A bilinear form on is nondegenerate whenIn finite dimensions this is equivalent to nondegeneracy in the first argument.
Define the linear mapNondegeneracy makes injective. Since and its dual space have the same finite dimension, is an isomorphism. Similarly define and setThen is linear and
If , this identity gives for every . Conversely, if for every , then for every , so nondegeneracy gives . HenceThis is the representation of a bilinear form relative to a nondegenerate bilinear form.
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Fix . By assumption there is a neighbourhood of on which with uniform convergence. Each restriction is continuous, and a uniform limit of continuous functions is continuous. Thus is continuous, in particular at . Since was arbitrary, is continuous on .
Now let be compact and let . For each , choose a neighbourhood on which convergence is uniform. The sets cover , so compactness gives a finite subcoverFor each , choose such thatTaking , every belongs to one of these finitely many neighbourhoods, and thereforeThus uniformly on every compact subset. This proves the local uniform convergence on compact subsets principle.
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The domains are not conformally equivalent. Suppose that were a conformal equivalence. Since is bounded near zero, the Riemann removable singularity theorem extends it holomorphically across zero. The extension is a bounded entire function, so the Liouville theorem makes it constant, contradicting bijectivity. This is the punctured plane is not conformally equivalent to the punctured unit disc obstruction.
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The domains are not conformally equivalent. If were a conformal equivalence, composing it with a Cayley transform from the upper half-plane to the unit disc would produce a bounded nonconstant entire function. This contradicts the Liouville theorem, proving that the complex plane is not conformally equivalent to the upper half-plane.
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The domains are conformally equivalent. The MΓΆbius transformationmaps the upper half of the unit disc onto the first quadrant: its diameter maps to the positive real axis and its upper semicircle maps to the positive imaginary axis. Squaring maps the first quadrant bijectively and conformally onto the upper half-plane. Thereforeis the required equivalence, as recorded by the conformal equivalence between the upper half-disc and upper half-plane.
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Write the expectation value asDifferentiating and retaining the possible explicit time dependence of the observable givesThe Schrodinger equation and its adjoint arewhere the Hamiltonian operator is Hermitian. Substitution yieldsThis is the proof of Ehrenfest theorem from the Schrodinger equation.
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For a particle in the scalar potential energy ,The canonical commutation relation givesThe Ehrenfest theorem with therefore givesSince and direct action on a wavefunction gives ,Finally has no explicit time dependence and , so
The first two equations are the expectation-value counterparts of momentum equals mass times velocity and Newton's second law; the last is conservation of energy. They become the classical equations directly when the force varies negligibly across the wave packet, so that . These conclusions are summarized by the classical equations from Ehrenfest theorem.
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Let be the angle between and the positive -axis. By superposition of the electric potential of point charges,For , the Legendre polynomial expansion givesThereforeThe three displayed terms are respectively the monopole, dipole, and quadrupole terms of the electric multipole expansion. In particular, the total charge is and the electric dipole moment is . This is the multipole expansion of three collinear charges.
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The monopole vanishes exactly whenand the dipole vanishes exactly whenSince and are positive integers, both vanish precisely for
Assume now that the monopole has been cancelled. If is held fixed while , the quadrupole coefficient tends to zero, whereas the dipole coefficient has a finite limit. For this is a point-dipole limit; for the limiting external potential vanishes.
If instead is held fixed, the dipole coefficient isIt diverges unless . When and , both lower multipoles vanish and the quadrupole coefficient has a finite nonzero limit. These are the dipole and quadrupole scaling limits of three collinear charges.
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Here and . At , the -components of the fields of the two outer charges cancel by reflection symmetry. By Coulomb's law, the remaining field isMultiplying by the test charge givesThe quantity in parentheses is positive. Thus for the force points in the negative direction, while for it points in the positive direction. It is always attractive toward the origin, as in the transverse force from a collinear electric quadrupole.
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The nonzero orthogonal polynomials have distinct degrees and form an orthogonal basis of . DefineFor each ,Thus the residual is orthogonal to all of .
For any , writeThe two terms are orthogonal, so the Pythagorean theorem in an inner-product space givesEquality holds only for . This proves the formula and uniqueness of the least-squares polynomial in an orthogonal-polynomial basis.
