The document provides information on rotational spectroscopy and the rotational spectra of molecules. It discusses key topics like:
1) Classification of molecules as linear, symmetric top, spherical top, and asymmetric top based on their moments of inertia.
2) The rigid rotor model and how it leads to quantized rotational energy levels expressed by the rotational constant B.
3) The selection rule for rotational transitions of ΔJ = ±1, which results in a series of equally spaced spectral lines.
4) Factors that determine the intensity of rotational lines, including Boltzmann distribution of molecular populations and degeneracy of energy levels.
This document provides an introduction to molecular spectroscopy and rotational spectroscopy. It discusses how electromagnetic radiation interacts with molecules to produce absorption or emission spectra. Rotational spectroscopy specifically analyzes the microwave spectra produced when molecules absorb microwave radiation, undergoing rotational transitions between energy levels. The frequency differences between lines in the rotational spectra are directly related to the rotational constant of the molecule.
The document summarizes the Franck-Condon principle, which states that during an electronic transition between two states of a molecule, the transition occurs so rapidly that the positions of the nuclei remain almost unchanged. It describes the different types of molecular energy levels and vibrational transitions. It also provides three cases that illustrate how the Franck-Condon principle determines the relative intensities of vibrational transitions between electronic states based on differences in the equilibrium internuclear distances of the states.
This document provides an overview of electron spectroscopy techniques, including X-ray photoelectron spectroscopy (XPS), Auger electron spectroscopy (AES), and ultraviolet photoelectron spectroscopy (UPS). It discusses the basic principles, instrumentation, applications, and advantages/limitations of each technique. XPS is described as using X-rays to eject core electrons and measure their kinetic energy to determine elemental composition. AES uses electrons to eject core electrons which cause additional electrons to fall into the vacancy, emitting energy measured to identify elements. UPS uses UV light to eject valence electrons and measure their kinetic energy to determine molecular orbital energies.
This document discusses electron diffraction and neutron diffraction techniques. Electron diffraction works by firing electrons at a crystal sample and observing the interference pattern of diffracted electrons. This allows determining atomic structure. Neutron diffraction also determines atomic structure by firing neutrons at samples and observing diffraction patterns. Key advantages of neutron diffraction are its ability to locate light atoms and detect isotopes via nuclear scattering, and reveal magnetic structure via magnetic scattering. Both techniques provide structural information at the atomic scale but neutron diffraction can analyze bulk properties and magnetic structures.
Nuclear Quadrupole Resonance Spectroscopy (NQR) is a chemical analysis technique that detects nuclear energy level transitions in the absence of a magnetic field through the absorption of radio frequency radiation. NQR is applicable to solids due to the quadrupole moment averaging to zero in liquids and gases. The interaction between a nucleus's quadrupole moment and the electric field gradient of its surroundings results in quantized energy levels. Transitions between these levels are detected as NQR spectra and provide information about electronic structure, hybridization, and charge distribution. NQR finds applications in studying charge transfer complexes, detecting crystal imperfections, and locating land mines.
This document provides an overview of rotational and vibrational Raman spectroscopy. It begins by explaining the selection rules and energy level diagrams for pure rotational and vibrational transitions in diatomic molecules. Formulas are provided for calculating the Raman shift based on changes in rotational or vibrational quantum numbers. The positions of Stokes and anti-Stokes lines are tabulated. Applications of Raman spectroscopy such as identification of molecular structures and states, as well as detection of materials and diseases, are briefly outlined.
The document provides information on rotational spectroscopy and the rotational spectra of molecules. It discusses key topics like:
1) Classification of molecules as linear, symmetric top, spherical top, and asymmetric top based on their moments of inertia.
2) The rigid rotor model and how it leads to quantized rotational energy levels expressed by the rotational constant B.
3) The selection rule for rotational transitions of ΔJ = ±1, which results in a series of equally spaced spectral lines.
4) Factors that determine the intensity of rotational lines, including Boltzmann distribution of molecular populations and degeneracy of energy levels.
This document provides an introduction to molecular spectroscopy and rotational spectroscopy. It discusses how electromagnetic radiation interacts with molecules to produce absorption or emission spectra. Rotational spectroscopy specifically analyzes the microwave spectra produced when molecules absorb microwave radiation, undergoing rotational transitions between energy levels. The frequency differences between lines in the rotational spectra are directly related to the rotational constant of the molecule.
The document summarizes the Franck-Condon principle, which states that during an electronic transition between two states of a molecule, the transition occurs so rapidly that the positions of the nuclei remain almost unchanged. It describes the different types of molecular energy levels and vibrational transitions. It also provides three cases that illustrate how the Franck-Condon principle determines the relative intensities of vibrational transitions between electronic states based on differences in the equilibrium internuclear distances of the states.
This document provides an overview of electron spectroscopy techniques, including X-ray photoelectron spectroscopy (XPS), Auger electron spectroscopy (AES), and ultraviolet photoelectron spectroscopy (UPS). It discusses the basic principles, instrumentation, applications, and advantages/limitations of each technique. XPS is described as using X-rays to eject core electrons and measure their kinetic energy to determine elemental composition. AES uses electrons to eject core electrons which cause additional electrons to fall into the vacancy, emitting energy measured to identify elements. UPS uses UV light to eject valence electrons and measure their kinetic energy to determine molecular orbital energies.
This document discusses electron diffraction and neutron diffraction techniques. Electron diffraction works by firing electrons at a crystal sample and observing the interference pattern of diffracted electrons. This allows determining atomic structure. Neutron diffraction also determines atomic structure by firing neutrons at samples and observing diffraction patterns. Key advantages of neutron diffraction are its ability to locate light atoms and detect isotopes via nuclear scattering, and reveal magnetic structure via magnetic scattering. Both techniques provide structural information at the atomic scale but neutron diffraction can analyze bulk properties and magnetic structures.
Nuclear Quadrupole Resonance Spectroscopy (NQR) is a chemical analysis technique that detects nuclear energy level transitions in the absence of a magnetic field through the absorption of radio frequency radiation. NQR is applicable to solids due to the quadrupole moment averaging to zero in liquids and gases. The interaction between a nucleus's quadrupole moment and the electric field gradient of its surroundings results in quantized energy levels. Transitions between these levels are detected as NQR spectra and provide information about electronic structure, hybridization, and charge distribution. NQR finds applications in studying charge transfer complexes, detecting crystal imperfections, and locating land mines.
