Survey of Mathematics
Unit 7

Differential equations

Change described by equations, solved with linear algebra.

7 chapters written · 49 definitions · 68 theorems · builds on Unit 3, Unit 4, Unit 5

The story

Differential equations describe change. Existence and uniqueness (7.1) come from the fixed point theorem of Unit 4. Linear equations have solution sets that are vector spaces (7.2 and 7.3), so Unit 2 applies directly.

Systems x′=Axx' = Ax are solved by the matrix exponential, computed with eigenvalues (7.4). Power series solve the equations that have no closed form (7.5), and phase portraits show long-run behaviour without solving anything (7.6).

Chapters

  1. 7.1Existence and uniqueness for differential equationsA differential equation with a starting value has exactly one solution, for a short time, as long as its right-hand side does not stretch distances too fast. The proof turns the equation into an integral equation and applies the contraction mapping theorem to the space of continuous functions.
  2. 7.2Linear differential equationsThe solutions of a homogeneous linear equation of order n form a vector space of dimension n, because "solution to starting values" is an isomorphism. Every solution of the inhomogeneous equation is one particular solution plus a homogeneous one. With constant coefficients, the roots of the characteristic polynomial write the whole solution space down.
  3. 7.3The Wronskian, variation of parameters and undetermined coefficientsThe Wronskian is a determinant of functions and their derivatives. A non-zero value proves independence; for solutions of one linear equation it is either zero everywhere or non-zero everywhere. The same determinant solves the inhomogeneous equation (variation of parameters), and for special right-hand sides a short guess does it faster (undetermined coefficients, annihilators).
  4. 7.4Systems of equations and the matrix exponentialThe system x' = Ax is solved by x(t) = e^(tA) x(0), where the matrix exponential is the exponential series with a matrix in place of the number. It always converges, and it is computed by diagonalizing, by splitting A into a scalar part and a nilpotent part (Jordan form), or by Putzer's method. The eigenvalues also decide the shape of the solution curves.
  5. 7.5Power series solutions, Legendre and BesselWhen the coefficients of a linear equation change with x, assume a power series (or a power series times a power of x) and the equation turns into a recurrence for the coefficients. At an ordinary point the series converges as far as the coefficients do. At a regular singular point the indicial equation says which power to start with. Legendre's equation gives orthogonal polynomials, Bessel's gives the function J0, and Airy's equation is the model of a turning point.
  6. 7.6Phase portraits, stability and linearizationAn autonomous system is studied by drawing its orbits in the plane. An equilibrium is stable if nearby solutions stay near it. For a linear system the trace and the determinant of the matrix decide the picture completely. For a nonlinear system, near a hyperbolic equilibrium the picture is that of the Jacobian matrix there. The pendulum and the predator-prey equations show both the power and the limits of this idea.
  7. 7.7Applications to springs, circuits, epidemics and qubitsFour real systems run on the machinery of Unit 7. Coupled masses split into independent oscillators along the eigenvectors of a symmetric matrix. An RLC circuit is a damped oscillator, so the same equation, the same roots and the same resonance. The SIR epidemic has a threshold R0 that is the sign of one eigenvalue at the disease-free equilibrium. The state of a two-level quantum system evolves by the matrix exponential of -iH/hbar.

The theorem chain

Every theorem in the unit, in the order it is proved. Each one is used by the ones after it. The label says whether it is on the 375/376 exams (T), an Apostol extra (A), or beyond both (B).

