Bills Lecture 5 (Pending Title) Flashcards
Synchotron Radiation
A method of making X-Rays
Particle accelerators accelerate electrons to near the speed of light. They give of X-rays when they slow down.
X-Rays
Wavelength of 0.01 to 10 nm / 0.1 to 100 Å
Parameters that describe an electromagnetic wave
Amplitude, Wavelength, and Phase (where a locus is on the wave)
Destructive Interference
Zero amplitude, waves cancel out.
Constructive Interference
Stronger Amplitude
Intermediate between Destructive Interference and Constructive Interference
Reduced Amplitude
Bragg’s Law
λ=2dsinθ
xy=yz=dsinθ
xyz=2dsinθ
Explains X-ray diffraction by treating crystals as consisting of layers or planes of semi-transparent mirrors. Some X-rays are reflected with an angle of reflection that equals the angle of incidence and some are transmitted through the plane and reflected by subsequent planes.
Compton Effect
Reduction in frequency of scattered x-ray beam occurs since the collision of photons with the electron results in an energy loss.
Elastic Scattering
Production of scattered radiation with the same wavelength as the incident beam.
The Atomic Scattering Factor “f”
(sinθ)/λ
Amplitude of x-rays scattered by an atom in any direction. Given in arbitrary electron units (e.u.), such that the forward scattering at θ=0 is equal to the number of extra nuclear atoms Z.
The Structure Factor “F”
F=Σf
I ∝ |F|^2 : Intensity is proportional to the magnitude of F squared.
This is the amplitude of X-rays scattered by one unit cell, in e.u.’s in the direction of the hkl reflection. Into a reflection hkl, each atom scatters its amplitude f. The amplitudes from all the atoms add together with phase differences dependent on hkl and the positions of the atoms.
Vector Representation of a Wave
Argand Diagram
A + iB = c cosα + ic sinα is equivalent to c*exp[iα]
Where c = Amplitude and exp[iα] = Phase
The Electron Density Equation
ρ(x,y,z) = 1/Vc * Σ F(h,k,l)*exp[-2πi(hx+ky+lz)]
Where:
ρ(x,y,z) = Electron density at any point x,y,z
Vc = Volume of the unit cell
The Patterson Function
Puvw = 1/Vc Σ |F|^2 cos2π(hu + kv + lw)
The height of a Patterson peak depends on the number of electrons in the atoms between which the vector occurs and is proportional to their atomic numbers (Z).
Vectors between heavy atoms appear with heights equivalent to the square of their atomic numbers (Z) and so can stand out against the heavy-light, light-light atom vectors.
No phase information required, only intensity measurements and knowledge of symmetry
The Patterson function is centrosymmetric even if original structure is not.
Types of Patterson Vector
Cross Vectors: Between atoms in the same asymmetric unit
Harker vectors: Between symmetry related atoms