This document provides an overview of rotational and vibrational Raman spectroscopy. It begins by explaining the selection rules and energy level diagrams for pure rotational and vibrational transitions in diatomic molecules. Formulas are provided for calculating the Raman shift based on changes in rotational or vibrational quantum numbers. The positions of Stokes and anti-Stokes lines are tabulated. Applications of Raman spectroscopy such as identification of molecular structures and states, as well as detection of materials and diseases, are briefly outlined.
The document discusses different types of molecular energies including electronic, vibrational, rotational, and translational energies. It then describes different molecular spectroscopy techniques based on the type of transition observed, including rotational, vibrational, electronic, Raman, nuclear magnetic resonance, and electron spin resonance spectroscopy. Key details about absorption spectroscopy and chromophores/auxochromes are provided. Molecular spectroscopy techniques analyze the spectra produced during transitions between different molecular energy levels to study molecular structure and interactions.
For UG students of All Engineering Branches (Mechanical Engg., Chemical Engg., Instrumentation Engg., Food Technology) and PG students of Chemistry, Physics, Biochemistry, Pharmacy
The link of the video lecture at YouTube is
https://www.youtube.com/watch?v=t3QDG8ZIX-8
This document provides an overview of molecular spectroscopy techniques, including rotational spectroscopy, vibrational spectroscopy, and absorption and emission spectroscopy. Rotational spectroscopy uses microwave spectroscopy to study the quantized rotational energy levels of molecules. Vibrational spectroscopy uses infrared spectroscopy to analyze the quantized vibrational energy levels of bonds as they stretch, bend, and vibrate. Absorption and emission spectroscopy examines how molecules absorb and emit photons during electronic transitions between energy levels.
This document provides an overview of the unit on molecular spectroscopy that will be covered in 14 lectures. It discusses the interaction of electromagnetic radiation with matter and the different types of molecular motion and spectra. Key topics covered include the characteristics of electromagnetic radiation, types of spectra, energy level diagrams indicating electronic, vibrational and rotational transitions, conditions for pure rotational and vibrational spectra, selection rules, and applications of microwave and infrared spectroscopy. Identification methods for compounds, both classical and instrumental, are also mentioned.
This document provides an overview of Fourier transform infrared (FT-IR) spectroscopy. It discusses the electromagnetic spectrum and how infrared radiation lies between visible light and microwaves. Infrared spectroscopy works by detecting the vibrations of bonds between atoms in molecules as they absorb infrared light. An FT-IR uses an interferometer to measure an infrared spectrum with advantages of high sensitivity, accuracy, and resolution compared to other methods. The document outlines applications of infrared spectroscopy such as pharmaceutical analysis and environmental monitoring.
The document provides an introduction to nuclear chemistry, which deals with the study of atomic nuclei and nuclear reactions. It discusses the composition of nuclei, which contain protons and neutrons. The number of protons defines the element, while the total number of protons and neutrons is the mass number. The document also summarizes two nuclear models - the nuclear shell model, which proposes protons and neutrons exist in shells, and the liquid drop model, which views the nucleus as a homogeneous drop with short-range nuclear forces. Examples of nuclear reactions like alpha-induced and proton-induced reactions are also briefly described.
Mossbauer spectroscopy involves the resonant absorption and emission of gamma rays between atomic nuclei bound in a solid material. It can provide information about the chemical and electronic environment of atomic nuclei. The document discusses the basic principles, instrumentation, and analysis of Mossbauer spectroscopy. Key applications include determining chemical shifts, quadrupole splitting, magnetic properties, and using these parameters to study chemical bonding, structure, and biochemical systems.
Rotational spectroscopy measures the energies of rotational states of molecules. It can observe the rotation of polar molecules using microwave or infrared spectroscopy, and of non-polar molecules using Raman spectroscopy. Molecules can be modeled as rigid or non-rigid rotors. Diatomic and linear molecules can be modeled as rigid rotors, while distortions are accounted for in non-rigid rotor models. Vibrational states are modeled as harmonic oscillators, though anharmonicity is considered. Rotational and vibrational states are quantized, and selection rules apply to rotational-vibrational transitions.
Hyperfine splitting occurs due to the interaction between an electron's spin and the nucleus' spin. This interaction causes each electron spin state to split into 2I+1 levels, where I is the nuclear spin quantum number. As examples, the document discusses the hyperfine splitting in hydrogen, where the nuclear spin is 1/2, and deuterium, where the nuclear spin is 1. Hyperfine splitting has applications in radio astronomy, nuclear technology such as laser isotope separation, and atomic clocks.
Mossbauer spectroscopy - Principles and applicationsSANTHANAM V
Mossbauer spectroscopy involves the absorption of gamma ray photons by atomic nuclei. It can provide information about chemical environments and oxidation states. The document discusses key principles such as recoil effect, Doppler tuning, conditions required for Mossbauer spectra, instrumentation, and information that can be obtained from isomer shift, quadruple splitting, and magnetic interactions. Iron-57 is the most commonly studied isotope due to its suitable nuclear properties and applications in chemistry, mineralogy, and biology.
Partition function indicates the mode of distribution of particles in various energy states. It plays a role similar to the wave function of the quantum mechanics,which contains all the dynamical information about the system.
Electronic spectra of metal complexes-1SANTHANAM V
This document discusses electronic spectra of metal complexes. It begins by relating the observed color of complexes to the light absorbed and corresponding wavelength ranges. It then discusses the use of electronic spectra to determine d-d transition energies and the factors that affect d orbital energies. Key terms like states, microstates, and quantum numbers are introduced. Configuration, inter-electronic repulsions described by Racah parameters, nephelauxetic effect, and spin-orbit coupling are explained as factors that determine the splitting of energy levels. Russell-Saunders and j-j coupling are outlined as approaches to describe spin-orbit interactions in light and heavy elements respectively.