7.1 Existence and uniqueness for differential equations

  1. Fact · T A higher-order equation is a first-order system Put x=(y,y′,…,y(n−1))x = (y, y', \dots, y^{(n-1)}). Then y(n)=f(t,y,…,y(n−1))y^{(n)} = f(t, y, \dots, y^{(n-1)}) is the same as x′=F(t,x)x' = F(t, x) for a vector function FF.
  2. Theorem · T An IVP is an integral equation A continuous function yy solves y′=f(t,y)y' = f(t, y), y(t0)=y0y(t_0) = y_0 on an interval exactly when y(t)=y0+∫t0tf(s,y(s)) dsy(t) = y_0 + \int_{t_0}^{t} f(s, y(s))\,ds for every tt in it.
  3. Theorem · B Derivative test for a Lipschitz condition If f(t,x)f(t, x) is differentiable in the real variable xx on a region where ∣∂f/∂x∣≤L\lvert \partial f/\partial x \rvert \le L and the region contains the segment between any two positions at the same time, then ff satisfies a Lipschitz condition with constant LL.
  4. Theorem · T Picard–Lindelöf theorem If ff is continuous and Lipschitz in xx on a rectangle around (t0,x0)(t_0, x_0), the IVP has exactly one solution on a short interval around t0t_0, and Picard iteration converges to it.
  5. Fact · B The norm of an integral For a continuous curve v:[a,b]→Rmv : [a, b] \to \mathbb R^m, ∥∫abv(s) ds∥≤∫ab∥v(s)∥ ds\lVert \int_a^b v(s)\,ds \rVert \le \int_a^b \lVert v(s) \rVert\,ds.
  6. Corollary · B Two solutions that meet are equal If ff is continuous and satisfies a Lipschitz condition on every closed rectangle inside its domain, then two solutions of the same IVP agree on every interval where both are defined.
  7. Theorem · B Linear systems have solutions on the whole interval If A(t)A(t) and g(t)g(t) are continuous on an interval JJ, then x′=A(t)x+g(t)x' = A(t)x + g(t), x(t0)=x0x(t_0) = x_0 has exactly one solution, and it is defined on all of JJ.

7.2 Linear differential equations

  1. Fact · T A linear differential operator is a linear map L(f+g)=Lf+LgL(f + g) = Lf + Lg and L(cf)=c LfL(cf) = c\,Lf, so the solutions of Ly=0Ly = 0 form the null space of a linear map.
  2. Theorem · T Homogeneous and inhomogeneous solution sets The solutions of Ly=0Ly = 0 form a vector space. If Ly=RLy = R and RR is not the zero function, the solutions do NOT form a vector space: they are yp+ker⁡Ly_p + \ker L, where ypy_p is any one solution.
  3. Theorem · T Existence and uniqueness for linear equations of order n For continuous coefficients and right-hand side on JJ, any t0∈Jt_0 \in J and any numbers c0,…,cn−1c_0, \dots, c_{n-1}, the equation Ly=RLy = R has exactly one solution on all of JJ with y(k)(t0)=cky^{(k)}(t_0) = c_k for k<nk < n.
  4. Theorem · T Dimension of the solution space of a linear ODE The solution space ker⁡L\ker L of a homogeneous linear equation of order nn has dimension exactly nn.
  5. Corollary · T General solution of a linear equation If b1,…,bnb_1, \dots, b_n is a basis of ker⁡L\ker L and ypy_p solves Ly=RLy = R, then every solution is y=yp+c1b1+⋯+cnbny = y_p + c_1b_1 + \dots + c_nb_n.
  6. Theorem · T Constant-coefficient operators multiply like polynomials If A=PA(D)A = P_A(D) and B=PB(D)B = P_B(D) then AB=(PAPB)(D)AB = (P_AP_B)(D). In particular AB=BAAB = BA.
  7. Fact · T Derivative of a complex exponential For a complex number r=α+iβr = \alpha + i\beta, ert=eαt(cos⁡βt+isin⁡βt)e^{rt} = e^{\alpha t}(\cos\beta t + i\sin\beta t) satisfies D(ert)=rertD(e^{rt}) = re^{rt}.
  8. Fact · T Shifting an exponential For a polynomial pp and a number rr: (D−r)(p(t)ert)=p′(t) ert(D - r)\big(p(t)e^{rt}\big) = p'(t)\,e^{rt}.
  9. Theorem · T Basis for repeated roots The mm functions ert,tert,…,tm−1erte^{rt}, te^{rt}, \dots, t^{m-1}e^{rt} are a basis of the solutions of (D−r)my=0(D - r)^my = 0.
  10. Fact · T Kernel of a factor lies in the kernel of the product If A=A1A2⋯AkA = A_1A_2\cdots A_k are constant-coefficient operators, then ker⁡Aj⊆ker⁡A\ker A_j \subseteq \ker A for every jj.
  11. Theorem · T Basis of solutions from the roots If PA(t)=∏i=1k(t−ri)miP_A(t) = \prod_{i=1}^{k}(t - r_i)^{m_i} with distinct roots rir_i, the n=∑min = \sum m_i functions tjeritt^je^{r_it} (i≤ki \le k, 0≤j<mi0 \le j < m_i) are a basis of the solutions of Ay=0Ay = 0.
  12. Theorem · T Real solutions from complex roots If AA has real coefficients and r=α+iβr = \alpha + i\beta (β≠0\beta \ne 0) is a root of multiplicity mm, then so is rˉ\bar r, and the 2m2m functions tjeαtcos⁡βtt^je^{\alpha t}\cos\beta t and tjeαtsin⁡βtt^je^{\alpha t}\sin\beta t (0≤j<m0 \le j < m) replace the 2m2m complex solutions tjertt^je^{rt} and tjerˉtt^je^{\bar rt}.

