Lecture 5: Quantitative Emission/Absorption

Similar documents
Title: Radiative transitions and spectral broadening

Rate of Absorption and Stimulated Emission

SUPPLEMENTARY INFORMATION

Lecture 6: Diatomic gases (and others)

4. INTERACTION OF LIGHT WITH MATTER

Degenerate PT. ψ φ λψ. When two zeroth order states are degenerate (or near degenerate), cannot use simple PT.

4. Blackbody Radiation, Boltzmann Statistics, Temperature, and Thermodynamic Equilibrium

Lecture 3. Interaction of radiation with surfaces. Upcoming classes

4. INTERACTION OF LIGHT WITH MATTER

STATISTICAL MECHANICS

ECEN 5005 Crystals, Nanocrystals and Device Applications Class 19 Group Theory For Crystals

Lecture 3: Boltzmann distribution

) is the unite step-function, which signifies that the second term of the right-hand side of the

Radiation Chapter 12 L8 (MMV031) Martin Andersson

Physics 3 (PHYF144) Chap 2: Heat and the First Law of Thermodynamics System. Quantity Positive Negative

3. Be able to derive the chemical equilibrium constants from statistical mechanics.

THERMAL DISTRIBUTION IN THE HCL SPECTRUM OBJECTIVE

Atmospheric Radiation Fall 2008

A REVIEW OF ERROR ANALYSIS

Level Crossing Spectroscopy

EXAM INFORMATION. Harmonic Oscillator. Anharmonic Oscillator 1 ~ 1. Rigid Rotor

Applied Nuclear Physics (Fall 2004) Lecture 23 (12/3/04) Nuclear Reactions: Energetics and Compound Nucleus

5.04, Principles of Inorganic Chemistry II MIT Department of Chemistry Lecture 32: Vibrational Spectroscopy and the IR

Robert Eisberg Second edition CH 09 Multielectron atoms ground states and x-ray excitations

TP A SOLUTION. For an ideal monatomic gas U=3/2nRT, Since the process is at constant pressure Q = C. giving ) =1000/(5/2*8.31*10)

Physics 607 Exam 1. ( ) = 1, Γ( z +1) = zγ( z) x n e x2 dx = 1. e x2

THEOREMS OF QUANTUM MECHANICS

NAME and Section No. it is found that 0.6 mol of O

7 Stellar Structure III. introduc)on to Astrophysics, C. Bertulani, Texas A&M-Commerce 1

Introduction to Vapor/Liquid Equilibrium, part 2. Raoult s Law:

( T) Blackbody Radiation. S hν. hν exp kt MODEL

S Advanced Digital Communication (4 cr) Targets today

10/9/2003 PHY Lecture 11 1

Open Systems: Chemical Potential and Partial Molar Quantities Chemical Potential

The Geometry of Logit and Probit

Measurement of Radiation: Exposure. Purpose. Quantitative description of radiation

V. Electrostatics. Lecture 25: Diffuse double layer structure

Problem Points Score Total 100

Lecture 4. Instructor: Haipeng Luo

5.60 Thermodynamics & Kinetics Spring 2008

Econ107 Applied Econometrics Topic 3: Classical Model (Studenmund, Chapter 4)

Department of Chemistry Purdue University Garth J. Simpson

CHAPTER 5 NUMERICAL EVALUATION OF DYNAMIC RESPONSE

Introduction to Super-radiance and Laser

Frequency dependence of the permittivity

Introduction to Statistical Methods

Electrostatic Potential from Transmembrane Currents

between standard Gibbs free energies of formation for products and reactants, ΔG! R = ν i ΔG f,i, we

...Thermodynamics. If Clausius Clapeyron fails. l T (v 2 v 1 ) = 0/0 Second order phase transition ( S, v = 0)

8. Superfluid to Mott-insulator transition

Molecular Spectroscopy and Group Theory Chemistry 630 Bruce Johnson

Chemistry 163B Free Energy and Equilibrium E&R ( ch 6)

where v means the change in velocity, and t is the

Course Electron Microprobe Analysis

Lagrangian Field Theory

Influence of chemi-ionization and chemi-recombination processes on the population of hydrogen Rydberg states in atmospheres of late type dwarfs

6. Stochastic processes (2)

6. Stochastic processes (2)

Chapter 1. Probability

Characteristics of populations and gains in neon-like argon Ar IX

Randomness and Computation

Experimental Techniques for Nuclear and Particle Physics. Interactions of particles in matter (1)

Multi-dimensional Central Limit Theorem

Chapter-1. Photon interaction with matter and production of fluorescent. X-rays

5.76 Lecture #21 2/28/94 Page 1. Lecture #21: Rotation of Polyatomic Molecules I

V T for n & P = constant

If two volatile and miscible liquids are combined to form a solution, Raoult s law is not obeyed. Use the experimental data in Table 9.