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Part (a) shows that is orthogonal to . Sincethe Pythagorean theorem in an inner-product space immediately givesThis is the norm decomposition associated with orthogonal projection onto a finite-dimensional subspace.
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Let . First-step analysis givesand, because state moves to or remains at with equal probabilities,The last equation gives . Substitution into the second gives , and the first then gives . HenceThese are the expected hitting times of the absorbing state.
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Let be the probability of reaching state before state . The boundary values are and . First-step analysis at states and givesTherefore , so the requested hitting probability is
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Let be the expected number of visits to state before absorption, counting the present state when . Its reward equations areThe last equation gives , so the second nontrivial equation gives . Hence , andThus the expected occupation count is two; together with the previous parts, this is the four-state reflecting absorbing random walk calculation.
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For ordered bases of and of , the matrix representation of a linear map is the matrix whose th column consists of the -coordinates of . Thus
The operators are conjugate linear operators when there is an isomorphism such thatIn one basis their matrices therefore satisfy , so they are similar matrices.
For invertible , the mapis linear, and its inverse is ; hence it is a linear isomorphism of . If , define . A direct substitution givesso and are conjugate. This is the conjugation operator on an endomorphism space.
It remains to compute the Jordan normal form over . By the preceding conjugacy, we may put in Jordan form.
Ifthen the matrix units are eigenvectors becauseThusThis includes the scalar case , when is the identity.
Otherwise has one size-two Jordan block. Multiplying by a nonzero scalar does not change , and conjugating within its Jordan class allows us to use with . Put . Direct multiplication givesHence , , and . The nilpotent Jordan blocks of therefore have sizes three and one. Adding the identity givesThese two cases are the Jordan normal form of conjugation on two-by-two matrices.
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Letbe primitive. The Eisenstein criterion states that if a prime number satisfiesthen is an irreducible polynomial in , equivalently in by Gauss lemma for polynomials.
To prove it, suppose that with of positive degree. Primitivity and Gauss's lemma let us take such an integral factorisation if a factorisation over exists. Reducing modulo givesBecause does not divide the leading coefficient of , neither factor loses degree on reduction. The polynomial ring is a unique factorization domain, so both reductions are monomials of positive degree. In particular, divides both constant terms and . It follows that dividesa contradiction. This proves the criterion.
For a prime , translate the geometric sum by one:Its leading coefficient is one, every other coefficient is divisible by , and its constant coefficient is , which is not divisible by . It is therefore Eisenstein at . Translation is an automorphism of , soThis is the geometric-sum irreducibility criterion.
The evaluation homomorphismhas image and contains in its kernel. Since is monic, division by in writes every as with . If , then ; the irreducibility of says that is the minimal polynomial of , so . Thus , and the first isomorphism theorem for rings gives
Now take . Then , and the Eisenstein integers areComplex conjugation sends to , so the field norm isGiven , choose integers with . For ,For with , apply this to and put . ThenHence the norm is a Euclidean function, proving that is a Euclidean domain. This is the Euclidean norm on the Eisenstein integers.
Finally suppose satisfies . Make the free abelian group into a -module by definingThis is well-defined precisely because obeys the same polynomial relation as . The module is finitely generated. It is also torsion-free module: if and , multiplication by the conjugate of gives , and the additive group has no nonzero integer torsion.
A Euclidean domain is a principal ideal domain, and the structure theorem for finitely generated modules over a principal ideal domain says that a finitely generated torsion-free module over one is free. Thusfor some . Since has free module basis over , comparison of abelian ranks gives . There can consequently be no such matrix when is odd.
If , choose a -basis . Thenis a -basis, and . In this basis the matrix of is a direct sum of copies ofEvery admissible matrix is therefore conjugate in to . Hence there is exactly one conjugacy class for even , and none for odd . This is the classification of integral matrices satisfying the third cyclotomic polynomial.
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A compact space is a topological space in which every open cover has a finite subcover. A Hausdorff space is one in which every two distinct points have disjoint open neighbourhoods. A homeomorphism is a bijection that is continuous and whose inverse is continuous.
