Diffraction and Spectroscopy PDF
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These handwritten notes cover topics in diffraction and spectroscopy, including formulas, wave properties, concepts, and various types of spectroscopy. The notes include specific examples and calculations related to spectra, energy levels and transitions.
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### 03/01/25 ### Friday - 2dsinθ=nλ - E=E<sub>0</sub>ei(kx-wt) - (Semiconductors) - Spectroscopy & Diffraction? - Study of spectrum - Plot btw intensity/amplitude (vs) Energy. - I/A - Structure - Energy levels - Spectrum - H+ - +H+ - +H - Diffractio...
### 03/01/25 ### Friday - 2dsinθ=nλ - E=E<sub>0</sub>ei(kx-wt) - (Semiconductors) - Spectroscopy & Diffraction? - Study of spectrum - Plot btw intensity/amplitude (vs) Energy. - I/A - Structure - Energy levels - Spectrum - H+ - +H+ - +H - Diffraction pattuen (Solids) - XRD - Electron - CD (Visible light) - H<sub>2</sub>O ice - Amorphous (T<0<sup>o</sup>C) - Crystalline ### 7/01/25 ### Tuesday ### Waves - E=E<sub>0</sub>ei(kr-wt) - Frequency. - K - wave vector, which shows direction. - Re(E) at t=0 - E - electric field - H=H<sub>0</sub>e<sup>i(kr-wt)</sup> - Plane wave - H⊥E⊥k - <S>= ±(ExH*) - Pointing vector - <S> gives the energy flow. - Reason why waves imp in spectroscopy - Wave interact with material - 1. Molecular atoms. - 2. Bonding H bond/covalent - 3. Special arrangment. - Solid, liquid, Gas. - Contribute final - x band structure (λ) - Electronic structure in a material. ### - Energy levels lump together - Transition (excitation) - Emission - n=2 (emission process) - n=1 (Ground state) - 1<sup>st</sup> excited state - Coord (in Four Space) - Inelastic process - Typically represented by K - Elastic process - Comes from a quantum - E<sub>lev</sub> - Visible range - Elastic - Inelastic - Not belong to absorption - Either release a photon(or) phonon (deexcitation) - Happen based on - 1. hv photon - 2. phonon - Thermal (N/0e<sup>V</sup> ~ 3-4 eV) enough energy - - Plot bed. - Photon comes and hits the molecule & then - Out put intensity - Which is not absorbed. - I<sub>o</sub>e<sup>-αx </sup> ; x-unit length. - Comes in term of a curve. ### - At t=0 - E=E<sub>0</sub>e<sup>i(kz)</sup> - n - refractive index - n=n<sub>o</sub>+n<sub>1</sub>, - amount of absorption we have in a material - Spectrum - Depend of absorption, n<sub>o</sub>+n<sub>1</sub> - Inversely proportional. - When products of n<sub>o</sub>+n<sub>1</sub> and absorption are increased, the spectrum also becomes broadened. - Case 2 - As multiple level are increased, spectrum also broaden, where it was narrow time ### - n<sub>1</sub> & a are independent in concentration. - How do we calculate the absorption co-efficient? - How do you find transition probability of the given level to the other level? - For ex: based on the equation n=∫f(E)D(E) dE - Total(S<sub>1</sub>) (emp S<sub>2</sub>)(ΔE) - (E) - limits matters. - Emplaty (empty state) - Total(S<sub>1</sub>) (D<sub>Os</sub>) (Cmps) (ΔE) - Total(S<sub>1</sub>) - Density - States - e<sup>r</sup> - Change in transition. - 1 mole = 1 mole/L=6×10<sup>23</sup> mole/L - V=V<sub>2</sub>= 2.5×10<sup>-3</sup> m calculate no.d. molecules/cm<sup>3</sup> - 10<sup>-3</sup>A 10<sup>-3</sup> moles = 1.17×10<sup>17</sup> - 1mM - Beam, 5mm, 1x10<sup>-2 </sup>m - What decides height of peaks/absorption co-efficient? - If you have more eo which conduct, there will be more absorption. - How do you find probability / "(E) =∫f(E) P(E) dE for a transition to happen? - (No.q.es in ground state) (Empty State in 1st Excited State)(ΔE) ### - Can we do absorption in spectroscopy for a single crystal? - No. It's 10<sup>5</sup>-10<sup>7</sup> 1mM - No. It's 