7.3 The Wronskian, variation of parameters and undetermined coefficients

  1. Theorem · T A non-zero Wronskian proves independence If W(f1,…,fn)(t0)≠0W(f_1, \dots, f_n)(t_0) \ne 0 at even one point t0t_0 of JJ, then f1,…,fnf_1, \dots, f_n are linearly independent on JJ.
  2. Theorem · T Wronskian of solutions of a linear equation For nn solutions of Ly=0Ly = 0 the following are equivalent: they are linearly independent; W(t)≠0W(t) \ne 0 for every tt; W(t0)≠0W(t_0) \ne 0 for some t0t_0. So WW is either zero everywhere or non-zero everywhere.
  3. Theorem · A Abel's formula If b1,…,bnb_1, \dots, b_n solve y(n)+an−1y(n−1)+⋯=0y^{(n)} + a_{n-1}y^{(n-1)} + \dots = 0, their Wronskian satisfies W′=−an−1WW' = -a_{n-1}W, so W(t)=W(t0)exp⁡ ⁣(−∫t0tan−1)W(t) = W(t_0)\exp\!\big(-\int_{t_0}^{t}a_{n-1}\big).
  4. Fact · T Wronskian of exponentials For distinct numbers r1,…,rnr_1, \dots, r_n, W(er1t,…,ernt)=e(r1+⋯+rn)t⋅VW(e^{r_1t}, \dots, e^{r_nt}) = e^{(r_1 + \dots + r_n)t}\cdot V with V=det⁡(ri j)V = \det(r_i^{\,j}) non-zero, so the exponentials are independent.
  5. Theorem · T Wronskian test for power series If ff and gg are power series with radius of convergence 11, then f,gf, g are linearly independent on (−1,1)(-1, 1) if and only if W(f,g)W(f, g) is not identically zero.
  6. Theorem · T Variation of parameters formula If b1,…,bnb_1, \dots, b_n is a basis of ker⁡L\ker L with Wronskian matrix W\mathcal W, and u′=W−1(0,…,0,R)Tu' = \mathcal W^{-1}(0, \dots, 0, R)^{\mathsf T}, then yp=u1b1+⋯+unbny_p = u_1b_1 + \dots + u_nb_n solves Ly=RLy = R.
  7. Theorem · A Shape of a particular solution If R=q(t)ertR = q(t)e^{rt} with qq a polynomial of degree dd and rr is a root of PLP_L of multiplicity ss (s=0s = 0 if rr is not a root), then Ly=RLy = R has a particular solution yp=ts h(t) erty_p = t^s\,h(t)\,e^{rt} with hh a polynomial of degree at most dd.

