For positive arrival rates and capacities with every route nonempty, maximizing over , has a unique positive optimizer . The Karush-Kuhn-Tucker conditions give for nonnegative link prices with complementary slackness. Under proportional scaling by , the Stirling formula gives a uniform logarithmic weight approximation . Strict concavity and compactness give an objective gap away from , while only polynomially many feasible states exist. Thus the stationary distribution has in probability, with exponentially small probabilities outside any fixed neighborhood of . In particular .
Factorial proof of Mertens first theorem 2026-10-14
The prime factorization of gives . The Chebyshev estimate bounds the error on replacing each floor by its argument by . Dividing by and using the Stirling formula gives . The contribution of is bounded by the convergent series . This proves the Mertens first theorem without the Prime number theorem.
Independent spin-one-half two-level system 2026-09-29
For distinguishable noninteracting spins, let a fraction occupy the level and the remainder occupy . The Stirling formula givesThe relation yieldsPositive temperature corresponds to ; a population inversion has negative temperature.
Integrated Chebyshev sum Created 2026-10-06 Updated 2026-10-14
For , finite rearrangement and the Von Mangoldt divisor identity giveThe Stirling formula, or integral comparison for the logarithm, gives for real .
Order-one growth of the Riemann xi function 2026-10-14
The pole-subtracted theta integral for the completed zeta function bounds the Riemann xi function on by a polynomial in times . The Stirling formula gives logarithmic growth . On the positive real axis, the definition and give . Thus its order of an entire function is exactly one.
// Target: analytic-number-theory.bigb
Past exam of the mathematics course of the University of Cambridge 2002 iii Paper 25 3 Solution Created 2026-10-03 Updated 2026-10-14
Write and let run over Nontrivial zeros of the Riemann zeta function, including multiplicity. The bounds involving below are for . At bounded heights their uniform versions use ; itself cannot be the right bound near zero or .
Start with the Hadamard factorization of the Riemann xi function, an entire function of order one. Its logarithmic derivative has the convergent expansionDifferentiating givesThe real sum of converges absolutely: makes its terms at large height, and the order-one Hadamard factorization ensures the required summability. Thus these terms and form a fixed constant. The Stirling formula for the digamma function gives, uniformly for and ,This is the useful real form of the global partial-fraction expansion of the zeta logarithmic derivative. Every term subtracted is nonnegative because the Euler product excludes zeros with . At the simple pole , one also has as .
The three-four-one zero-free-region argument now detects a zero too close to one. The Von Mangoldt function is nonnegative and the absolutely convergent Dirichlet series givesbecause the corresponding coefficient at is . If is a zero, retain its term in the expansion at height and discard the other nonpositive terms. The expansion at height gives an upper bound even without retaining a particular zero. We obtain, for an absolute constant ,Choose so small that , put , and take . If , the last inequality would requirea contradiction. Thereforefor some fixed . This proves the required zero-free region of the Riemann zeta function. Nonvanishing on at bounded nonzero heights, proved in Question 2, and the isolation of zeros allow a decrease of giving the uniform formulation with as well. Near , apply this observation to the nonzero holomorphic function .
Next evaluate the real expansion at . The absolutely convergent Dirichlet series bounds uniformly in , soSince , each term on the left is at least . The smoothed zeta zero-count bound follows:Each zero satisfying contributes more than , so this also gives the local zero count for the Riemann zeta function:The same kernel sum is bounded at compact heights, since its tail converges uniformly there; the bounds with are consequently valid for all real .
For completeness, the contour estimate used in Question 2 follows from these very formulas. Subtract the complex logarithmic derivative expansion at from that at , with and . Terms with have differences , whose sum is by the kernel bound. There are remaining terms. After reducing , the zero-free region of the Riemann zeta function separates every such zero horizontally from the half-width boundary by : their heights satisfy . Thus on the left edge, and on the horizontal edges at , each reciprocal is . The Gamma function and pole terms satisfy the same required bound; at small heights on the left edge the pole distance is . This proves on those edges and justifies the contour shift without choosing heights that dodge unknown zeros.
Past exam of the mathematics course of the University of Cambridge 2003 iii Paper 13 1 Solution Created 2026-10-03 Updated 2026-10-14
Put , with a prime number, and . The printed bound needs a size qualification: for , and , all three singletons satisfy the intersection restriction, whereas . The intended nontrivial prime-power modular intersection bound holds when ; without that qualification the universally valid conclusion isWhen this follows simply by counting all -sets. We prove the sharper intended form for .
