SlideShare una empresa de Scribd logo
1 de 9
Descargar para leer sin conexión
Born–Oppenheimer Approximation
Dr. Anjali Devi J S
Assistant Professor (Contract Faculty), Mahatma Gandhi University, Kerala
1
Max Born
• German-British physicist.
• Born in Breslau (now Wroclaw, Poland),
1882.
• Died in Göttingen, West Germany 1970.
• Professor Berlin, Cambridge, Edinburgh.
• Nobel Prize, 1954.
• One of the founders of quantum
mechanics.
• Originator of the probability interpretation
of the (square of the) wave function.
Max Born (1882-1970)
Nobel Prize for Physics (for his fundamental research in quantum mechanics)
2
J. Robert Oppenheimer
• American physicist.
• Born in New York, 1904.
• Died in Princeton 1967.
• Professor California Institute of Technology.
• Fermi award for nuclear research, 1963.
• Important contributions to nuclear physics.
• Director of the Manhattan Project 1943–1945.
Victimized as a security risk by senator Joseph
McCarthy’s Un-American Activities Committee in
1954.
• Central figure of the eponymous PBS TV series
(Oppenheimer: Sam Waterston).
J. Robert Oppenheimer 1904-1967
The Father of the atomic bomb
3
Born–Oppenheimer Approximation
• Born and Oppenheimer showed in 1927 that the nuclei in a molecule
are stationary with respect to the electrons.
The approximation states that the Schrödinger
equation for a molecule may be separated into an
electronic and a nuclear interaction.
1 pm
Nucleus
Electron
4
Consequences
To calculate energy of the molecule,
-Solve electronic Schrödinger equation
-Then add electronic energy to the inter-nuclear repulsion to get the
total internal energy.
Molecule has a shape.
Electron
1 pm
1 pm
Electron
5
Molecule has a shape.
The nuclei in a molecule see a time-averaged electron cloud. The nuclei vibrate about equilibrium points which
define the molecular geometry; this geometry can be expressed simply as the nuclear Cartesian coordinates, or
alternatively as bond lengths and angles r and a here) and dihedrals, i.e. as internal coordinates. As far as size
goes, the experimentally determined van der Waals surface encloses about 98% of the electron density of a
molecule
6
A molecule has a definite shape because unlike the electrons, the nuclei are (relatively)
stationary (since they are much more massive). If the masses of the nuclei and the electrons could
be made equal, the distinction in lethargy would be lost, and the molecular geometry would dissolve.
7
Molecule has a shape…..
In detail:
• Because of the rapid motion of the electrons compared to the nuclei
the “permanent” geometric parameters of the molecule are the
nuclear coordinates.
• The energy (and the other properties) of a molecule is a function of
the electron coordinates (E =Ψ(x, y, z of each electron);
8
Geometry Optimisation
• A geometry optimization is the process of changing the system’s
geometry ( the nuclear coordinates and potentially the lattice vectors)
to minimize the total energy of the systems.
9

Más contenido relacionado

La actualidad más candente

PRINCIPLES OF ESR
PRINCIPLES OF ESRPRINCIPLES OF ESR
PRINCIPLES OF ESR
SANTHANAM V
 
6563.nuclear models
6563.nuclear models6563.nuclear models
6563.nuclear models
akshay garg
 

La actualidad más candente (20)

Magnetic properties
Magnetic propertiesMagnetic properties
Magnetic properties
 
Mossbauer spectroscopy - Principles and applications
Mossbauer spectroscopy - Principles and applicationsMossbauer spectroscopy - Principles and applications
Mossbauer spectroscopy - Principles and applications
 
Electron Spin Resonance Spectroscopy
Electron Spin Resonance Spectroscopy Electron Spin Resonance Spectroscopy
Electron Spin Resonance Spectroscopy
 
Quantum Chemistry
Quantum ChemistryQuantum Chemistry
Quantum Chemistry
 
Term symbols
Term symbolsTerm symbols
Term symbols
 
Mossbauer spectroscopy
Mossbauer spectroscopyMossbauer spectroscopy
Mossbauer spectroscopy
 
PRINCIPLES OF ESR
PRINCIPLES OF ESRPRINCIPLES OF ESR
PRINCIPLES OF ESR
 
Mossbauer Spectroscopy
Mossbauer SpectroscopyMossbauer Spectroscopy
Mossbauer Spectroscopy
 
