enthusiasm, especially thoseauthorswhoadaptedfiguresatmyrequest.Eachjournalandauthor isindividuallyacknowledgedinthefigurecaptions. Finally I must acknowledge the UCL astronomers of the past and present who have answered my many questions on astrophysics with a patience their frequent stupidity probably did not deserve. Particularly highonthislistarePeteStoreyandMikeBarlow,buttherestofthevaried lunchcrewshouldnotbeforgotten.Withoutyoumyknowledgeofthings astronomical would be the same as it was the day I arrived at UCL — nothing. JonathanTennyson London, July2004 May18,2005 12:24 WSPC/SPI-B267:AstronomicalSpectroscopy fm CONTENTS Preface v 1. WhyRecordSpectraofAstronomicalObjects? 1 1.1 AHistoricalIntroduction . . . . . . . . . . . . . . . . . . . . 1 1.2 WhatOneCanLearnfromStudyingSpectra . . . . . . . . . 3 2. TheNatureofSpectra 7 2.1 Transitions . . . . . . . . . . . . . . . . . . . . . . . . . . . . 7 2.2 AbsorptionandEmission . . . . . . . . . . . . . . . . . . . . 8 2.3 OtherMeasuresofTransitionProbabilities . . . . . . . . . . 10 2.4 StimulatedEmission . . . . . . . . . . . . . . . . . . . . . . . 10 2.5 OpticalDepth . . . . . . . . . . . . . . . . . . . . . . . . . . 11 2.6 CriticalDensity. . . . . . . . . . . . . . . . . . . . . . . . . . 12 2.7 WavelengthorFrequency? . . . . . . . . . . . . . . . . . . . 13 2.8 TheElectromagneticSpectrum . . . . . . . . . . . . . . . . . 14 3. AtomicHydrogen 17 3.1 Overview . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17 3.2 TheSchro¨dingerEquationofHydrogen-LikeAtoms . . . . 17 3.3 ReducedMass . . . . . . . . . . . . . . . . . . . . . . . . . . 18 3.4 AtomicUnits . . . . . . . . . . . . . . . . . . . . . . . . . . . 19 3.5 WavefunctionsforHydrogen. . . . . . . . . . . . . . . . . . 20 3.6 EnergyLevelsandQuantumNumbers . . . . . . . . . . . . 21 3.7 H-AtomDiscreteSpectra . . . . . . . . . . . . . . . . . . . . 23 vii May18,2005 12:24 WSPC/SPI-B267:AstronomicalSpectroscopy fm viii AstronomicalSpectroscopy 3.8 H-AtomSpectrainDifferentLocations . . . . . . . . . . . . 30 3.8.1 Balmerseries . . . . . . . . . . . . . . . . . . . . . . . 30 3.8.2 Lymanseries . . . . . . . . . . . . . . . . . . . . . . . 33 3.8.3 Infraredlines . . . . . . . . . . . . . . . . . . . . . . . 34 3.9 H-AtomContinuumSpectra . . . . . . . . . . . . . . . . . . 35 3.9.1 Processes . . . . . . . . . . . . . . . . . . . . . . . . . 35 3.9.2 H-atomemissioninHIIregions . . . . . . . . . . . . 36 3.10 RadioRecombinationLines. . . . . . . . . . . . . . . . . . . 38 3.11 RadioRecombinationLinesforOtherAtoms . . . . . . . . 40 3.12 AngularMomentumCouplingintheHydrogenAtom . . . 43 3.13 TheFineStructureofHydrogen . . . . . . . . . . . . . . . . 44 3.14 HyperfineStructureintheHAtom . . . . . . . . . . . . . . 46 3.15 AllowedTransitions . . . . . . . . . . . . . . . . . . . . . . . 47 3.16 HydrogeninNebulae . . . . . . . . . . . . . . . . . . . . . . 48 4. ComplexAtoms 51 4.1 GeneralConsiderations . . . . . . . . . . . . . . . . . . . . . 51 4.2 CentralFieldModel . . . . . . . . . . . . . . . . . . . . . . . 52 4.3 IndistinguishableParticles . . . . . . . . . . . . . . . . . . . 54 4.4 ElectronConfigurations . . . . . . . . . . . . . . . . . . . . . 