The document discusses nuclear chemistry and nuclear reactions. It defines nuclear chemistry as the study of nuclear changes in atoms, which are the source of radioactivity and nuclear power. There are two main types of nuclear reactions - artificial transmutation induced by bombarding atoms and natural transmutation that occurs spontaneously. Nuclear fission and fusion reactions are also described, where fission is the splitting of heavy nuclei and fusion is the combining of light nuclei. Key components of nuclear reactors like fuel, moderator, control rods and coolants are outlined. The document also discusses atomic bombs and how they work by achieving supercritical mass through compressing or combining subcritical masses. Applications of radioisotopes as tracers in chemical investigations are briefly mentioned.
This document discusses neutron diffraction and its applications. Neutron diffraction uses neutron scattering to determine the atomic and magnetic structure of materials. Neutrons can be scattered through both nuclear scattering via interaction with atomic nuclei, and magnetic scattering via interaction of the neutron's magnetic moment with the magnetic moments of atoms. This allows neutron diffraction to probe both atomic structure and magnetic ordering. Some key advantages of neutron diffraction are that neutrons are highly penetrating, non-destructive, and sensitive to light atoms. This technique is widely used to determine crystal and magnetic structures.
This document discusses molecular spectroscopy and the interaction of electromagnetic radiation with matter. It covers the characteristics of electromagnetic radiation and the different regions of the electromagnetic spectrum. It also describes molecular energy levels and the types of molecular spectra, including pure rotational, vibrational rotational, electronic band, and Raman spectra. Formulas are given for rotational and vibrational energy levels of diatomic molecules as well as selection rules and intensities of rotational spectral lines.
This document summarizes electronic spectroscopy of diatomic molecules. It discusses:
1) The Born-Oppenheimer approximation which treats electronic, vibrational, and rotational energies as independent.
2) Vibrational transitions produce a "coarse structure" spectrum and rotational transitions a "fine structure".
3) The Franck-Condon principle which states that electronic transitions occur rapidly without changes in internuclear distance, leading to vertical transitions between vibrational levels.
4) Dissociation of electronically excited molecules and the relationship between dissociation energies and excitation energies.
The document discusses different types of molecular energies including electronic, vibrational, rotational, and translational energies. It then describes different molecular spectroscopy techniques based on the type of transition observed, including rotational, vibrational, electronic, Raman, nuclear magnetic resonance, and electron spin resonance spectroscopy. Key details about absorption spectroscopy and chromophores/auxochromes are provided. Molecular spectroscopy techniques analyze the spectra produced during transitions between different molecular energy levels to study molecular structure and interactions.
For UG students of All Engineering Branches (Mechanical Engg., Chemical Engg., Instrumentation Engg., Food Technology) and PG students of Chemistry, Physics, Biochemistry, Pharmacy
The link of the video lecture at YouTube is
https://www.youtube.com/watch?v=t3QDG8ZIX-8
This document provides an overview of molecular spectroscopy techniques, including rotational spectroscopy, vibrational spectroscopy, and absorption and emission spectroscopy. Rotational spectroscopy uses microwave spectroscopy to study the quantized rotational energy levels of molecules. Vibrational spectroscopy uses infrared spectroscopy to analyze the quantized vibrational energy levels of bonds as they stretch, bend, and vibrate. Absorption and emission spectroscopy examines how molecules absorb and emit photons during electronic transitions between energy levels.
This document provides an overview of the unit on molecular spectroscopy that will be covered in 14 lectures. It discusses the interaction of electromagnetic radiation with matter and the different types of molecular motion and spectra. Key topics covered include the characteristics of electromagnetic radiation, types of spectra, energy level diagrams indicating electronic, vibrational and rotational transitions, conditions for pure rotational and vibrational spectra, selection rules, and applications of microwave and infrared spectroscopy. Identification methods for compounds, both classical and instrumental, are also mentioned.
This document provides an overview of Fourier transform infrared (FT-IR) spectroscopy. It discusses the electromagnetic spectrum and how infrared radiation lies between visible light and microwaves. Infrared spectroscopy works by detecting the vibrations of bonds between atoms in molecules as they absorb infrared light. An FT-IR uses an interferometer to measure an infrared spectrum with advantages of high sensitivity, accuracy, and resolution compared to other methods. The document outlines applications of infrared spectroscopy such as pharmaceutical analysis and environmental monitoring.
The document provides an introduction to nuclear chemistry, which deals with the study of atomic nuclei and nuclear reactions. It discusses the composition of nuclei, which contain protons and neutrons. The number of protons defines the element, while the total number of protons and neutrons is the mass number. The document also summarizes two nuclear models - the nuclear shell model, which proposes protons and neutrons exist in shells, and the liquid drop model, which views the nucleus as a homogeneous drop with short-range nuclear forces. Examples of nuclear reactions like alpha-induced and proton-induced reactions are also briefly described.
Mossbauer spectroscopy involves the resonant absorption and emission of gamma rays between atomic nuclei bound in a solid material. It can provide information about the chemical and electronic environment of atomic nuclei. The document discusses the basic principles, instrumentation, and analysis of Mossbauer spectroscopy. Key applications include determining chemical shifts, quadrupole splitting, magnetic properties, and using these parameters to study chemical bonding, structure, and biochemical systems.
Rotational spectroscopy measures the energies of rotational states of molecules. It can observe the rotation of polar molecules using microwave or infrared spectroscopy, and of non-polar molecules using Raman spectroscopy. Molecules can be modeled as rigid or non-rigid rotors. Diatomic and linear molecules can be modeled as rigid rotors, while distortions are accounted for in non-rigid rotor models. Vibrational states are modeled as harmonic oscillators, though anharmonicity is considered. Rotational and vibrational states are quantized, and selection rules apply to rotational-vibrational transitions.
Hyperfine splitting occurs due to the interaction between an electron's spin and the nucleus' spin. This interaction causes each electron spin state to split into 2I+1 levels, where I is the nuclear spin quantum number. As examples, the document discusses the hyperfine splitting in hydrogen, where the nuclear spin is 1/2, and deuterium, where the nuclear spin is 1. Hyperfine splitting has applications in radio astronomy, nuclear technology such as laser isotope separation, and atomic clocks.
Mossbauer spectroscopy - Principles and applicationsSANTHANAM V
Mossbauer spectroscopy involves the absorption of gamma ray photons by atomic nuclei. It can provide information about chemical environments and oxidation states. The document discusses key principles such as recoil effect, Doppler tuning, conditions required for Mossbauer spectra, instrumentation, and information that can be obtained from isomer shift, quadruple splitting, and magnetic interactions. Iron-57 is the most commonly studied isotope due to its suitable nuclear properties and applications in chemistry, mineralogy, and biology.