Lecture 4. Macrostates and Microstates (Ch. 2 )

arxiv:astro-ph/ v1 30 Dec 1999

Röntgen s experiment in X-ray Spectroscopy. Röntgen s experiment. Interaction of x-rays x. x-rays. with matter. Wavelength: m

EXAFS. Extended X-Ray Absorption Fine Structure. Santiago J. A. Figueroa Researcher Beamline coordinator XAFS2

Investigation of a New Monte Carlo Method for the Transitional Gas Flow

Lecture 6 More on Complete Randomized Block Design (RBD)

3.1 Expectation of Functions of Several Random Variables. )' be a k-dimensional discrete or continuous random vector, with joint PMF p (, E X E X1 E X

Internal energy excitation and dissociation of molecular nitrogen in a compressing flow

Applied Stochastic Processes

Dynamics 4600:203 Homework 08 Due: March 28, Solution: We identify the displacements of the blocks A and B with the coordinates x and y,

Thermodynamics II. Department of Chemical Engineering. Prof. Kim, Jong Hak

A quote of the week (or camel of the week): There is no expedience to which a man will not go to avoid the labor of thinking. Thomas A.

Laser Types Two main types depending on time operation Continuous Wave (CW) Pulsed operation Pulsed is easier, CW more useful

Lecture 3: Probability Distributions

The non-negativity of probabilities and the collapse of state

Physics 115. Molecular motion and temperature Phase equilibrium, evaporation

Continuous Time Markov Chain

Turbulent Nonpremixed Flames

Primer on High-Order Moment Estimators

Numerical Solution of Ordinary Differential Equations

SPACE-FREQUENCY MODEL OF ULTRA WIDE-BAND INTERACTIONS IN FREE-ELECTRON LASERS. Yosef Pinhasi Yuri Lurie Asher Yahalom

PhysicsAndMathsTutor.com

Homework Assignment 3 Due in class, Thursday October 15

Using T.O.M to Estimate Parameter of distributions that have not Single Exponential Family

Chapter 7 Channel Capacity and Coding

A Nonlinear Transport Problem of Monochromatic Photons in Resonance with a Gas

Bayesian decision theory. Nuno Vasconcelos ECE Department, UCSD

IIM Shillong PGP ( ) Admissions Process

Thermodynamics General

NUMERICAL DIFFERENTIATION

Abneesh Srivastava and Joseph T. Hodges

Chapter 15: Radiation Heat Transfer

On resolving the optical spectra of the edge plasma radiation against a strong background of the divertor stray light

Transcription:

Lecture 5: Quanttatve Emsson/bsorpton. Eqn. of radatve transfer / Beer s Law o (ν) Gas (ν). Ensten theory of radaton 3. pectral absorpton coeffcent Collmated lht @ ν L 4. Radatve lfetme 5. Lne strenths Lht transmsson throuh a slab of as Beer s Law () = o () (- L)

. Eqn. of radatve transfer / Beer s Law Enery balance ν hn sample of emttn/absorbn as ν +d ν Collmated lht @ ν dx absorpton reflecton scattern transmsson spectral absorptvty, or absorbance dx d no unts spectral transmssvty pectral absorpton coeffcent (the d / dx - fracton of ncdent lht ν over cm frequency rane ν ν+dν whch s absorbed per unt lenth dx W/cm spectral ntensty n or cm nterate over ν W/cm d lso apples to @ ν for total W/cm Hz

. Eqn. of radatve transfer / Beer s Law Enery balance ν hn sample of emttn/absorbn as ν +d ν Collmated lht @ ν dx Consder emsson from the as slab em pectral no unts emssvty em no unts Blacbody spectral radancy Krchhoff s Law emssvty equals absorptvty emsson absorpton d emsson absorpton Dfferental form of the eqn. of radatve transfer d dx 3

. Eqn. of radatve transfer / Beer s Law Enery balance Dfferental form of the eqn. of radatve transfer d dx nterate over L nterated form of the eqn. of radatve transfer L L Optcal depth o (ν) Gas (ν) Collmated lht @ ν L Consder two nterestn cases: Emsson, bsorpton 4

. Eqn. of radatve transfer / Beer s Law Case : Emsson erment (no external radaton source) Emsson types: pectral radancy: pectral emssvty: L L L, L nterate over ν L Ld L L L L nle/multple lne nle/multple bands Contnuum Optcal depth: Optcally thc: Optcally thn: L L 4 L, L, Note: d d L 4 d -4 tefan-boltzmann constant 5 - - 5.67 er cm s K L L L, ε L 5