7.4 Systems of equations and the matrix exponential

  1. Fact · T Eigenvectors give solutions If Av=λvAv = \lambda v with v≠Ov \ne O, then x(t)=eλtvx(t) = e^{\lambda t}v solves x′=Axx' = Ax.
  2. Theorem · T The matrix norm is submultiplicative ∥AB∥≤∥A∥ ∥B∥\lVert AB\rVert \le \lVert A\rVert\,\lVert B\rVert, hence ∥Ak∥≤∥A∥k\lVert A^k\rVert \le \lVert A\rVert^k.
  3. Theorem · T Absolutely convergent matrix series converge If ∑k∥Mk∥\sum_k\lVert M_k\rVert converges as a series of numbers, then ∑kMk\sum_kM_k converges in the space of matrices.
  4. Theorem · T The matrix exponential always converges For every square matrix MM the series ∑Mk/k!\sum M^k/k! converges, and ∥eM∥≤n−1+e∥M∥\lVert e^M\rVert \le n - 1 + e^{\lVert M\rVert}.
  5. Theorem · T The derivative of e^(tA) ddtetA=AetA=etAA\dfrac{d}{dt}e^{tA} = Ae^{tA} = e^{tA}A.
  6. Theorem · T The law of exponents for one matrix e0A=Ie^{0A} = I, e(s+t)A=esAetAe^{(s+t)A} = e^{sA}e^{tA}, and etAe^{tA} is invertible with inverse e−tAe^{-tA}.
  7. Theorem · T Solution of the linear system The IVP x′=Axx' = Ax, x(a)=bx(a) = b has the unique solution x(t)=e(t−a)Abx(t) = e^{(t-a)A}b, defined for all real tt.
  8. Theorem · T e^(A+B) equals e^A e^B when A and B commute If AB=BAAB = BA then eA+B=eAeBe^{A+B} = e^Ae^B. Without AB=BAAB = BA the equation can fail.
  9. Corollary · T e^A is always invertible For every square matrix AA, eAe^A is invertible and (eA)−1=e−A(e^A)^{-1} = e^{-A}. Moreover det⁡eA=etr⁡A\det e^A = e^{\operatorname{tr}A} (a fact beyond the course).
  10. Fact · T The exponential of a diagonal matrix etdiag⁡(d1,…,dn)=diag⁡(ed1t,…,ednt)e^{t\operatorname{diag}(d_1, \dots, d_n)} = \operatorname{diag}(e^{d_1t}, \dots, e^{d_nt}).
  11. Theorem · T Exponential of a diagonalizable matrix If A=CDC−1A = CDC^{-1} with DD diagonal, then etA=CetDC−1e^{tA} = Ce^{tD}C^{-1}.
  12. Theorem · T Exponential of a rotation-scaling block For A=[a−bba]=aI+bJA = \begin{bmatrix}a & -b\\b & a\end{bmatrix} = aI + bJ with J=[0−110]J = \begin{bmatrix}0 & -1\\1 & 0\end{bmatrix}: etA=eat[cos⁡bt−sin⁡btsin⁡btcos⁡bt]e^{tA} = e^{at}\begin{bmatrix}\cos bt & -\sin bt\\\sin bt & \cos bt\end{bmatrix}.