Partition function indicates the mode of distribution of particles in various energy states. It plays a role similar to the wave function of the quantum mechanics,which contains all the dynamical information about the system.
Electronic spectra of metal complexes-1SANTHANAM V
This document discusses electronic spectra of metal complexes. It begins by relating the observed color of complexes to the light absorbed and corresponding wavelength ranges. It then discusses the use of electronic spectra to determine d-d transition energies and the factors that affect d orbital energies. Key terms like states, microstates, and quantum numbers are introduced. Configuration, inter-electronic repulsions described by Racah parameters, nephelauxetic effect, and spin-orbit coupling are explained as factors that determine the splitting of energy levels. Russell-Saunders and j-j coupling are outlined as approaches to describe spin-orbit interactions in light and heavy elements respectively.
The document discusses nuclear chemistry and nuclear reactions. It defines nuclear chemistry as the study of nuclear changes in atoms, which are the source of radioactivity and nuclear power. There are two main types of nuclear reactions - artificial transmutation induced by bombarding atoms and natural transmutation that occurs spontaneously. Nuclear fission and fusion reactions are also described, where fission is the splitting of heavy nuclei and fusion is the combining of light nuclei. Key components of nuclear reactors like fuel, moderator, control rods and coolants are outlined. The document also discusses atomic bombs and how they work by achieving supercritical mass through compressing or combining subcritical masses. Applications of radioisotopes as tracers in chemical investigations are briefly mentioned.
This document discusses neutron diffraction and its applications. Neutron diffraction uses neutron scattering to determine the atomic and magnetic structure of materials. Neutrons can be scattered through both nuclear scattering via interaction with atomic nuclei, and magnetic scattering via interaction of the neutron's magnetic moment with the magnetic moments of atoms. This allows neutron diffraction to probe both atomic structure and magnetic ordering. Some key advantages of neutron diffraction are that neutrons are highly penetrating, non-destructive, and sensitive to light atoms. This technique is widely used to determine crystal and magnetic structures.
This document discusses molecular spectroscopy and the interaction of electromagnetic radiation with matter. It covers the characteristics of electromagnetic radiation and the different regions of the electromagnetic spectrum. It also describes molecular energy levels and the types of molecular spectra, including pure rotational, vibrational rotational, electronic band, and Raman spectra. Formulas are given for rotational and vibrational energy levels of diatomic molecules as well as selection rules and intensities of rotational spectral lines.
This document summarizes electronic spectroscopy of diatomic molecules. It discusses:
1) The Born-Oppenheimer approximation which treats electronic, vibrational, and rotational energies as independent.
2) Vibrational transitions produce a "coarse structure" spectrum and rotational transitions a "fine structure".
3) The Franck-Condon principle which states that electronic transitions occur rapidly without changes in internuclear distance, leading to vertical transitions between vibrational levels.
4) Dissociation of electronically excited molecules and the relationship between dissociation energies and excitation energies.
Describe the Schroedinger wavefunctions and energies of electrons in an atom leading to the 3 quantum numbers. These can be also observed in the line spectra of atoms.
ir spectroscopy: introduction modes of vibration, selection rule, factor, influcing of vibration, scaning of ir spectroscopy(instrumentation) vibration frequency of organic and inorganic compound
Rotational spectroscopy deals with the rotational energy transitions of molecules using microwave or far infrared radiation. When radiation of the proper frequency interacts with a rotating molecule, it can cause transitions between different rotational energy levels within the same vibrational state. This produces a pure rotational spectrum. The spectrum provides information about molecular parameters like the rotational constant. Only molecules with a dipole moment can interact with electromagnetic radiation and be observed spectroscopically. Replacement of one atom with its isotope changes the molecular moment of inertia slightly, resulting in a small measurable shift in the rotational transition frequencies.
This document discusses electromagnetic radiation and the wave-particle duality of light. It explains that electromagnetic radiation travels as waves with characteristics of wavelength and frequency. The energy of individual photons is related to their frequency by Planck's constant. Electrons in atoms can only occupy certain allowed energy levels, absorbing or emitting photons of specific frequencies as they transition between levels. This explains atomic emission spectra and helped develop the theories of quantum mechanics.
This document contains a summary of several physics concepts related to wave-particle duality and quantum physics. It includes 3 sample problems worked out in detail that demonstrate: 1) using the Compton scattering equation to estimate the Compton wavelength from experimental data, 2) relating the number of photons emitted by a laser to its power and photon energy, and 3) calculating the energy of the most energetic electron in uranium using the particle in a box model. The worked problems provide insight into applying relevant equations and show the conceptual and mathematical steps.
This document provides information about quantum theory and atomic structure:
- It introduces the wave nature of light and electromagnetic radiation, including frequency, wavelength, and speed of light.
- Models of the atom are discussed, from the Bohr model to the quantum mechanical model using the Schrodinger wave equation.
- Key concepts in quantum theory are explained, such as quantization of energy, photons, wave-particle duality, and the Heisenberg uncertainty principle.
- Atomic orbitals are described using quantum numbers such as principal, angular momentum, and magnetic, and how these relate to electron configuration.
This document provides an overview of the development of atomic models over time, including:
- Thomson's model which depicted the atom as a uniform sphere of positive charge with electrons embedded within it.
- Rutherford's model based on his gold foil experiment, which determined that the positive charge and nearly all of the mass of the atom are concentrated in a very small, dense nucleus at the center.
- Bohr's model built on Rutherford's by proposing that electrons orbit the nucleus in fixed, quantized energy levels. It helped explain atomic emission spectra but had limitations.
- Later developments including Planck's quantum theory, de Broglie's hypothesis of matter waves, Heisenberg's uncertainty principle
Infrared spectroscopy analyzes the interaction of infrared radiation with matter. The IR spectrum provides information about a compound's chemical structure and molecular structure by measuring the absorption of IR radiation. IR spectroscopy is widely used to analyze organic materials. An IR spectrum results from molecular vibrations that cause changes in the dipole moment. Absorption bands in the fingerprint region from 1300-400 cm-1 are characteristic of the whole molecule and useful for identification.
