中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)

中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)
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作者: [英] (J.Tennyson)
2015-01
版次: 1
ISBN: 9787301251706
定价: 41.00
装帧: 平装
开本: 16开
纸张: 胶版纸
页数: 240页
字数: 240千字
分类: 自然科学
  •   对于宇宙的观测,其信息几乎都来自于光。观测一方面要把光分解成各种成分,另一方面也要了解原子和分子的性质。《中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)》对于这两方面都进行了系统讲述。在天文光谱学的研究中,本书能够提供丰富而实用的知识。
      《中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)》适合天文学领域的研究者和研究生阅读。   (英)坦尼森,伦敦大学学院教授。 Prefacev
    1.WhyRecordSpectraofAstronomicalObjects?1
    1.1AHistoricalIntroduction...................1
    1.2WhatOneCanLearnfromStudyingSpectra........3

    2.TheNatureofSpectra7
    2.1Transitions............................7
    2.2AbsorptionandEmission...................8
    2.3OtherMeasuresofTransitionProbabilities.........10
    2.4StimulatedEmission......................10
    2.5OpticalDepth..........................11
    2.6CriticalDensity.........................12
    2.7WavelengthorFrequency?...................13
    2.8TheElectromagneticSpectrum................14

    3.AtomicHydrogen17
    3.1Overview.............................17
    3.2TheSchr¨odingerEquationofHydrogen-LikeAtoms....17
    3.3ReducedMass..........................18
    3.4AtomicUnits..........................19
    3.5WavefunctionsforHydrogen.................20
    3.6EnergyLevelsandQuantumNumbers...........21
    3.7H-AtomDiscreteSpectra....................23
    3.8H-AtomSpectrainDifferentLocations............29
    3.8.1Balmerseries......................29
    3.8.2Lymanseries......................33
    3.8.3Infraredlines......................35
    3.9H-AtomContinuumSpectra..................35
    3.9.1Processes........................35
    3.9.2H-atomemissioninHIIregions...........36
    3.10RadioRecombinationLines..................38
    3.11RadioRecombinationLinesforOtherAtoms........40
    3.12AngularMomentumCouplingintheHydrogenAtom..43
    3.13TheFineStructureofHydrogen................44
    3.14HyperfineStructureintheHAtom..............45
    3.15AllowedTransitions......................46
    3.16HydrogeninNebulae......................47

    4.ComplexAtoms51
    4.1GeneralConsiderations....................51
    4.2CentralFieldModel.......................52
    4.3IndistinguishableParticles...................54
    4.4ElectronConfigurations....................55
    4.5ThePeriodicTable.......................56
    4.6Ions................................58
    4.7AngularMomentuminComplexAtoms...........59
    4.7.1L-SorRussell-Saunderscoupling..........59
    4.7.2j-jcoupling.......................61
    4.7.3Whytwocouplingschemes?.............61
    4.8SpectroscopicNotation.....................62
    4.9ParityoftheWavefunction...................63
    4.10TermsandLevelsinComplexAtoms.............64

    5.HeliumSpectra69
    5.1HeIandHeIISpectra......................69
    5.2SelectionRulesforComplexAtoms.............71
    5.3ObservingForbiddenLines..................74
    5.4GrotrianDiagrams.......................75
    5.5PotentialFeltbyElectronsinComplexAtoms........77
    5.6EmissionsofHelium-LikeIons................78

    6.AlkaliAtoms81
    6.1Sodium..............................81
    6.2Spin-OrbitInteractions.....................84
    6.3FineStructureTransitions...................88
    6.4AstronomicalSodiumSpectra.................89
    6.5OtherAlkaliMetal-LikeSpectra................93

    7.SpectraofNebulae99
    7.1Nebulium............................100
    7.2TheBowenMechanism.....................104
    7.3TwoValenceElectrons.....................107
    7.4AutoionisationandRecombination..............109

    8.SpectrainMagneticFields115
    8.1UniformMagneticField....................116
    8.2StrongMagneticField.....................117
    8.3WeakMagneticField......................118
    8.3.1ThenormalZeemaneffect..............118
    8.3.2TheanomolousZeemaneffect............119
    8.4SpectrainMagneticField...................120