10<sup>9</sup>-10<sup>11</sup> 1nM. How do we reduce this no? - Let have arbitrary sample. - Difficult to calculate inelastic - Backward scattering - (I/I<sub>0</sub>)NAbsorption - No scatt - Pointless - Extinctiom = Absorptiom + Scattering - (elastic) - Energy Consumption purely - d - (dipole approximation ) - Based on this we can categorize spectroscopy into two types: - Absorption spectroscopy - Ex: absorption spectra - Scattering Spectroscopy - Ex: Raman effect - Sometimes called - Holoramission Spectroscopy. - (small) dipole absorption - If very small, the scattering looks like - Assuming particle is so small (f), scattering happens in a similar way to dipole. - So, how dipole scatters? ### - Im=1$/mole/L = 6.023×10<sup>23</sup>. MM=1 - Let's say beam of 5mm circle, solution of concentration 1mM. - In measurement volume, how many molecules? - Cylinder = πr<sup>2</sup>h - π(5x10<sup>-3</sup>)<sup>2</sup> - π(5x10<sup>-3</sup>)<sup>2</sup> - π(5x10<sup>-3</sup>)<sup>2</sup> - π(5x10<sup>-3</sup>)<sup>2</sup> - 5x10<sup>-3 </sup> cm - 1x10<sup>-2 </sup>m - Beam Cylinder. - 6×10<sup>23</sup>. - 6×10<sup>23</sup> - x = 6×10<sup>23</sup>/25 - (6×10<sup>23</sup>)/25 - X = 4×10<sup>9</sup> - 2 = 6×10<sup>23</sup> x 3.14 x 25 x 10<sup>-6</sup> - 6x3.14x25 - 117.75x10<sup>5</sup> - 1.1775x10<sup>17</sup> - (10<sup>5</sup>-10<sup>7</sup>)- 1mM ### - Distance blw person & wall = 100 cm. - Distance blw points on wall= 15 cm. - Periodicity-? - Gravity - (mmmmf) Periodicity- - (mm) - K 100cm. - Density (height, wt they say) - 0 - AE → - EELS and EDS - Xray - cathode luminascence - Input (light (e)) - Output (spectroscopy) (light(e)) ### - By Sairam Sir. - Infrared - causes heating (~700 nm) - UV - energy higher than visible light (~400 nm) - UV-Vis Spectroscopy - Based on the energy range peak. - Energy related to some events happening in atom - Emission - Absorption - Scattering - Electron - Electron energy loss spectroscopy - Sing signal coming - (From the sample) - Which means visible light going in and coming out - I vs λ - How do we do it? - "Prism" spectrum ### - Other points in α for a sample. - Red shift - Blue shift - Spectroscopy - quantifying, but looking at displacement (t). - Inelastic scattering event energy lost. - Electron energy lost spectroscopy: with the help of energy lost. - During it with photoemission by using x-rays (e's out) - 1. σ-(typical ) λ<sub>out</sub> - 2. - (k-1) - K(1-1/π) - 2 - 2 - 2 - 3. - ΔE - Virtual energy band ### - 28/01/25 ### Tuesday - Raman -no (s<sub>0</sub>) - Inelastic - E<sub>0</sub> ≠E<sub>1</sub> - Rayleigh scattering. - - ΔE - E<sub>0</sub>,<sub>3</sub> - E<sub>0</sub>,<sub>2</sub> - - ΔE=hc( ) - E<sub>0 </sub>,<sub>1</sub> = (Anti-stokes) - (Phonones supplies energy ) - E<sub>0</sub>,<sub>1</sub> < E<sub>1</sub> = (Stokes) - (Phonons take energy) - - Antistokes - Stokes - Higher energy - Lower energy → Rayleigh wavenumber ### - Why is Raman so special? - How does Raman tell you about bond into? - EELS - Quiz on ### - Scattered lig - (sunlight) white - Raylight scattered - Raman scattered. - violet - Green - Green filter - Observe - violet - Stokes of Antistokes in graph au mirror images. - Intensities of Stokes are higher than antistokes, why? - Strong spectrum = [ ]<sup>1/2</sup>cm<sup>-1</sup> - E<sub>1</sub>=532nm - E<sub>2</sub>=633nm (red) - I ### - Depends on laser we use, same positions of Raman peaks, but intensity varies. - v<sup>2</sup> =(1-/λ<sub>s</sub>) - This remains same. - G<sub>2</sub> - G<sub>1</sub> - What is the different b/w fluorescence of Raman. - What leads to laser emission. How is it beneficial? - Gas Lasers has narrow line width - Diode Lasers. Why is it important in terms of Raman speciality? - (bar) am&ad = ξ