This document summarizes an experiment that uses Fourier-Transform infrared spectroscopy to determine molecular characteristics of various molecules. It analyzes carbon monoxide, greenhouse gases NO2 and CH4, and molecular iodine. For carbon monoxide, it determines molecular constants and finds it acts more like a harmonic oscillator. For NO2 and CH4, it calculates their global warming potentials and finds NO2 is a more effective greenhouse gas. For molecular iodine, it obtains molecular constants for the X-State and B-State and finds the expected relationship between equilibrium bond length and vibrational energy.
This document discusses atomic structure and periodicity. It begins by explaining electromagnetic radiation and its wave characteristics. It then discusses Planck's discovery that energy is quantized and Einstein's proposal that light can be viewed as particles called photons. Next, it explains the photoelectric effect and how it provided evidence that light behaves as particles. It discusses the Bohr model of the hydrogen atom and how it correctly predicted the atom's quantized energy levels but was fundamentally incorrect. Finally, it summarizes the development of the modern quantum mechanical model of the atom and periodic trends in atomic properties such as ionization energy and atomic radius.
Infrared spectroscopy involves measuring the absorption of infrared radiation by a sample. The infrared spectrum produced provides information about the chemical bonds and molecular structure in the sample. Common methods to obtain an infrared spectrum include measuring absorption, emission, or reflection of infrared radiation. Infrared spectroscopy is widely used to analyze organic materials and some inorganic compounds.
1. Electronic spectroscopy relies on quantized energy states of electrons. Absorption of photons promotes electrons to excited states, and fluorescence occurs when electrons return to lower states.
2. Molecular electronic spectra involve changes in electronic, vibrational, and rotational energies of molecules. They appear in the visible and ultraviolet regions.
3. Potential energy curves describe different electronic states of diatomic molecules. Transitions between states emit or absorb radiation and give rise to band systems consisting of vibrational and rotational transitions within those bands.
This document discusses the development of atomic structure models from the early 20th century to the present. It describes experiments that showed light and matter have both wave-like and particle-like properties. This led to the development of quantum mechanics and quantum numbers to describe electron orbitals. The Bohr model of the hydrogen atom was an early success but did not apply to other atoms. Modern quantum mechanics uses probability distributions and accounts for electron spin and the Pauli exclusion principle.
09 UNIT-9(Electronics and down of Modern Physics) (1).pptxFatimaAfzal56
The document summarizes key concepts from a lecture on electronics and modern physics:
- Rectification converts alternating current to direct current using diodes in half-wave or full-wave configurations. Full-wave rectification uses two diodes or a bridge rectifier circuit to rectify both halves of the input cycle.
- Blackbody radiation is electromagnetic radiation that follows Planck's law and depends on the temperature of the blackbody. The Stefan-Boltzmann law states that a blackbody's total emissive power is directly proportional to the fourth power of its thermodynamic temperature.
- Photoelectric effect experiments provided evidence that light behaves as quantized packets of energy called photons, as described by Einstein's photo
Benzamide and Phenyl Acetate both contain a C=O bond. However, their IR spectra show differences in the C=O stretching frequency:
- Benzamide shows C=O stretching absorption around 1650 cm-1. This is due to resonance stabilization of the C=O bond by the adjacent NH group. The conjugation lowers the force constant and hence decreases the C=O stretching frequency.
- Phenyl Acetate shows C=O stretching absorption around 1730-1750 cm-1. This is higher than benzamide since there is no conjugation or resonance effects in phenyl acetate to stabilize and weaken the C=O bond.
So in summary, the lower frequency of
This document discusses key concepts in quantum mechanics including:
- Planck's quantum theory which established that atoms can only emit or absorb energy in discrete quanta.
- Einstein's explanation of the photoelectric effect using the particle nature of light (photons).
- Bohr's model of the hydrogen atom which explained its spectral lines by postulating discrete electron energy levels.
- Quantum numbers which describe the state of an electron including its orbital, orientation, and spin.
- Electron configuration which shows how electrons fill atomic orbitals according to the aufbau principle.
1) The document discusses the electronic structure of atoms, including the quantization of energy and the dual wave-particle nature of light and matter.
2) It describes Max Planck's quantum theory of energy and Albert Einstein's proposal that light can be described as discrete packets called photons.
3) The emission spectrum of hydrogen atoms is discussed, showing that only certain discrete energy levels are allowed, supporting the quantum nature of the atom.
ELECTRICAL DOUBLE LAYER-TYPES-DYNAMICS OF ELECTRON TRANSFER-MARCUS THEORY-TUNNELING - BUTLER VOLMER EQUATIONS-TAFEL EQUATIONS-POLARIZATION AND OVERVOLTAGE-CORROSION AND PASSIVITY-POURBAIX AND EVAN DIAGRAM-POWER STORAGE-FUEL CELLS
NEED FOR THE SECOND LAW OF THERMODYNAMICS - STATEMENT - CARNOT CYCLE - REFRIGERATOR CONCEPT - CONCEPT OF ENTROPY - FREE ENERGY FUNCTIONS - GIBB'S HELMHOLTZ EQUATIONS - MAXEWELL'S RELATIONS - THERMODYNAMICS EQUATION OF STATE - CRITERIA OF SPONTANITY - CHEMICAL POTENTIAL - GIBB'S DUHEM EQUATION
CONDUCTIVITY-TYPES-VARIATION WITH DILUTION-KOHLRAUSCH LAW - TRANSFERENCE NUMBER -DETERMINATION - IONIC MOBILITY - APPLICATION OF CONDUCTANCE MEASUREMENTS - CONDUCTOMENTRIC TITRATION
BOHR ATOM MODEL - BOHR SOMERFIELD MODEL - de-BROGLIE DUAL NATURE OF ATOM - SCHRODINGER WAVE EQUATION -MODERN PERIODIC LAW - ELECTRONEGATIVITY SCALES - SLATER RULE - BALANCING OF REDOX EQUATIONS
1. The document discusses key concepts in thermodynamics including the zeroth law, first law, internal energy, enthalpy, heat capacities, and various thermodynamic processes.
2. It provides mathematical expressions for relating work, heat, internal energy and enthalpy based on the first law of thermodynamics.
3. The different types of thermodynamic processes like isothermal, adiabatic, isochoric and isobaric processes are defined along with their characteristic properties.
