Quantum Mechanics and Atomic Physics – Flashcards

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probability of position
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|Γ|²
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Expectation value of A
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Hermitian operator
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∫ƒ(x)*(Ag(x))dx = ∫(Af(x))g(x)dx
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Facts about hermitians (2)
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All their eigenvalues are real Eigenfunctions corrisponding to different eigenvalues are orthogonal
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measurement of an operator
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always returns an eigenvalue, and if discrete the measurement of A is quantized
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sqrt of probability of a measurement
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Cn = ∫fn(x)*Γ(x,t)dx where fn is the orthonormal basis
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inner product of |a> and |b>
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hermitian conjugate
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the conjugate operator that would provide the same answer when the operator is applied to the other vector in the inner product
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hermitian operator
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hermitian operators are equal to their hermitian conjugate
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Hilbert Space
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Infinite dimensional vector space
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conjugate vectors in Hilbert Space
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<b| = (transposeb)*
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conjugate operators in Hilbert Sfpace
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A⁺ = (transposeA)*
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commutator
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[a,b] = ab-ba
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commutator of x and p
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{x,p} = ihbar
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commutator identity for [AB,C]
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[AB,C] = A[B,C] + [A,C]B
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commutator identity for [A,BC]
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[A,BC] = [A,B]C + B[A,C]
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Uncertainty principle
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σa²σb²≥((1/2i))²
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Heisenburg uncertainty principle
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σxσp≥hbar/2 and is usually in the range of ∆x∆p≈hbar
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nodes in quantum mechanics
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correspond to the energy level starting at 0 for n=0
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One dimension harmonic osc hamiltonian
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H = hbarw(a⁺a+1/2)
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harmonic osc [a,a+]
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[a,a⁺]=1
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harmonic osc energy levels
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En=hbarw(n+.5)|n> from 0→∞
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lowering operator a
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a|n> = √(n)|n-1>
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raising operator a+
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a⁺|n> = √(n+1)|n+1>
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viral theorem inc. harmonics
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==En/2
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three dimensional harmonic Energies
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En=(n₁+n₂+n₃+1.5)hbarw
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infinite square well wavefnctn
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γ=sqrt(2/a)sin(nπx/a)
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infinite square well energies
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n²π²hbar²/2ma²
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free particle wavefnctn
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γ=e^(±ikx)
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energy of free particle
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E=hbar²k²/2m where k=p/hbar
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scattering wavefnctns
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Before impact with V: Ae^(ikx) + Be^(-ikx) During impact with V: something After impact with V: Ce^(ik'x)
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probabilities of reflection and transmition
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R=|B|²/|A|²; T=|C|²/|A|²; R+T=1
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normalization in 3D
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radial and angular pieces are normalized seperately
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ang momentum operators
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Lx=yPz-zPy; Ly=zPx-xPz; Lz = xPy-yPx
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total angular momentum operator L^2
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L²=-hbar²del²
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z angular momentum operator
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Lz=-ihbard/d∅
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L^2 acting on angular wavefunction
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L²Y=l(l+1)hbar²Y
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Lz acting on angular wavefunction
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LzY=mhbarY
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allowed values of m given l
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m=l,l-1,...-l
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phi dependence of Y
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e^(im∅)
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Hamiltonian for hydrogen
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H = -hbar²del²/2µ + e²/(4πε₀r)
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Bohr radius
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a=4πε₀hbar²/µe^2
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wavefunction for hydrogen atom approx
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psy1 α e^(-r/a)
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energy for a hydrogenic atom
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hbar²/2µa² = E1
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energy for hydrogen ground state
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13.6 eV
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energy for following hydrogenic states
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E1/n²
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frequency of emitted light from hydrogenic atoms
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f α 1/n₂² - 1/n₁²
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fine structure constant
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1/137
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pauli spin matrix for x
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[0,1;1,0]
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pauli spin matrix for y
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[0,-i;i,0]
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pauli spin matrix for z
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[1,0;0,-1]
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addition of s
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s values dont add, but possible values range from s+s' to |s-s'|
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addition of ms
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mstot = ms +ms'
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Total spin operator for addition
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S = S₁ + S₂, can either be - or +
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spin lowering operator on two electrons in the s=1,m=1 state
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S⁻|↑>|↑> = (S⁻₁|↑>|↑> + S⁻₂|↑>|↑> = hbar(|↓>|↑>+|↑>|↓>), now in s=1,m=0 state
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singlet state of two electrons
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s=0,m=0; |↑>|↓>-|↓>|↑>
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wavefunctions of bosons
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symmetric (constructive)
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wavefunctions of fermions
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antisymmetric (destructive)
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Pauli Exclustion principle
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No two identical fermions can occupy the same state
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first order Hamiltonian perturbation
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H = H₀+λH';
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first order energy perturbation
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En = En₀ + λ
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2nd order energy perturbation
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E₀+λ²∑||²/En-Em
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simplification of
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H'mn, in other words, the off diagonal elements of H'mn
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degenerate actions
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Diagonalize the peturbation in the subspace of degenerate states
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variational principle
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cannot be less than the unperturbed ground state
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Adiabatic theorem of QM
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If starting in H, the particle will end up in the /corresponding/ eigenstate of H'
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Bohr model
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no radiation in specific rings around atom, L=nhbar
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Fine structure
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relativistic correction for the electron + spin orbit coupling, intro to J=L+S, order α² smaller
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Lamb shift
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accounts for J degeneracy; order α³ smaller
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Spin-Spin coupling
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magnetic dipole dipole interaction between protons and electrons; order α² smaller;
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orbital number per energy shell
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2n²
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states per orbital
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2(2l+1)
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Stark effect
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E field on Hydro, only m=0 is split, ∆H = eE.r
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Zeeman effect
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B field on Hydro, ∆H=(e/2m)(L+2S).B; e/2m is known as the gyromagnetic ratio
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Selection rules
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∆m=±1 or 0; ∆l=±1; except from 2s→1s
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Blackbody radiation intensity
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I α (hw³/c²)(1/(e^(hbarw/kbT) -1)
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Power per area pf Blackbody
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dP/dA α T⁴
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Peak of BB spectrum (Wein's displacement Law)
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λmax = (2.9x10⁻³ K.m)/T
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