For an equivalence relation on , let be the set of equivalence classes and letThe quotient topology declares open exactly when is open in . It follows directly from the definition that is continuous.
Suppose that the continuous map is constant on equivalence classes. The only possible factorisation iswhich is well-defined by the hypothesis and satisfies . For every open ,is open in . The definition of the quotient topology therefore makes open, so is continuous. This proves the universal property of the quotient topology.
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Let be compact and the quotient map. If is an open cover of , then is an open cover of . A finite subfamily covers ; because is surjective, the corresponding cover . Thus every quotient of a compact space is compact.
The Hausdorff property need not survive. On the real line, defineThe quotient has more than one point. If two nonempty open subsets of the quotient were disjoint, their inverse images would be disjoint nonempty open subsets of invariant under rational translation. But any two nonempty open intervals acquire an intersection after one is translated by a suitably chosen rational number, so two such saturated open sets cannot be disjoint. Distinct quotient points cannot be separated, and the quotient is not Hausdorff. This is the non-Hausdorff quotient of the real line by rational translation.
Finally let be a continuous bijection, with compact and Hausdorff. Every closed subset is compact. Its continuous image is compact, and every compact subset of a Hausdorff space is closed. Hence is a closed map. For every closed ,is closed in , so is continuous. Therefore is a homeomorphism. This is the compact-to-Hausdorff continuous bijection theorem.
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DefineThis is continuous and takes values on the unit sphere. It agrees at and , is constant on the bottom edge, and is constant on the top edge. Thus it is constant on every -class, so the universal property of the quotient topology gives a continuous map
For , the third coordinate determines , and the first two coordinates determine modulo one. Consequently the only equal values of in the open strip arise from and . At the whole edge maps to the north pole, and at the whole edge maps to the south pole. These are exactly the identifications defining , so is injective. The spherical-coordinate formula also shows that it is surjective.
The square is compact, hence its quotient is compact by part (ii), while is Hausdorff as a subspace of . The compact-to-Hausdorff continuous bijection theorem now makes a homeomorphism. Geometrically, identifying the vertical sides produces a cylinder and collapsing each boundary circle to a point produces the suspension of a topological space , which is . This proves the square quotient model of the two-sphere.
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Letbe reflection in the unit circle, and represent a MΓΆbius transformation byA direct calculation shows that is represented byThus exactly when and differ by a nonzero scalar. Applying the conjugate-linear involution twice shows that this scalar has modulus one. Rescaling by a suitable complex scalar then makes . Consequently all commuting maps, and only those maps, have the formThis is the MΓΆbius maps commuting with reflection in the unit circle classification.
For such a map,It follows that whenever precisely whenThe inverse has the same property, so these and only these maps preserve the unit disc.
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The Poincare disc model isIts geodesics through the origin are the Euclidean diameters. To see directly that the radial segment from to minimizes length, write an arbitrary joining curve as . Its hyperbolic length satisfiesThe radial segment has constant and monotone , so equality holds. Henceand every radial diameter is length minimizing. Rotational symmetry and uniqueness for the geodesic equation show that these are all geodesics through .
Given any geodesic and a point on it, a disc-preserving maptakes to the origin. By part (a), is a hyperbolic isometry and commutes with . The transformed geodesic is a diameter, hence a generalized circle invariant under . Its inverse image is therefore also a Generalized circle under a MΓΆbius transformation invariant under . Thus every hyperbolic geodesic is the part in of a Euclidean line or circle preserved by reflection in the unit circle; equivalently, it is a diameter or a circle orthogonal to the unit circle. This is the Geodesics of the Poincare disc description.
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Rotate the disc so that lies on the positive real axis. From part (b), the perpendicular hyperbolic line is a Euclidean circle orthogonal to the unit circle, with centre on the real axis and radius . Orthogonality of the two circles givesCombining the two equations yields
The radial distance formula from part (b) saysThe hyperbolic double-angle identities now giveThereforeThis is the Euclidean circle representing a perpendicular hyperbolic line.