This document discusses the third law of thermodynamics. It states that the entropy of a perfectly crystalline substance is zero at absolute zero temperature. The mathematical expressions for determining absolute entropy are provided. The document also discusses Nernst's heat theorem, which states that the change in Gibbs free energy of a reaction approaches the change in enthalpy as temperature approaches absolute zero. Exceptions to the third law for certain gases with non-ordered crystal structures are also noted.
This document defines alkynes as unsaturated hydrocarbons containing a carbon-carbon triple bond. It gives examples of common alkynes like acetylene and propyne. It then describes several methods for preparing alkynes, including from calcium carbide, dehalogenation of tetrahalides, and dehydrohalogenation of vicinal dihalides. The document discusses several chemical properties of alkynes, such as forming acetylides through replacement of hydrogen atoms with sodium, undergoing ozonolysis to form diketones, being oxidized to acids, and reacting with bromine to form tetrahalides or dibromides.
Definition - Mechanism - Effect of dielectric constant on the rate of reactions in solutions - Salt effect - Primary salt effect - Bronsted – Bjerrum equation - Secondary salt effect - Effect of pressure on rate of reaction in solution - Volume of activation - Significance
Solid state chemistry- laws of crystallography- Miller indices- X ray diffraction- Bragg equation- Spectrophotometer- Determination of interplanar distance- Types of crystal
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accelerated due to factors such as agriculture and urbanization. Information regarding land use and
cover is essential for various planning and management tasks related to the Earth's surface,
providing crucial environmental data for scientific, resource management, policy purposes, and
diverse human activities.
Accurate understanding of land use and cover is imperative for the development planning
of any area. Consequently, a wide range of professionals, including earth system scientists, land
and water managers, and urban planners, are interested in obtaining data on land use and cover
changes, conversion trends, and other related patterns. The spatial dimensions of land use and
cover support policymakers and scientists in making well-informed decisions, as alterations in
these patterns indicate shifts in economic and social conditions. Monitoring such changes with the
help of Advanced technologies like Remote Sensing and Geographic Information Systems is
crucial for coordinated efforts across different administrative levels. Advanced technologies like
Remote Sensing and Geographic Information Systems
9
Changes in vegetation cover refer to variations in the distribution, composition, and overall
structure of plant communities across different temporal and spatial scales. These changes can
occur natural.
বাংলাদেশের অর্থনৈতিক সমীক্ষা ২০২৪ [Bangladesh Economic Review 2024 Bangla.pdf] কম্পিউটার , ট্যাব ও স্মার্ট ফোন ভার্সন সহ সম্পূর্ণ বাংলা ই-বুক বা pdf বই " সুচিপত্র ...বুকমার্ক মেনু 🔖 ও হাইপার লিংক মেনু 📝👆 যুক্ত ..
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তাই একজন নাগরিক হিসাবে এই তথ্য গুলো আপনার জানা প্রয়োজন ...।
বিসিএস ও ব্যাংক এর লিখিত পরীক্ষা ...+এছাড়া মাধ্যমিক ও উচ্চমাধ্যমিকের স্টুডেন্টদের জন্য অনেক কাজে আসবে ...
How to Build a Module in Odoo 17 Using the Scaffold MethodCeline George
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How to Add Chatter in the odoo 17 ERP ModuleCeline George
In Odoo, the chatter is like a chat tool that helps you work together on records. You can leave notes and track things, making it easier to talk with your team and partners. Inside chatter, all communication history, activity, and changes will be displayed.
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This presentation includes basic of PCOS their pathology and treatment and also Ayurveda correlation of PCOS and Ayurvedic line of treatment mentioned in classics.
1. Associate Professor and Head
Department of Chemistry
Saiva Bhanu Kshatriya College , Aruppukkottai 626101,
Tamilnadu ,India .
2. Molecular Spectroscopy
The study of interaction of electromagnetic radiations with matter is called
Molecular spectroscopy.
Types of Molecular spectroscopy:
Pure rotational (Microwave) spectra
Vibrational (Infrared) spectra
Electronic (UV) Spectra
Raman Spectra
Nuclear Magnetic Resonance (NMR) spectra
Electron Spin Resonance (ESR) Spectra
3. Rotational spectra of diatomic molecule
• Definition:
The interaction between rotational energy levels of a gaseous
molecule and microwave radiation causes transition between the rotational
energy levels by the absorption of microwave radiation is called rotational
spectra
• Condition:
Molecules possess permanent dipole moment shows molecular
spectra .The microwave spectra occur in the spectral range of 1-100 cm-1
• Example :
HCl , CO ,H2O , NO ,etc.
4. .Explanations :
consider a diatomic molecule rotating about its center of gravity (C.G)
.Where,
r is the bond length
m1 is the mass of one atom
m2 is the mass of another atom
r1 is the distance of the atom 1 from the CG
r2 is the distance of the atom 2 from the CG
.At center of gravity :
m1r1 = m2r2 ---------- ( 1 )
Rotational spectra of diatomic molecule
5. Rotational spectra of diatomic molecule
. The moment of inertia I of a molecule is
I = μr2 ------- (2)
where , μ = reduced mass of the molecule =
𝑚1
𝑚2
𝑚1
+𝑚2
.According to classical mechanics , the angular momentum (L) of a rotating molecule is
L = Iω ------- (3)
where , ω = angular velocities
6. Rotational spectra of diatomic molecule
.According to quantum mechanics
L = 𝐽 ( 𝐽 + 1)
ℎ
2𝜋
------- (4)
where , J = rotational quantum number = 0,1,2,3,…….