    9.X-RaySpectra123
    9.1InnerShellProcesses......................123
    9.2TheSolarCorona........................127
    9.3TheStructureofHighlyIonisedAtoms...........127
    9.4IsotopeEffects..........................131

    10.MolecularStructure135
    10.1TheBorn-OppenheimerApproximation...........136
    10.2ElectronicStructureofDiatomics...............137
    10.2.1Labellingofelectronicstates.............140
    10.2.2Symmetry........................141
    10.2.3Statelabels.......................143
    10.3Schr¨odingerEquation.....................144
    10.3.1Nuclearmotionindiatomicmolecules.......144
    10.4Fractionation...........................149
    10.5Vibration-RotationEnergyLevels..............150
    10.6TemperatureEffects.......................152
    10.6.1Rotationalstatepopulations.............152
    10.6.2Vibrationalstatepopulations.............154
    10.6.3Electronicstatepopulations.............155

    11.RotationalSpectra157
    11.1RotationalStructureofPolyatomicMolecules........157
    11.2SelectionRules:PureRotationalTransitions.........160
    11.3SelectionRules.........................161
    11.4IsotopeEffects..........................166
    11.5RotationalSpectraofOtherMolecules............166
    11.6RotationalSpectraofMolecularHydrogen.........170
    11.7MaserEmissions........................170

    12.Vibration-RotationSpectra175
    12.1VibrationsinPolyatomicMolecules.............175
    12.2VibrationalTransitions.....................177
    12.2.1Structureofthespectrum...............178
    12.2.2Isotopeeffects.....................181
    12.2.3Hydrogenmoleculevibrationalspectra.......181
    12.3AstronomicalSpectra......................183

    13.ElectronicSpectraofDiatomicMolecules187
    13.1ElectronicTransitions......................187
    13.2SelectionRules.........................188
    13.2.1Vibrationalselectionrules..............189
    13.2.2Rotationalselectionrules...............190
    13.3TransitionFrequencies.....................192
    13.4AstronomicalSpectra......................193
    13.5Non-1_ElectronicStates....................195
    SolutionstoModelProblems199
    FurtherReadingandBibliography215
    Index217
  • 内容简介:
      对于宇宙的观测,其信息几乎都来自于光。观测一方面要把光分解成各种成分,另一方面也要了解原子和分子的性质。《中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)》对于这两方面都进行了系统讲述。在天文光谱学的研究中,本书能够提供丰富而实用的知识。
      《中外物理学精品书系·天文光谱学·天文光谱的原子与分子物理学导论(英文影印 第二版)》适合天文学领域的研究者和研究生阅读。
  • 作者简介:
      (英)坦尼森,伦敦大学学院教授。
  • 目录:
    Prefacev
    1.WhyRecordSpectraofAstronomicalObjects?1
    1.1AHistoricalIntroduction...................1
    1.2WhatOneCanLearnfromStudyingSpectra........3

    2.TheNatureofSpectra7
    2.1Transitions............................7
    2.2AbsorptionandEmission...................8
    2.3OtherMeasuresofTransitionProbabilities.........10
    2.4StimulatedEmission......................10
    2.5OpticalDepth..........................11
    2.6CriticalDensity.........................12
    2.7WavelengthorFrequency?...................13
    2.8TheElectromagneticSpectrum................14

    3.AtomicHydrogen17
    3.1Overview.............................17
    3.2TheSchr¨odingerEquationofHydrogen-LikeAtoms....17
    3.3ReducedMass..........................18
    3.4AtomicUnits..........................19
    3.5WavefunctionsforHydrogen.................20
    3.6EnergyLevelsandQuantumNumbers...........21
    3.7H-AtomDiscreteSpectra....................23
    3.8H-AtomSpectrainDifferentLocations............29
    3.8.1Balmerseries......................29
    3.8.2Lymanseries......................33
    3.8.3Infraredlines......................35
    3.9H-AtomContinuumSpectra..................35
    3.9.1Processes........................35
    3.9.2H-atomemissioninHIIregions...........36
    3.10RadioRecombinationLines..................38
    3.11RadioRecombinationLinesforOtherAtoms........40
    3.12AngularMomentumCouplingintheHydrogenAtom..43
    3.13TheFineStructureofHydrogen................44
    3.14HyperfineStructureintheHAtom..............45
    3.15AllowedTransitions......................46
    3.16HydrogeninNebulae......................47