Choose an integer with and define the integer-valued polynomialFor its top argument is nonnegative. The bottom argument has all its first base- digits equal to . The Lucas theorem therefore givesFor every , consider on the Boolean hypercube. Its multilinear reduction on the Boolean cube has degree at most and integer coefficients: the coefficient of a square-free monomial is an alternating sum of its integer values on Boolean vertices. This observation permits reduction modulo even though the ordinary power-basis coefficients of need not have denominators prime to .
At the characteristic vectors of sets , these reduced polynomials have evaluation matrix equal to the identity modulo . Hence their evaluation functions are linearly independent over . To count the available functions, let have rows indexed by subsets with , columns indexed by all -sets , and entries . Over the rational numbers, for ,Thus the matrix rank over the rational numbers is at most . Every larger integer minor is zero and remains zero modulo , so the same rank bound holds over . This low-degree evaluation rank on a uniform layer proves
For the applications alternative, take a prime number , set , , and let be the modular intersection graph on all -subsets of , joining distinct sets when their intersection has size . An independent set avoids the only possible off-diagonal intersection congruent to modulo , so
First embed as in Euclidean space. The Euclidean distance satisfiesso distance one corresponds exactly to an edge of . Every colour class in a proper graph colouring is an independent set, giving the lower bound on the chromatic number of Euclidean spaceThe Stirling formula gives , where is the binary entropy function. Here the ratio is and , so this is an exponential lower bound along these dimensions.
Second set and represent by the off-diagonal entries , , of the symmetric matrix . This is an injective representation: equality of the matrices would give , and the minus sign would require . The common diagonal can be omitted without changing distances. The Frobenius inner product gives the quadratic sign-vector diameter formulaThe term inside the square is congruent to modulo , and its smallest possible absolute value is one, attained exactly at . Such pairs exist. Consequently the diameter pairs of this finite set in dimension are precisely the edges of . Every part of strictly smaller diameter is an independent set and has at most points. The required number of parts is at least the same exponential ratio, which exceeds for sufficiently large primes. Thus bounded sets need not admit a partition into sets of smaller diameter: this supplies a Kahn-Kalai counterexample to the Borsuk conjecture. Both applications use the prime case of the proved prime-power result.
Past exam of the mathematics course of the University of Cambridge 2003 iii Paper 22 1 Solution Created 2026-10-03 Updated 2026-10-14
Write for the Chebyshev theta function and for the Second Chebyshev function. Throughout, denotes a prime and all logarithms are natural. Each prime divides the central binomial coefficient, soApply this at and telescope: . Bounding a general by the next power of two proves . Splitting the prime-counting function at now givesThis is the required Chebyshev estimate from central binomial coefficients, with no use of a prime asymptotic.
The higher prime powers also satisfyFor an integer , the prime factorization of a factorial givesThe Stirling formula, or integral comparison for , says . After division by we obtain . MoreoverSubtract this bounded contribution and replace by . The factorial proof of Mertens first theorem therefore yields
For fixed , apply partial summation to and :The main contribution isThe bounded error in contributes at the endpoint and in the integral, since . Thus the positive logarithmic moments of reciprocal primes satisfy
Past exam of the mathematics course of the University of Cambridge 2004 iii Paper 13 5 Solution Created 2026-10-03 Updated 2026-10-14
The Frankl-Wilson theorem is a striking example of the polynomial method in combinatorics: an intersection restriction creates a family of linearly independent low-degree polynomials, whose dimension bounds the set family. Let be a prime number, let have elements, and let be a set family such that member sizes modulo avoid while every distinct pair has intersection size in modulo . Its general modular form givesIf all members have the same size and , the uniform refinement gives .
For the proof, work over the finite field and associate to the modular intersection polynomialAt the characteristic vector of a set , this equals zero for and is nonzero for . A linear relation among the evaluation functions therefore has every coefficient zero. The multilinear reduction on the Boolean cube, replacing by for , preserves these evaluations and the degree bound . There are possible square-free monomials, proving the general form.
For uniform members, the low-degree evaluation rank on a uniform layer supplies the sharper dimension bound. To verify this without division modulo , form the integer incidence matrix with rows indexed by subsets of size at most , columns indexed by -subsets , and entries . Over the rational numbers, a row with is times the sum of all size- rows containing . Its matrix rank is at most . Every larger integer minor is consequently zero and remains zero modulo , giving the same bound over . The nonzero diagonal evaluation matrix of the then forces .
The theorem, proved by Frankl and Wilson in 1981, extends the theme of the Ray-Chaudhuri–Wilson theorem from ordinary intersection sizes to residues. Modular restrictions can be weaker than exact intersection restrictions yet still force unexpectedly small families. Here are three consequences from one explicit modular intersection graph.