.The energy of rotating molecule is
EJ =
1
2
𝐼𝜔2 =
𝐼2
𝜔2
2𝐼
=
𝐿2
2𝐼
=
𝐽 𝐽+1
ℎ
2𝜋
2
2𝐼
EJ =
𝐽 𝐽+1 ℎ2
2𝐼4𝜋2
EJ =
ℎ2
8𝜋2
𝐼
𝐽 𝐽 + 1 ------- (5)
7. Rotational spectra of diatomic molecule
The equation (5) is divided by hc in order to express the energy in cm-1
𝐸 𝐽
ℎ𝑐
=
ℎ2
8𝜋2
𝐼ℎ𝑐
𝐽 𝐽 + 1 cm-1
EJ =
ℎ
8𝜋2
𝐼𝑐
𝐽 𝐽 + 1 cm-1 ------- (6)
EJ = BJ( J+1) cm-1 -------- (7)
Where , B =
ℎ
8𝜋2
𝐼𝐶
8. Rotational spectra of diatomic molecule
Substituting the rotational quantum number (J = 0 , 1 , 2 , 3 , ….) in the equation (7) we
gets the quantized rotational energy levels of the rotating diatomic molecule
when ; J = 0 , E0 = 0
J = 1 , E1 = 2 Bcm-1
J = 2 , E2 = 6 Bcm-1
J = 3 , E3 = 12 Bcm-1
J = 4 , E4 = 20 Bcm-1
J = 5 , E5 = 30 Bcm-1
Since the rotational energy levels falls on the microwave region , the transition between
rotational energy level takes place by the absorption of microwave radiation as per the
selection rule ΔJ = ±1
9. Rotational spectra of diatomic molecule
So, the energy for a transition
J = 0 J = 1 is
ΔE = E1 – E0
ΔE0-1= 2B – 0 = 2B ; Since ΔE = γ
γ0-1 = 2B ;where, γ is frequency in cm-1 of the microwave causes transition
Similarly for,
J = 1 J = 2 is
γ1-2 = E2 – E1
γ1-2 = 6B – 2B = 4B
Similarly ; γ2-3 = 6B , γ3-4 = 8B
10. Rotational spectra of diatomic molecule
• The rotational spectrum of a rigid diatomic molecule appear at the following rotational
frequencies 2B, 4B, 6B, 8B .etc.. And each are appeared as a lines in the detector . These lines
are equally spaced by 2B
i.e. the interspaceial distance of the spectral lines is 2B and it shown in the diagram
11. Relative intensities of rotational spectral lines
• The plot of
𝑁 𝐽
𝑁0
versus J for a rigid diatomic molecule at room temperature is
• The value of J corresponding to the maximum in population is
Jmax = (
𝑘𝑡
2ℎ𝑐𝐵
)1/2
– ½
12. Vibrational spectra of diatomic molecule
• Definition : The interaction between the vibrational energy levels of a molecule and the
infrared radiation causes transition between the vibrational energy levels by the absorption of
infrared radiation is called infrared radiation
• Condition: The vibrations of a molecule involving changes in the dipole moment are IR active.
These spectra occur in the spectral range of 500-4000 cm-1
• Example : hetero diatomic molecule like CO , NO , CN , HCl ,(dipole moment) shows changes
in dipole moment during vibration.
i.e.. Homodiatomic molecule (H2 , O2 , N2 etc.) are IR-inactive but hetero diatomic molecules
are IR-active
13. Vibrational spectra of diatomic molecule
• Explanation : consider a vibrating diatomic molecule and the vibration is assumed to be
simple harmonic vibration
Where m1 and m2 are the masses of the atoms
re = equilibrium distance
x = displacement of the atom during vibration(expansion and compression) from the
equilibrium distance
14. Vibrational spectra of diatomic molecule
• The vibrational frequency of the vibrating molecule in term of cm-1 is
γ =
1
2π𝑒
𝑘
𝜇
cm-1 ---------(1)
Where ,
k = force constant , it is the restoring force acting on the molecule in order to come to
original position during expansion and compression
μ = reduced mass =
𝑚1
𝑚2
𝑚1
+𝑚2
According to Hooke's law , the potential energy (Vx) of the vibrating molecule is a function of
‘x’
i.e.. V(x) = ½ kx2 --------(2)
where x = r - re
15. Vibrational spectra of diatomic molecule
• The plot of potential energy (Vx) versus x gives parabolic curve
On solving the Schrodinger wave equation for a simple harmonic vibrator gives the
vibrational energy level
EV = ( v + ½ )h γ ----------(3)
where v = vibrational quantum number
= 0,1,2,3,……..
γ = vibrational frequency
16. Vibrational spectra of diatomic molecule
Equation (3) is divided by hc to get the energy in cm-1
𝐸 𝑣
ℎ𝑐
= (v + ½)
ℎγ
ℎ𝑐
= (v + ½)
γ
𝑐
Ev = (v + ½) ωe -----------(4)
where ωe = equilibrium vibrational frequency
By putting the value of v in equation (4) we get the energy of various vibrational level
When ; v = 0 , E0 =
ωe
2
called zero point energy
v = 1 , E1 =
3ωe
2
; v = 2 , E2 =
5ωe
2
v = 3 , E3 =
7ωe
2
; v = 4 , E4 =
9ωe
2
v = 5 , E5 =
11ωe
2
17. Vibrational spectra of diatomic molecule
• This shows the vibration energy levels are equally spaced by ωe . Since the vibrational
energies are falling into IR region , the transition between vibrational energy levels takes
place by the absorption of IR radiation as per the selection rule Δv = +1
18. Vibrational spectra of diatomic molecule
• The energy of the IR radiation in term of cm-1 ( γ )that causes the vibrational energy
transition is equal to Ev+1 – Ev
i.e.. For v = 0 ----- v = 1 For v = 1 ----- v = 2
γ = E1 – E0 =
3ωe
2
–
ωe
2
= ωe γ = E2 – E1 =
5ωe
2
–
3ωe
2
= ωe
For v = 2 ----- v = 3 For v = 3 ----- v = 4
γ = E3 – E2 =
7ωe
2
–
5ωe
2
= ωe γ = E4 – E3 =
9ωe
2
–
7ωe
2
= ωe
This shows all vibrational energies transition as per the selection rule Δv = ±1 occurs
at only one frequency we called fundamental vibrational frequencies and gives only one
vibrational spectrum line
19. Vibrations of polyatomic molecules
• Total degree of freedom for polyatomic molecule = 3N
where N is number of atoms
• The translational degree of freedom for polyatomic molecule = 3
• The rotational degree of freedom for
linear molecule = 2
non linear molecule = 3
• So , the vibrational degree of freedom for
polyatomic linear molecule = 3N – 5
polyatomic non linear molecule = 3N – 6
20. Vibrations of polyatomic molecules
1. Linear CO2 molecule
N = 3
• The vibrational degree of freedom
= 3 N – 5
= (3 X 3) – 5
= 9 – 5
= 4
• The four types vibrations in CO2
molecule are IR active are shown
in figure
21. Vibrations of polyatomic molecules
2. Linear H2O molecule
N = 3
• The vibrational degree of freedom
= 3 N – 6
= (3 X 3) – 6
= 9 – 6
= 3
• The three types vibrations in H2O
molecule are IR active are shown in
figure
22. Electronic spectra
• Definition : The interaction between the electronic energy levels in a molecule and the
visible and ultra violet radiation causes transition between the electronic energy levels
by the absorption of the visible (or) u.v radiation is called electronic spectra
• Conditions : Components containing π – bond shows electronic spectra. The electronic
spectra in the visible region span 12,500-25,000 cm-1 ,those in the ultra violet region
span 25,000-75,000 cm-1
• Explanation :
The total energy of a molecule in the ground state is
E = Eelc + Evib + E rot --------(1)
(since Etrans is not quantized , it is not included in equation 1 )
The total energy of a molecule in the excited state is
E
,
= E
,
elc + E
,
vib + E
,
rot ---------(2)
23. Electronic spectra
• Equation (2) – (1) gives the energy required to make the electronic transition from E to
E
,
i.e.. E
,
– E = (E
,
elc – Eelc ) + (E
,
vib – Evib ) + (E
,
rot – E rot )
ΔE = ΔEelc + ΔEvib + ΔE rot ---------(3)
• Since , ΔEelc >> ΔEvib >> ΔE rot ; the two electronic states transition is accompanied by
simultaneous transition between the vibrational and rotational level.