  13. Theorem · A Exponential of a 2 by 2 matrix For a 2×22 \times 2 matrix with eigenvalues λ,μ\lambda, \mu: if λ=μ\lambda = \mu, etA=eλt(I+t(A−λI))e^{tA} = e^{\lambda t}\big(I + t(A - \lambda I)\big); if λ≠μ\lambda \ne \mu, etA=eλtI+eλt−eμtλ−μ(A−λI)e^{tA} = e^{\lambda t}I + \frac{e^{\lambda t} - e^{\mu t}}{\lambda - \mu}(A - \lambda I); if λ,μ=a±ib\lambda, \mu = a \pm ib, etA=eat(cos⁡bt I+sin⁡btb(A−aI))e^{tA} = e^{at}\big(\cos bt\,I + \frac{\sin bt}{b}(A - aI)\big).
  14. Theorem · T Real and imaginary parts of a complex solution If AA is real and Av=λvAv = \lambda v with λ=a+ib\lambda = a + ib, b≠0b \ne 0, and v=u+iwv = u + iw with u,wu, w real vectors, then x1=eat(cos⁡bt u−sin⁡bt w)x_1 = e^{at}(\cos bt\,u - \sin bt\,w) and x2=eat(sin⁡bt u+cos⁡bt w)x_2 = e^{at}(\sin bt\,u + \cos bt\,w) are two independent real solutions of x′=Axx' = Ax.
  15. Theorem · T Exponential of a scalar plus a nilpotent matrix If A=λI+NA = \lambda I + N with Nk=ON^k = O, then etA=eλt(I+tN+t2N22!+⋯+tk−1Nk−1(k−1)!)e^{tA} = e^{\lambda t}\Big(I + tN + \frac{t^2N^2}{2!} + \dots + \frac{t^{k-1}N^{k-1}}{(k-1)!}\Big).
  16. Theorem · A Putzer's method With eigenvalues λ1,…,λn\lambda_1, \dots, \lambda_n listed with multiplicity and P0=IP_0 = I, Pk=(A−λ1I)⋯(A−λkI)P_k = (A - \lambda_1I)\cdots(A - \lambda_kI), one has etA=∑k=0n−1rk+1(t)Pke^{tA} = \sum_{k=0}^{n-1}r_{k+1}(t)P_k, where r1′=λ1r1r_1' = \lambda_1r_1, r1(0)=1r_1(0) = 1 and rk+1′=λk+1rk+1+rkr_{k+1}' = \lambda_{k+1}r_{k+1} + r_k, rk+1(0)=0r_{k+1}(0) = 0.
  17. Theorem · T Variation of constants for systems The IVP x′=Ax+g(t)x' = Ax + g(t), x(a)=bx(a) = b has the unique solution x(t)=e(t−a)Ab+∫ate(t−s)Ag(s) dsx(t) = e^{(t-a)A}b + \int_a^te^{(t-s)A}g(s)\,ds.
  18. Theorem · T The Neumann series If ∥A∥<1\lVert A\rVert < 1 for the matrix norm of this chapter, then I−AI - A is invertible and (I−A)−1=∑k≥0Ak(I - A)^{-1} = \sum_{k\ge0}A^k.
  19. Theorem · B Classification of planar linear systems