    4.ComplexAtoms51
    4.1GeneralConsiderations....................51
    4.2CentralFieldModel.......................52
    4.3IndistinguishableParticles...................54
    4.4ElectronConfigurations....................55
    4.5ThePeriodicTable.......................56
    4.6Ions................................58
    4.7AngularMomentuminComplexAtoms...........59
    4.7.1L-SorRussell-Saunderscoupling..........59
    4.7.2j-jcoupling.......................61
    4.7.3Whytwocouplingschemes?.............61
    4.8SpectroscopicNotation.....................62
    4.9ParityoftheWavefunction...................63
    4.10TermsandLevelsinComplexAtoms.............64

    5.HeliumSpectra69
    5.1HeIandHeIISpectra......................69
    5.2SelectionRulesforComplexAtoms.............71
    5.3ObservingForbiddenLines..................74
    5.4GrotrianDiagrams.......................75
    5.5PotentialFeltbyElectronsinComplexAtoms........77
    5.6EmissionsofHelium-LikeIons................78

    6.AlkaliAtoms81
    6.1Sodium..............................81
    6.2Spin-OrbitInteractions.....................84
    6.3FineStructureTransitions...................88
    6.4AstronomicalSodiumSpectra.................89
    6.5OtherAlkaliMetal-LikeSpectra................93

    7.SpectraofNebulae99
    7.1Nebulium............................100
    7.2TheBowenMechanism.....................104
    7.3TwoValenceElectrons.....................107
    7.4AutoionisationandRecombination..............109

    8.SpectrainMagneticFields115
    8.1UniformMagneticField....................116
    8.2StrongMagneticField.....................117
    8.3WeakMagneticField......................118
    8.3.1ThenormalZeemaneffect..............118
    8.3.2TheanomolousZeemaneffect............119
    8.4SpectrainMagneticField...................120

    9.X-RaySpectra123
    9.1InnerShellProcesses......................123
    9.2TheSolarCorona........................127
    9.3TheStructureofHighlyIonisedAtoms...........127
    9.4IsotopeEffects..........................131

    10.MolecularStructure135
    10.1TheBorn-OppenheimerApproximation...........136
    10.2ElectronicStructureofDiatomics...............137
    10.2.1Labellingofelectronicstates.............140
    10.2.2Symmetry........................141
    10.2.3Statelabels.......................143
    10.3Schr¨odingerEquation.....................144
    10.3.1Nuclearmotionindiatomicmolecules.......144
    10.4Fractionation...........................149
    10.5Vibration-RotationEnergyLevels..............150
    10.6TemperatureEffects.......................152
    10.6.1Rotationalstatepopulations.............152
    10.6.2Vibrationalstatepopulations.............154
    10.6.3Electronicstatepopulations.............155

    11.RotationalSpectra157
    11.1RotationalStructureofPolyatomicMolecules........157
    11.2SelectionRules:PureRotationalTransitions.........160
    11.3SelectionRules.........................161
    11.4IsotopeEffects..........................166
    11.5RotationalSpectraofOtherMolecules............166
    11.6RotationalSpectraofMolecularHydrogen.........170
    11.7MaserEmissions........................170

    12.Vibration-RotationSpectra175
    12.1VibrationsinPolyatomicMolecules.............175
    12.2VibrationalTransitions.....................177
    12.2.1Structureofthespectrum...............178
    12.2.2Isotopeeffects.....................181
    12.2.3Hydrogenmoleculevibrationalspectra.......181
    12.3AstronomicalSpectra......................183

    13.ElectronicSpectraofDiatomicMolecules187
    13.1ElectronicTransitions......................187
    13.2SelectionRules.........................188
    13.2.1Vibrationalselectionrules..............189
    13.2.2Rotationalselectionrules...............190
    13.3TransitionFrequencies.....................192
    13.4AstronomicalSpectra......................193
    13.5Non-1_ElectronicStates....................195
    SolutionstoModelProblems199
    FurtherReadingandBibliography215
    Index217
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