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Use the hyperboloid model with Minkowski inner productPut the vertex with angle at , and place the endpoints of its adjacent sides of lengths and atThe geodesic through perpendicular to has spacelike unit normalwhile the geodesic through perpendicular to has spacelike unit normal
These two geodesics form the remaining two sides of the quadrilateral. Their angle equals the angle between their normals in the tangent plane at their intersection. The third right angle therefore givesDividing by proves the Lambert quadrilateral identity
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Because the matrix-valued Laplace transform is taken componentwise, for every we haveThe sum is finite and is constant, so it may be moved outside the integral. Therefore
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Taking the Laplace transform of the differential equation and usinggivesHenceWhenever is not an eigenvalue of , the matrix is invertible, and thusThis is the Laplace-transform solution of a constant-coefficient vector ODE.
Set . The given homogeneous solution is , so the preceding formula saysfor every initial vector . Equality on every vector gives the matrix identityon the common domain of convergence and in particular away from the eigenvalues of . This is the Laplace transform of a matrix exponential.
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The coefficient matrix has eigenvector with eigenvalue and eigenvector with eigenvalue . WriteSinceand , the system diagonalises toUsing an integrating factor givesThe unique fastest term is thereforeConsequently diverges for , tends to zero for , and for tends to the finite nonzero vectorThus the only requested integer isThis is an instance of dominant eigenmode in a forced linear system.
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Let and , where the variations vanish on the boundary. The first variation isApplying integration by parts to the four derivative terms and discarding the boundary contributions givesThe variations and are independent and arbitrary in the interior. The fundamental lemma of the calculus of variations therefore gives the two Euler-Lagrange equations for two fields
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For the displacement gradient tensor specified in the question,while the divergence is . Hence the isotropic linear-elastic energy density isExpanding the square and collecting terms yields
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Let the displayed integrand be . Since it has no explicit dependence on or , the Euler-Lagrange equations for two fields areIts derivatives areThusUsing the Laplacian, gradient, and divergence, these combine into the static Navier-Cauchy equation
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In the one-dimensional limit, and . The first component of the Navier-Cauchy equation reduces toFor a nondegenerate one-dimensional elastic material, , so and . The boundary conditions and give and . Therefore the uniform extension of a one-dimensional elastic body is
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Take the Fourier transform in . Since , the transformed heat equation isThereforeThe given transform pair and the convolution theorem yield the heat-kernel solution
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The causal Green function for the heat operator iswhere is the Heaviside step function. It vanishes for , satisfies the homogeneous heat equation away from the source, and approaches as . Superposing the responses to all infinitesimal sources gives Duhamel principle:The lower limit and causality give the required homogeneous initial data.
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LetConvolution with the initial Dirac delta function translates the heat kernel, while part (b) propagates the impulsive source from time one. HenceAt this becomesIt vanishes exactly whenThis is the cancellation of two heat-kernel impulses.
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Use and the canonical commutation relation. With ,Using these two transformation laws on givesThese are the orbital angular momentum commutation relations.
NowThe factor is antisymmetric in and its remaining product is symmetric after the two terms are combined, so the contraction vanishes:
The same commutators show that and are rotational scalars: their commutators with every vanish by contraction of the antisymmetric with a symmetric product. Therefore also commutes with every , and forwe have , henceIn particular are pairwise commuting Hermitian operators. By simultaneous diagonalization, they admit a common eigenbasis, subject to the usual spectral-domain qualifications for unbounded operators. This is the rotational invariance of a central-potential Hamiltonian.
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For a bound state, and therefore . As , the terms proportional to are subleading and the radial Schrodinger equation has dominant balanceIts exponential behaviours are and . The growing solution is not normalizable, so
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Put . ThenAfter substitution and cancellation of the terms, the equation becomesFor the power series , the coefficient of isThus
If the series does not terminate, then , so acquires the large- behaviour and grows like . Normalizability therefore requires termination, which occurs whenfor some positive integer . HenceThe ground state has , so the hydrogen ground-state energy isThis is the series-termination quantization of the Coulomb radial equation.
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Take the spherical harmonic to have unit angular norm. The radial normalization condition is thenThereforeEquivalently, if denotes the entire spherically symmetric wavefunction rather than the radial factor multiplying normalized , then .