Nuclear chemistry B Sc III-SEM-VI
 Nuclear chemistry B Sc III-SEM-VI Nuclear chemistry B Sc III-SEM-VI
Nuclear chemistry B Sc III-SEM-VI
 
Dft presentation
Dft presentationDft presentation
Dft presentation
 
Photoelectron spectroscopy
Photoelectron spectroscopyPhotoelectron spectroscopy
Photoelectron spectroscopy
 
Intrinsic and extrinsic defects
Intrinsic and extrinsic defects Intrinsic and extrinsic defects
Intrinsic and extrinsic defects
 
Spectroscopy
SpectroscopySpectroscopy
Spectroscopy
 
Band theory of solid
Band theory of solidBand theory of solid
Band theory of solid
 
Tanabe sugano diagram
Tanabe sugano diagramTanabe sugano diagram
Tanabe sugano diagram
 
Lecture7
Lecture7Lecture7
Lecture7
 
6563.nuclear models
6563.nuclear models6563.nuclear models
6563.nuclear models
 
Hammonds postulates
Hammonds postulatesHammonds postulates
Hammonds postulates
 
Quantum course
Quantum courseQuantum course
Quantum course
 
WALSH DIAGRAM- SEMINAR TOPIC
WALSH DIAGRAM- SEMINAR TOPICWALSH DIAGRAM- SEMINAR TOPIC
WALSH DIAGRAM- SEMINAR TOPIC
 

Similar a Born–Oppenheimer Approximation.pdf

Atomic structurepadmini
Atomic structurepadminiAtomic structurepadmini
Atomic structurepadmini
ritajindal2
 
SCIENCE PRESENTATION
SCIENCE PRESENTATIONSCIENCE PRESENTATION
SCIENCE PRESENTATION
Chescaralba
 
FINAL POWERPOINT PRESENTATION
FINAL POWERPOINT PRESENTATIONFINAL POWERPOINT PRESENTATION
FINAL POWERPOINT PRESENTATION
Chescaralba
 
Understanding the atom
Understanding the atomUnderstanding the atom
Understanding the atom
Sunyata55
 

Similar a Born–Oppenheimer Approximation.pdf (20)

Atomic Theory & Structure
Atomic Theory & StructureAtomic Theory & Structure
Atomic Theory & Structure
 
Atomic Models.pptx
Atomic Models.pptxAtomic Models.pptx
Atomic Models.pptx
 
Structure Of Atom- Science Presentation
Structure Of Atom- Science PresentationStructure Of Atom- Science Presentation
Structure Of Atom- Science Presentation
 
Quantum Numbers
Quantum NumbersQuantum Numbers
Quantum Numbers
 
Lecture 5.1- Atomic Orbitals
Lecture 5.1- Atomic OrbitalsLecture 5.1- Atomic Orbitals
Lecture 5.1- Atomic Orbitals
 
Introduction
IntroductionIntroduction
Introduction
 
TRM-4.ppt
TRM-4.pptTRM-4.ppt
TRM-4.ppt
 
Atomic structurepadmini
Atomic structurepadminiAtomic structurepadmini
Atomic structurepadmini
 
Atomic structure 2
Atomic structure 2Atomic structure 2
Atomic structure 2
 
Atomic theory presentation finale
Atomic theory presentation finaleAtomic theory presentation finale
Atomic theory presentation finale
 
Atomic theory presentation finale
Atomic theory presentation finaleAtomic theory presentation finale
Atomic theory presentation finale
 
Atomic structure
Atomic structureAtomic structure
Atomic structure
 
ADVANCED NUCLEAR PHYSICS
ADVANCED NUCLEAR PHYSICSADVANCED NUCLEAR PHYSICS
ADVANCED NUCLEAR PHYSICS
 
CHAPTER 4 Structure of the Atom
CHAPTER 4Structure of the AtomCHAPTER 4Structure of the Atom
CHAPTER 4 Structure of the Atom
 
SCIENCE PRESENTATION
SCIENCE PRESENTATIONSCIENCE PRESENTATION
SCIENCE PRESENTATION
 
the building block ATOMS
the building block ATOMSthe building block ATOMS
the building block ATOMS
 