• Divide equation (3) by hc we get the energy in terms of frequency for the electronic
transition in cm-1
ΔE
ℎ𝑐
=
ΔEelc + ΔEvib + ΔE rot
ℎ𝑐
= γ cm-1 ----------(4)
• The electronic energy levels transition will be governed by the Franck - Condon
principle
24. Electronic spectra – Franck Condon principle
• Franck Condon principle states that an electronic transition takes place without any
change in the internucler distance of the vibrating molecule .
25. Electronic spectra – Franck Condon principle
• Since the bonding in the excited state is weaker than in the ground state , the minimum in
the potential energy curve for the excited state occurs at a slightly greater internucler
distance than the corresponding minimum in the ground electronic state
• So , when a photon falls on the molecule , the most probable electronic transition according
to Franck-Condon principle is v0 ----- v
,
2 and is shown in the above diagram as 0 ----- 2
• Application : The unsaturated molecules containing C=C and C=O (aldehydes and ketone)
are identified using electronic spectrum since they shows n – π* and π – π* electronic
transition
26. Raman spectroscopy
• Definition : It is the branch of molecular spectroscopy which deals about the scattering of
light radiation by the molecules in which the scattered light radiation will have either a
higher or a lower frequency than the incident light radiation and this effect is called
Raman effect
• Diagrammatically:
• Condition : Changes in polarisability of the molecule is the condition for getting Raman
spectrum. Raman spectra are observed in the visible region, 12,500-25,000 cm-1
27. Raman spectroscopy – Quantum theory
• According to quantum theory , a photon of frequency (γ) falling on a molecule ,
collision takes place between the molecule and photon .
• If the collision is elastic , then the scattered photon will have the same energy and
same frequency as the incident radiation . This scattering is called Rayleigh
scattering
• If the collision is inelastic , the scattered photon will have either higher (or) lower
energy and frequency then the incident radiation . This scattering is called Raman
scattering
29. Raman spectroscopy – Quantum theory
• Figure b : when the molecule excited to the higher unstable vibrational energy level then
returns to the original vibrational energy level of the ground state we get Rayleigh scattering
• Figure a : when the molecule excited to the higher unstable vibrational energy level then
returns to the different vibrational energy level of the ground state we get Raman scattering
called stokes lines
• Figure c : when the molecule , initially in the first excited vibrational energy level of the
ground state is promoted to a higher unstable vibrational state and returns to the ground
state we get Raman scattering called anti stokes line
• The shifts in frequency (γ – γ
,
) is called Raman shifts and it fall in the range 100 – 4,000 cm-1
31. Application of Raman spectra
1. Using the mutual exclusion rule , it gives information about molecular vibrations which
are IR inactive
i.e.. Molecule having center of symmetry (H2 , O2 , CO2 …) IR active vibrations are Raman
inactive and IR inactive vibrations are Raman active
Example : In CO2 , the symmetric stretching vibration has no dipole moment so it is IR
inactive but it gives Raman spectra
32. Application of Raman spectra
2. The existence of cis and trans isomers in dichloro ethylene can be confirmed by
Raman's spectra
Raman active IR active
i.e.. if the compound has trans isomer only , it gives Raman spectra only but dichloro
ethylene gives both Raman and IR spectra. This indicates that the existence of cis and
trans isomers in equilibrium
33. Application of Raman spectra
3. All the vibrations for CS2 are Raman active and IR inactive . This indicates that the
structure of CS2 has center of symmetry like
4. All the vibrations for N2O are Raman active and IR active . This indicates that the
structure of N2O has no center of symmetry like
34. Experimental technique for Raman spectroscopy
• As shown in the diagram is the experimental set-up for the Raman spectroscopy
35. Experimental technique for Raman spectroscopy
Experiment :
• When a current discharge passes through the large spiral discharge tube emits intense
monochromatic radiation allowed to fall on the cell containing a gaseous (or) liquid
sample
• The scattered light is observed at right angles to the direction of incident radiation
and allowed to pass through the filter and monochromator then finally fall on the
detector
• The detector used is photographic plate
36. Pure Rotational Raman spectra
• The selection rule for Rotational Raman spectra is
ΔJ = 0 , ± 2
when
ΔJ = 0 → Rayleigh scattering
ΔJ = +2 → stokes lines
ΔJ = -2 → Anti stokes lines
Raman scattering
37. Rotation – vibration Raman spectrum
• The selection rule for Rotation - vibration
Raman spectra is Δv = +1 , ΔJ = 0 , ± 2
• The transition with Δv = +1 and ΔJ = 0
is called Q - branch lines
• The transition with Δv = +1 and ΔJ = +2
is called S - branch lines
• The transition with Δv = +1 and ΔJ = -2
is called 0 - branch lines