7.5 Power series solutions, Legendre and Bessel

  1. Theorem · T Matching coefficients If a power series ∑cn(x−x0)n\sum c_n(x - x_0)^n equals 00 at every point of an interval around x0x_0, then every coefficient cnc_n is 00.
  2. Theorem · A Series solutions at an ordinary point If pp and qq are analytic on (x0−r,x0+r)(x_0 - r, x_0 + r), then y′′+py′+qy=0y'' + py' + qy = 0 has two independent solutions that are power series in x−x0x - x_0 converging on the whole interval. The coefficients come from a recurrence, with a0a_0 and a1a_1 free.
  3. Theorem · A Recurrence for Legendre's equation Series solutions y=∑anxny = \sum a_nx^n of Legendre's equation satisfy an+2=(n−ν)(n+ν+1)(n+1)(n+2) ana_{n+2} = \dfrac{(n-\nu)(n+\nu+1)}{(n+1)(n+2)}\,a_n. They converge for ∣x∣<1\lvert x \rvert < 1, and they stop (are polynomials) when ν\nu is an integer of the right parity.
  4. Theorem · A Legendre polynomials solve Legendre's equation PnP_n has degree nn and satisfies (1−x2)Pn′′−2xPn′+n(n+1)Pn=0(1 - x^2)P_n'' - 2xP_n' + n(n+1)P_n = 0 and Pn(1)=1P_n(1) = 1.
  5. Theorem · A Orthogonality of the Legendre polynomials ∫−11Pm(x)Pn(x) dx=0\int_{-1}^{1}P_m(x)P_n(x)\,dx = 0 for m≠nm \ne n, and ∫−11Pn(x)2 dx=22n+1\int_{-1}^{1}P_n(x)^2\,dx = \dfrac{2}{2n+1}.
  6. Corollary · A Expansion in Legendre polynomials PnP_n is orthogonal to every polynomial of degree less than nn. A polynomial ff of degree at most NN equals ∑k=0NckPk\sum_{k=0}^{N}c_kP_k with ck=2k+12∫−11fPk dxc_k = \frac{2k+1}{2}\int_{-1}^{1}fP_k\,dx.
  7. Theorem · A The Frobenius recurrence The Frobenius series xs∑anxnx^s\sum a_nx^n with a0=1a_0 = 1 solves x2y′′+xPy′+Qy=0x^2y'' + xPy' + Qy = 0 exactly when F(s)=0F(s) = 0 and, for every n≥1n \ge 1, F(s+n) an=−∑k=0n−1[(s+k)pn−k+qn−k]akF(s+n)\,a_n = -\sum_{k=0}^{n-1}\big[(s+k)p_{n-k} + q_{n-k}\big]a_k.
  8. Theorem · A The Frobenius theorem At a regular singular point with indicial roots α1≥α2\alpha_1 \ge \alpha_2, the larger root always gives a Frobenius series solution u1u_1. If α1−α2\alpha_1 - \alpha_2 is not a whole number, the smaller root gives a second one. If the roots are equal, or differ by a whole number, a second solution contains u1ln⁡xu_1\ln x.
  9. Theorem · A J0 solves Bessel's equation of order zero The series J0J_0 converges for every real xx and solves x2y′′+xy′+x2y=0x^2y'' + xy' + x^2y = 0. The indicial equation is s2=0s^2 = 0 (a double root), so a second solution contains ln⁡x\ln x.

7.6 Phase portraits, stability and linearization

  1. Fact · B Orbits do not cross Two orbits of an autonomous system either coincide or never meet. A solution that comes back to its starting point is periodic, and its orbit is a closed curve.
  2. Theorem · B Classification of the origin by trace and determinant
  3. Theorem · B Stability of a linear system For x′=Axx' = Ax with AA real n×nn \times n: the origin is asymptotically stable if every eigenvalue has negative real part (and then ∥etA∥≤Ce−μt\lVert e^{tA}\rVert \le Ce^{-\mu t}); unstable if some eigenvalue has positive real part. If all real parts are ≤0\le 0 it is stable exactly when every eigenvalue with real part 00 has only 1×11 \times 1 Jordan blocks.
  4. Theorem · B Hartman–Grobman theorem Near a hyperbolic equilibrium, a nonlinear system has the same phase portrait as its linearization, up to a continuous change of coordinates that preserves the direction of time.
  5. Theorem · B Linearization and stability If every eigenvalue of J=DF(x∗)J = DF(x^*) has negative real part, then x∗x^* is asymptotically stable for the nonlinear system. If some eigenvalue has positive real part, it is unstable.
  6. Theorem · B The Lotka–Volterra conservation law For x′=x(a−by)x' = x(a - by), y′=y(dx−c)y' = y(dx - c) with positive constants, H=dx−cln⁡x+by−aln⁡yH = dx - c\ln x + by - a\ln y is constant along solutions in the open first quadrant. Every orbit there is a closed curve around the equilibrium (c/d, a/b)(c/d,\ a/b), and the average of xx and of yy over a period equal its equilibrium value.
  7. Theorem · B Lyapunov's direct method If there is a Lyapunov function near x∗x^*, then x∗x^* is stable. If there is a strict one, x∗x^* is asymptotically stable.