The expected radius isFor the ground state, . The Bohr radius is , soThe mean radius is therefore of the Bohr-radius scale and is one and a half times . This is the radial normalization of the hydrogen ground state.
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Write the free surface as the zero setBecause this is a material surface, the kinematic boundary condition is . Thus, on ,Thereforeat the free surface. This is the kinematic boundary condition for a free-surface graph.
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For irrotational flow, . Incompressibility gives the Laplace equationThe rigid side walls impose no penetration:and decay in the infinitely deep fluid requires as .
Linearizing the kinematic condition from part (a) about givesThe Unsteady Bernoulli equation, evaluated at the surface and linearized about hydrostatic equilibrium, gives the dynamic conditionThese are the linearized free-surface boundary conditions. Initial values for and specify the transient; below we also record the initially quiescent solution.
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Forthe normal derivative at contains and the normal derivative at contains . Both therefore vanish at the side walls.
At , has exactly the same horizontal dependence as the imposed pressure. The dynamic boundary condition is consequently consistent provided has that same horizontal mode. This is the rectangular standing surface-gravity mode selected by the forcing.
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Substitution into givesSetThen . Since the fluid occupies , decay as forces . Absorbing into and choosing givesThis is the usual exponential depth dependence of a deep-water gravity wave.
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The dynamic condition reduces toDifferentiate and define the natural frequencyThen the surface amplitude obeys the forced harmonic oscillatorFor , its general solution and the corresponding potential amplitude are
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The denominators in part (v) vanish when the forcing frequency equals the natural surface gravity wave frequencyAt this value, the initially quiescent resonant solution isBoth contain a term growing linearly in time. This is resonance: the pressure forcing repeatedly supplies energy in phase with the box's standing-wave mode. In the ideal inviscid linear model there is no damping or nonlinear saturation, so its amplitude is unbounded. This is the resonance of a pressure-forced rectangular surface-gravity mode.
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Write the linear mean model asThe errors are independent but heteroscedastic. Minimizing the unweighted residual sum of squaresgives the normal equationThus, provided ,Since ,Hence it is an unbiased estimator. This is the least-squares part of the estimators for a Poisson exposure model.
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Ignoring terms independent of , the log-likelihood isIts score function isSince , the interior critical point is the maximum, givingThe sum of independent Poisson distributions is Poisson with mean , soThus the maximum-likelihood estimator is also unbiased.
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PutIndependence and givewhereas givesThe Cauchy-Schwarz inequality, applied to and , yieldsConsequentlyEquality holds exactly when all positive exposures are equal. This is the variance comparison for Poisson exposure estimators.
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Both alternatives have larger , so use upper-tail rejection regions. Let be the 95th quantile of the standard normal distribution.
For the likelihood estimator,When is large, the normal approximation to the Poisson distribution gives, under ,An approximate size- test therefore rejects when
When every is large, independently. A linear combination of independent normal variables is normal, so under ,The corresponding approximate size- test rejects whenIn both cases the null rejection probability is approximately , while values near the alternative mean increasingly fall in the rejection region as the total exposure grows. These are the normal-approximation tests for a Poisson exposure model.
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Let be Player I's row-strategy distribution and let denote an all-ones vector of the required dimension. Against column , the expected payoff is . Thus Player I's matrix-game optimization problem isEquivalently, Player I maximizes over the probability simplex.
Let be an optimal mixed strategy for Player II and let the game value be . A sufficient condition for a probability vector to be optimal for Player I isIndeed, this makes guarantee at least against every pure column and hence every mixed strategy. On the other hand, the optimality of prevents any row strategy from obtaining more than against . Therefore is optimal. This is the mixed-strategy optimality certificate for a matrix game.
Now suppose that is invertible and symmetric and that . PutThe vector is nonzero and nonnegative, so and are probability vectors. Since is symmetric,Thus guarantees and holds the payoff to . By the minimax theorem,This proves the symmetric inverse formula for a matrix-game equilibrium.
For the card game, the payoff matrix to Player I isIt is symmetric and invertible, and direct solution of givesThe preceding result therefore gives the same optimal strategy for both players:Thus each player chooses cards with probabilities , respectively, and the value to Player I isThis is the three-card threshold-sum zero-sum game.
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