. Eqn. of radatve transfer / Beer s Law Case : bsorpton erment L L L L = v (- v ) = absorbance Beer s Law / Beer-Lambert Law lternate form: L Observatons:. he same equaton would apply to the transmsson of a pulse of laser exctaton, wth enery E [/cm /cm - ],.e., =E /E. he fundamental parameter controlln absorpton over lenth L s the spectral absorpton coeffcent,. How s related to fundamental molecular parameters? 6

. Ensten theory of radaton mplfed theory (Mlne heory) tate ranston probablty/s of process per atom n state or pontaneous Emsson nduced bsorpton nduced Emsson B ρ(ν) B ρ(ν) E Enery E h tate otal transton rate [molec/s] N N B ρ(ν) N B ρ(ν) Ensten coeffcents of radaton B ρ(ν) B ρ(ν) he probablty/s that a molecule n state osed to radaton of spectral densty ρ(ν) [/(cm 3 Hz)] wll absorb a quantum hν and pass to state. he Ensten B-coeffcent thus carres unts of cm 3 Hz( s). he probablty/s that a molecule n state osed to radaton of spectral densty ρ(ν) wll emt a quantum hν and pass to state. he probablty/s of spontaneous transfer from state to wth release of photon of enery hν (wthout reard to the presence of ρ(ν)). 7

. Ensten theory of radaton mplfed theory (Mlne heory) Equlbrum Detaled balance N N B N B eq rad molec/s entern state N B h N B eq Planc s blacbody dstrbuton B rad. equl. 3 8h 3 B c statstcal equl. 3 3 8 h / c B eq / h / molec/s leavn state Note: for collmated lht eq 3 - eq np h /cm s - n h cw/cm s B B / B 3 8h / c h / Radatve lfetme Where s the ln to? p h / 3 / c 8

. Ensten theory of radaton Fnd for a structureless absorpton lne of wdth δν Recall Beer s Law: L d dx ν δν Gas ν δν+(d ν )δν bsorbed power Optcally thn lmt P abs ncdent power over fracton absorbed W/cm L W/cm s - s - dx P dx Now, let s fnd fracton absorbed usn Ensten coeffcents abs dx Pabs fracton absorbed dx 9

. Ensten theory of radaton Fnd ν for a structureless absorpton lne of wdth δν ν δν Enery balance d nduced emsson spontaneous emsson nduced absorpton nduced emsson = nduced absorpton = for collmated lht ndx B h molec/cm ndx B h molec/cm n state n state prob/s of emsson prob/s of emsson d n B n B d dx enery per photon enery per photon h cm n B h / c h n B c h c dx n B Gas dx Recall: ν δν+(d ν )δν nce ν s a functon of δν, we conclude depends on lnewdths + hence shape; next, repeat wth realstc lneshape / c

Where are we headed next? mproved Ensten heory, Radatve Lfetme, Lne trenth 3. pectral absorpton coeffcent wth proper lneshape 4. Radatve lfetme 5. Lne strenths emperature dependence = absorbance X HO =. L = 5 cm Band strenth Wavenumber [cm - ] Water vapor absorpton spectrum smulated from HRN

. pectral absorpton coeffcent Eqn. of radatve transfer Recall: o Gas (ν) (ν) Collmated lht @ ν L L L ndependent of lneshape! d, cm dx For structureless absorpton lne of wdth δν (Hz), we found h n B h cm / c Note n, B, and /δ Next: use realstc lneshape to replace /δ

. pectral absorpton coeffcent Repeat dervaton of ν usn an mproved lneshape model tructureless absorpton lne of wdth δν Replace wth realstc lneshape typcal absorpton lne wth typcal structure 3

3. pectral absorpton coeffcent ν Recall Beer s Law: Defne: Note: d, max p,max d lne d L L Normalzed lneshape functon verae wdth cmor s, d lne nverse frequency ln Relevant transton probabltes have the same spectral dependence (shape) as and () nd we can antcpate that /v wll be replaced by n v equaton 4

3. pectral absorpton coeffcent Modfed model tate ranston probablty/s/molec (n level or ) for rane ν to ν +dν pontaneous Emsson nduced bsorpton nduced Emsson φ(ν)dν B φ(ν)dνρ(ν) B φ(ν)dνρ(ν) E Enery E h tate Ensten coeffcents of radaton φ(ν)dν B φ(ν)dνρ(ν) he probablty/s of a molecule underon spontaneous emsson, n the rane ν ν+dν. [Note that the nteral of ths quantty over the rane of allowed s just [s - ],.e., d.] he probablty/s of a molecule underon a transton from, n the rane ν ν+dν. B φ(ν)dνρ(ν) Recall: he probablty/s of a molecule underon a transton from, n the rane ν ν+dν. / c 5

3. pectral absorpton coeffcent Enery balance ν dν Gas ν dν+(d ν )dν d d [W/cm n ν to ν+dν] dx emsson n d absorpton n #/cc n dx molec/cm B d / c h ndx B d c h / prob/s molec for d d dx h n c d enery/photon B nb h nb h / c nterated absorpton / Lne strenth d cm s - - lne h c n B h / 6