7.7 Applications to springs, circuits, epidemics and qubits

  1. Theorem · B Normal-mode decomposition If MM is symmetric positive definite with orthonormal eigenvectors v1,…,vnv_1, \dots, v_n and eigenvalues ωj2\omega_j^2, then every solution of x′′=−Mxx'' = -Mx is x(t)=∑j(ajcos⁡ωjt+bjsin⁡ωjt)vjx(t) = \sum_j\big(a_j\cos\omega_jt + b_j\sin\omega_jt\big)v_j with aj=vj⋅x(0)a_j = v_j\cdot x(0) and bj=vj⋅x′(0)/ωjb_j = v_j\cdot x'(0)/\omega_j.
  2. Fact · B A passive circuit loses energy With no source, the stored energy W=12LI2+q22CW = \frac12LI^2 + \frac{q^2}{2C} satisfies W˙=−RI2≤0\dot W = -RI^2 \le 0. With a source, W˙=IE−RI2\dot W = IE - RI^2.
  3. Theorem · T Steady-state response of the driven RLC circuit For E(t)=E0cos⁡ωtE(t) = E_0\cos\omega t, every solution is a decaying transient plus the steady state Iss(t)=E0∣Z∣cos⁡(ωt−φ)I_{ss}(t) = \dfrac{E_0}{\lvert Z\rvert}\cos(\omega t - \varphi), where Z=R+i(ωL−1ωC)Z = R + i\left(\omega L - \dfrac{1}{\omega C}\right) is the impedance.
  4. Theorem · B The epidemic threshold
  5. Theorem · B Peak and final size of an epidemic Along every solution of the SIR system, i+s−1R0ln⁡si + s - \dfrac1{R_0}\ln s is constant. Hence the infection peaks when s=1/R0s = 1/R_0 at imax⁡=i0+s0−1+ln⁡(R0s0)R0i_{\max} = i_0 + s_0 - \dfrac{1 + \ln(R_0s_0)}{R_0}, and the epidemic ends with i→0i \to 0 and s→s∞s \to s_\infty where ln⁡s0s∞=R0(s0+i0−s∞)\ln\dfrac{s_0}{s_\infty} = R_0(s_0 + i_0 - s_\infty).
  6. Theorem · B Unitary evolution The solution of iℏψ′=Hψi\hbar\psi' = H\psi is ψ(t)=U(t)ψ(0)\psi(t) = U(t)\psi(0) with U(t)=e−iHt/ℏU(t) = e^{-iHt/\hbar}. For Hermitian HH the matrix U(t)U(t) is unitary, so ∥ψ(t)∥=∥ψ(0)∥\lVert\psi(t)\rVert = \lVert\psi(0)\rVert for all tt: total probability stays 11.
  7. Theorem · B The Rabi formula For H=ℏ2(δσz+Ωσx)H = \frac\hbar2(\delta\sigma_z + \Omega\sigma_x) and ΩR=δ2+Ω2\Omega_R = \sqrt{\delta^2 + \Omega^2}: e−iHt/ℏ=cos⁡ΩRt2 I−isin⁡ΩRt2⋅δσz+ΩσxΩRe^{-iHt/\hbar} = \cos\frac{\Omega_Rt}{2}\,I - i\sin\frac{\Omega_Rt}{2}\cdot\frac{\delta\sigma_z + \Omega\sigma_x}{\Omega_R}. Starting in level 1, the probability of level 2 is Ω2ΩR2sin⁡2ΩRt2\dfrac{\Omega^2}{\Omega_R^2}\sin^2\dfrac{\Omega_Rt}{2}.

Terms this unit defines

Unit review

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Where it leads

Units that build on this one: Unit 15, Optimisation, dynamics and computation.