FINAL POWERPOINT PRESENTATION
FINAL POWERPOINT PRESENTATIONFINAL POWERPOINT PRESENTATION
FINAL POWERPOINT PRESENTATION
 
ATOMIC TIMELINE
ATOMIC TIMELINEATOMIC TIMELINE
ATOMIC TIMELINE
 
Chemchapt4 101015131310-phpapp02
Chemchapt4 101015131310-phpapp02Chemchapt4 101015131310-phpapp02
Chemchapt4 101015131310-phpapp02
 
Understanding the atom
Understanding the atomUnderstanding the atom
Understanding the atom
 

Más de Anjali Devi J S

Más de Anjali Devi J S (16)

Classical & Quantum Statistics
Classical & Quantum StatisticsClassical & Quantum Statistics
Classical & Quantum Statistics
 
Phase diagram
Phase diagramPhase diagram
Phase diagram
 
Coordination complexes-bonding and magnetism.pdf
Coordination complexes-bonding and magnetism.pdfCoordination complexes-bonding and magnetism.pdf
Coordination complexes-bonding and magnetism.pdf
 
1. Random walk.pdf
1. Random walk.pdf1. Random walk.pdf
1. Random walk.pdf
 
Poisson distribution
Poisson distributionPoisson distribution
Poisson distribution
 
Probability
ProbabilityProbability
Probability
 
Normal distribution
Normal distributionNormal distribution
Normal distribution
 
Binomial distribution
Binomial distributionBinomial distribution
Binomial distribution
 
Computational Chemistry- An Introduction
Computational Chemistry- An IntroductionComputational Chemistry- An Introduction
Computational Chemistry- An Introduction
 
Gamma function
Gamma functionGamma function
Gamma function
 
Lagrange multiplier
 Lagrange multiplier Lagrange multiplier
Lagrange multiplier
 
Stirling's approximation
Stirling's approximationStirling's approximation
Stirling's approximation
 
Combinatorics
CombinatoricsCombinatorics
Combinatorics
 
Raman imaging -Anjali Devi J S
Raman imaging -Anjali Devi J SRaman imaging -Anjali Devi J S
Raman imaging -Anjali Devi J S
 
Dynamic Light Scattering Anjali Devi J S
Dynamic Light Scattering Anjali Devi J SDynamic Light Scattering Anjali Devi J S
Dynamic Light Scattering Anjali Devi J S
 
Anticancer ruthenium(ii) complexes - Anjali Devi J S
Anticancer ruthenium(ii) complexes - Anjali Devi J SAnticancer ruthenium(ii) complexes - Anjali Devi J S
Anticancer ruthenium(ii) complexes - Anjali Devi J S
 

Último

Bacterial Identification and Classifications
Bacterial Identification and ClassificationsBacterial Identification and Classifications
Bacterial Identification and Classifications
Areesha Ahmad
 
Presentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptxPresentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptx
gindu3009
 
Formation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disksFormation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disks
Sérgio Sacani
 
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 bAsymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Sérgio Sacani
 
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic  data.pptxSeismic Method Estimate velocity from seismic  data.pptx
Seismic Method Estimate velocity from seismic data.pptx
AlMamun560346
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Sérgio Sacani
 
Pests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdfPests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdf
PirithiRaju
 

Último (20)

Bacterial Identification and Classifications
Bacterial Identification and ClassificationsBacterial Identification and Classifications
Bacterial Identification and Classifications
 
VIRUSES structure and classification ppt by Dr.Prince C P
VIRUSES structure and classification ppt by Dr.Prince C PVIRUSES structure and classification ppt by Dr.Prince C P
VIRUSES structure and classification ppt by Dr.Prince C P
 
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43bNightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b
 
Presentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptxPresentation Vikram Lander by Vedansh Gupta.pptx
Presentation Vikram Lander by Vedansh Gupta.pptx
 
Isotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on IoIsotopic evidence of long-lived volcanism on Io
Isotopic evidence of long-lived volcanism on Io
 
Botany 4th semester file By Sumit Kumar yadav.pdf
Botany 4th semester file By Sumit Kumar yadav.pdfBotany 4th semester file By Sumit Kumar yadav.pdf
Botany 4th semester file By Sumit Kumar yadav.pdf
 
Formation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disksFormation of low mass protostars and their circumstellar disks
Formation of low mass protostars and their circumstellar disks
 
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
❤Jammu Kashmir Call Girls 8617697112 Personal Whatsapp Number 💦✅.
 
Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency
Hire 💕 9907093804 Hooghly Call Girls Service Call Girls AgencyHire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency
Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency
 
Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...
Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...
Vip profile Call Girls In Lonavala 9748763073 For Genuine Sex Service At Just...
 
CELL -Structural and Functional unit of life.pdf
CELL -Structural and Functional unit of life.pdfCELL -Structural and Functional unit of life.pdf
CELL -Structural and Functional unit of life.pdf
 
Biological Classification BioHack (3).pdf
Biological Classification BioHack (3).pdfBiological Classification BioHack (3).pdf
Biological Classification BioHack (3).pdf
 
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
High Class Escorts in Hyderabad ₹7.5k Pick Up & Drop With Cash Payment 969456...
 
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 bAsymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b
 
GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)GBSN - Microbiology (Unit 2)
GBSN - Microbiology (Unit 2)
 
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...
 
Seismic Method Estimate velocity from seismic data.pptx
Seismic Method Estimate velocity from seismic  data.pptxSeismic Method Estimate velocity from seismic  data.pptx
Seismic Method Estimate velocity from seismic data.pptx
 
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroidsHubble Asteroid Hunter III. Physical properties of newly found asteroids
Hubble Asteroid Hunter III. Physical properties of newly found asteroids
 
Pests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdfPests of mustard_Identification_Management_Dr.UPR.pdf
Pests of mustard_Identification_Management_Dr.UPR.pdf
 
Botany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdfBotany 4th semester series (krishna).pdf
Botany 4th semester series (krishna).pdf
 

Born–Oppenheimer Approximation.pdf

  • 1. Born–Oppenheimer Approximation Dr. Anjali Devi J S Assistant Professor (Contract Faculty), Mahatma Gandhi University, Kerala 1
  • 2. Max Born • German-British physicist. • Born in Breslau (now Wroclaw, Poland), 1882. • Died in Göttingen, West Germany 1970. • Professor Berlin, Cambridge, Edinburgh. • Nobel Prize, 1954. • One of the founders of quantum mechanics. • Originator of the probability interpretation of the (square of the) wave function. Max Born (1882-1970) Nobel Prize for Physics (for his fundamental research in quantum mechanics) 2
  • 3. J. Robert Oppenheimer • American physicist. • Born in New York, 1904. • Died in Princeton 1967. • Professor California Institute of Technology. • Fermi award for nuclear research, 1963. • Important contributions to nuclear physics. • Director of the Manhattan Project 1943–1945. Victimized as a security risk by senator Joseph McCarthy’s Un-American Activities Committee in 1954. • Central figure of the eponymous PBS TV series (Oppenheimer: Sam Waterston). J. Robert Oppenheimer 1904-1967 The Father of the atomic bomb 3
  • 4. Born–Oppenheimer Approximation • Born and Oppenheimer showed in 1927 that the nuclei in a molecule are stationary with respect to the electrons. The approximation states that the Schrödinger equation for a molecule may be separated into an electronic and a nuclear interaction. 1 pm Nucleus Electron 4
  • 5. Consequences To calculate energy of the molecule, -Solve electronic Schrödinger equation -Then add electronic energy to the inter-nuclear repulsion to get the total internal energy. Molecule has a shape. Electron 1 pm 1 pm Electron 5
  • 6. Molecule has a shape. The nuclei in a molecule see a time-averaged electron cloud. The nuclei vibrate about equilibrium points which define the molecular geometry; this geometry can be expressed simply as the nuclear Cartesian coordinates, or alternatively as bond lengths and angles r and a here) and dihedrals, i.e. as internal coordinates. As far as size goes, the experimentally determined van der Waals surface encloses about 98% of the electron density of a molecule 6
  • 7. A molecule has a definite shape because unlike the electrons, the nuclei are (relatively) stationary (since they are much more massive). If the masses of the nuclei and the electrons could be made equal, the distinction in lethargy would be lost, and the molecular geometry would dissolve. 7 Molecule has a shape…..
  • 8. In detail: • Because of the rapid motion of the electrons compared to the nuclei the “permanent” geometric parameters of the molecule are the nuclear coordinates. • The energy (and the other properties) of a molecule is a function of the electron coordinates (E =Ψ(x, y, z of each electron); 8
  • 9. Geometry Optimisation • A geometry optimization is the process of changing the system’s geometry ( the nuclear coordinates and potentially the lattice vectors) to minimize the total energy of the systems. 9