3. pectral absorpton coeffcent Lne strenth alternate forms Lne strenth does not depend on lneshape, but s a functon of n,, B Oscllator strenth n 8 e n mec f f where h / cm s h / cm s.65cm Hzn f h actual /, p n 7 cm / atm.38 @ P, n =n=.7x 9 cm -3, ( hν /)<<, actual h /, classcal e, classcal n mec e, mec f f.65cm Hz f 7

3. pectral absorpton coeffcent mportant observatons. From the ornal defnton of ν and we have. When h / cm sde: @λ=44nm, hν/= 4 K @λ=7nm, hν/=x 4 K @λ=36nm, hν/=4x 4 K h / Hz as s common for electronc state transtons e n mec.65cm Hz n 8 f f n f / f.5 cm Radatve lfetme of the transton / 8

3. pectral absorpton coeffcent Example: Resonance ranston Resonance transton one that couples the round state to the frst excted state lower (L) upper (U) Electronc transton of a sodum atom Na3 / 3 P/ 5, 589nm 5.89 cm Conventons: atoms: (L-U) molecules:(u L), arrow denotes absorpton or emsson f j : denotes ntal state, j denotes fnal 9 f 589nm.5 cm 5.4 s 9 8 Measured: 6. s.6 s f.35 tron atomc transton: snle electron Much smaller for molecular transtons: ~ - - -4 9

3. pectral absorpton coeffcent Oscllator strenth ranstons f λ [nm] 3 / 3 P /.33 589.6 3 / 3 P 3/.67 589. 3 4 P.4 33. Oscllator strenths of selected sodum transtons Molecule CO OH v' v Electronc ranston Band center [cm - ] - 43.9x -5-46 7.5x -8-3568 4.x -6 Σ Π 36.x -3 CN Π Σ 97.x - bsorpton oscllator strenths of selected vbratonal and vbronc bands of a few molecules f

4. Radatve lfetme u l dn dt Radatve and non-radatve lfetmes u Rate equaton for radatve decay n Upper level u u u l l spontaneous emsson only Lower level l Radatve lfetme (zero-pressure lfetme) Rate equaton for non-radatve decay dnu nu nrnu dt nr nr Rate parameter [s - ] Non-radatve decay tme, depends on the transton consdered and on the surroundn molecules r n u t n t ul l u ul l ntal number densty multaneous presence of radatve and non-radatve transtons dnu nu nu nu, r nr Lfetme of level u dt r nr

5. Lne strenths.. 3. 4. lternate forms Lne strenths cm cm cm cm ccm/s s d cm / ccm /s cm / atm cm / Patm cm / cm cm / cd s Number densty of absorbn speces n state n c h / P atm 8 * cm / moleccm nmolec/ cc cm / atm deal as law * cm / moleccm 35dynes/ cm atm cm / atm 6.3854 er/k * 7.34 cm atm @ =96K HRN unt P * atm 9.4797 cm atm

5. Lne strenths lternate forms Beer s Law,, L n L PL PL n = number densty of the absorbn speces [molecules/cm 3 ] σ ν = absorpton cross-secton [cm /molec] = lne strenth [cm - atm - ] or [cm - sec - /atm] β ν = frequency-dependent absorpton coeffcent [cm - /atm] P = partal pressure of speces [atm] φ ν = frequency-dependent lneshape functon [cm] or [s] v = v L = absorbance Common to use atmosphere and wavenumber unts n R cm /atm d cm s cp atm 8.8 c 8 n P 3 P n atm f h / h / / P absorpton coeffcent per atmosphere of pressure 3

emperature dependence 4 5. Lne strenths,, hc hc hce Q Q Lne strenth n unts of [cm - atm - ] Lne strenth n unts of [cm - /(molecule cm - ],, * * hc hc hce Q Q * *

Band strenth 5 5. Lne strenths Example: Heteronuclear Datomc Band trenth ' ' ' v v R P band band lnes 6 6 / 8.3 / 8.3 n n c P n n c R / n n c 6 8.3 h n n c R R / ' /.3 8 ' 6 ' atm, P n P Based on normalzed Hönl-London factor

5. Lne strenths Band strenth band lnes band Example: Heteronuclear Datomc Band trenth 6.3 c 8 Band strenth of CO: 3. 8 CO 73K 8cm /atm 5cm 36s 6.4 3 s.8s Compare wth prevous example of τ Na 6ns R transtons have much lower values of and loner radatve lfetme than UV/Vsble transtons due to ther smaller chanes n dpole moment 6

Next: pectral Lneshapes Doppler, Natural, Collsonal and tar Broadenn Vot Profles