55 4.5 ThePeriodicTable . . . . . . . . . . . . . . . . . . . . . . . . 57 4.6 Ions . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58 4.7 AngularMomentuminComplexAtoms . . . . . . . . . . . 59 4.7.1 L–SorRussell–Saunderscoupling . . . . . . . . . . . 60 4.7.2 j–jcoupling . . . . . . . . . . . . . . . . . . . . . . . . 61 4.7.3 Whytwocouplingschemes? . . . . . . . . . . . . . . 62 4.8 SpectroscopicNotation . . . . . . . . . . . . . . . . . . . . . 62 4.9 ParityoftheWavefunction . . . . . . . . . . . . . . . . . . . 64 4.10 TermsandLevelsinComplexAtoms . . . . . . . . . . . . . 64 5. HeliumSpectra 69 5.1 HeIandHeIISpectra . . . . . . . . . . . . . . . . . . . . . . 69 5.2 SelectionRulesforComplexAtoms . . . . . . . . . . . . . . 71 5.3 ObservingForbiddenLines . . . . . . . . . . . . . . . . . . . 74 5.4 GrotrianDiagrams . . . . . . . . . . . . . . . . . . . . . . . . 75 5.5 PotentialFeltbyElectronsinComplexAtoms . . . . . . . . 77 5.6 EmissionsofHelium-LikeIons . . . . . . . . . . . . . . . . . 78 May18,2005 12:24 WSPC/SPI-B267:AstronomicalSpectroscopy fm Contents ix 6. AlkaliAtoms 81 6.1 Sodium . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 81 6.2 Spin-OrbitInteractions . . . . . . . . . . . . . . . . . . . . . 84 6.3 FineStructureTransitions . . . . . . . . . . . . . . . . . . . . 88 6.4 AstronomicalSodiumSpectra . . . . . . . . . . . . . . . . . 89 6.5 OtherAlkaliMetal-LikeSpectra . . . . . . . . . . . . . . . . 93 7. SpectraofNebulae 99 7.1 Nebulium . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 99 7.2 TheBowenMechanism . . . . . . . . . . . . . . . . . . . . . 104 7.3 TwoValenceElectrons . . . . . . . . . . . . . . . . . . . . . . 108 7.4 AutoionisationandRecombination . . . . . . . . . . . . . . 110 8. X-RaySpectra 116 8.1 TheSolarCorona. . . . . . . . . . . . . . . . . . . . . . . . . 119 8.2 IsotopeEffects . . . . . . . . . . . . . . . . . . . . . . . . . . 120 9. MolecularStructure 124 9.1 TheBorn–OppenheimerApproximation . . . . . . . . . . . 125 9.2 ElectronicStructureofDiatomics . . . . . . . . . . . . . . . 126 9.2.1 Labellingofelectronicstates . . . . . . . . . . . . . . 128 9.2.2 Symmetry . . . . . . . . . . . . . . . . . . . . . . . . . 130 9.2.3 Statelabels . . . . . . . . . . . . . . . . . . . . . . . . 132 9.3 Schro¨dingerEquation . . . . . . . . . . . . . . . . . . . . . . 132 9.4 Fractionation . . . . . . . . . . . . . . . . . . . . . . . . . . . 137 9.5 Vibration–RotationEnergyLevels . . . . . . . . . . . . . . . 138 9.6 TemperatureEffects . . . . . . . . . . . . . . . . . . . . . . . 141 9.6.1 Rotationalstatepopulations . . . . . . . . . . . . . . 141 9.6.2 Vibrationalstatepopulations . . . . . . . . . . . . . . 143 9.6.3 Electronicstatepopulations . . . . . . . . . . . . . . 144 10. MolecularSpectra 146 10.1 SelectionRules:PureRotationalTransitions . . . . . . . . . 146 10.1.1 Isotopeeffects . . . . . . . . . . . . . . . . . . . . . . 151 10.1.2 Rotationalspectraofothermolecules . . . . . . . . . 151 10.1.3 Rotationalspectraofmolecularhydrogen . . . . . . 154 10.2 VibrationalTransitions . . . . . . . . . . . . . . . . . . . . . 155 10.2.1 Structureofthespectrum . . . . . . . . . . . . . . . . 156