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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            expectation value if the probabilities are known
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            inner product of |a> and |b>
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            dirac notation for the hermitian conjugate operator
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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