Take , , and let the vertices be all -subsets of , with an edge exactly when the intersection has size . An independent set avoids the only possible off-diagonal intersection congruent to modulo , so applying the Frankl-Wilson theorem with givesA clique has one exact intersection size. Apply the uniform theorem modulo a prime larger than , with , to get . Since there are vertices, this gives the explicit asymmetric Ramsey number bound . It illustrates how algebraic constructions produce graphs with simultaneously restricted cliques and independent sets.
For a geometric application, map each vertex to in . Then , so edges have unit Euclidean distance. Every proper colouring of Euclidean space therefore colours this finite graph, givingThe Stirling formula gives the ratio as , where is the binary entropy function in natural-log units. The positive constant proves an exponential chromatic number of Euclidean space lower bound along these dimensions.
Finally, a quadratic embedding converts this same forbidden intersection into a forbidden diameter pair. Set and . The quadratic sign-vector diameter formula follows from the Frobenius inner product:For distinct members the smallest possible absolute inner product is one, attained exactly when the intersection is . Thus maximum-distance pairs are exactly edges of . The matrices have common diagonal; using their off-diagonal coordinates, multiplied by , realizes them isometrically in dimensions. They are distinct because equal outer products require , and complements have size , not .
Any subset of smaller diameter contains at most points, so a partition into smaller-diameter pieces needs at least pieces. For sufficiently large primes this exceeds , disproving the Borsuk conjecture. This is the mechanism behind the Kahn-Kalai counterexample to the Borsuk conjecture: the number of required pieces grows exponentially in the original set-system parameter while dimension grows quadratically. Their 1993 paper establishes the resulting high-dimensional counterexample.
Past exam of the mathematics course of the University of Cambridge 2005 iii Paper 28 2 i Solution Created 2026-10-03 Updated 2026-10-14
With the normalization of the preceding completion, the super-completion is the Riemann xi functionThe pole-subtracted theta integral for the completed zeta function gives the particularly useful expressionIt proves directly that is an entire function, with and . Here “integral function” means entire, not integer-valued.
To prove the order-one growth of the Riemann xi function, put . For , the exponentially decreasing theta integrand bounds both and byMultiplication by the quadratic factor in and the Stirling formula imply . Hence the order of an entire function is at most one. On the positive real axis, , and the defining formula and Stirling formula giveThis lower bound proves that the order is at least one. Consequently is entire of order exactly one, generally not of finite exponential type.
Its zeros are precisely the Nontrivial zeros of the Riemann zeta function, counted with multiplicity. The values at zero and one are nonzero; the Gamma function has no zeros; and the completed functional equation together with the Euler product shows that there are no further completed zeros outside the closed critical strip. By Hadamard factorization for entire functions of order one,The genus-one factors give , and the logarithmic derivative converges locally normally away from the zeros:Differentiate the defining product of , the gamma factor, and . Rearranging proves the global partial-fraction expansion of the zeta logarithmic derivative:The summands must be kept together: each is for large , whereas separating the two complex reciprocal sums need not preserve absolute convergence. The gamma term accounts for the trivial zeros as well as cancellation at zero.
Past exam of the mathematics course of the University of Cambridge 2006 iii Paper 28 1 Solution Created 2026-10-03 Updated 2026-10-14
Write and for the two Chebyshev functions, and for the prime-counting function. If , the prime divides the central binomial coefficient . ConsequentlySum this inequality over dyadic integers . It gives . Monotonicity, with , gives for real . This is the Chebyshev estimate from central binomial coefficients; no information about the distribution of primes beyond unique factorization has been used.
Split the primes at . For , , soSince ,We also need . The contributions of higher prime powers satisfybecause only contribute, and for .
The Von Mangoldt divisor identity is , which follows by factoring into prime powers. Summing it for , with a positive integer, givesThe bound already proved makes the last error . Integral comparison for , or the Stirling formula, gives . ThereforeThe contribution from higher prime powers is uniformly bounded:Subtract it, and replace by , to obtain the Mertens first theorem
Now fix . Apply partial summation to and . With the lower endpoint interpreted as , so that the prime is included, this givesThe boundary term tends to zero, and the integral converges, since and . Thus the series converges for every positive . Keeping the main term of also gives the useful logarithmically weighted reciprocal-prime tailIndeed, subtract the finite partial sum from the limiting integral: the boundary contributes and the main integral contributes .
Past exam of the mathematics course of the University of Cambridge 2007 iii Paper 12 2 Solution Created 2026-10-03 Updated 2026-10-14
There is a genuine qualification missing from the printed bound. With , the family of three singletons has distinct intersections of size zero, which is not congruent to modulo . Nevertheless its size is three, whereas . Thus that bound cannot hold without a restriction on the parameters. The valid prime-power modular intersection bound isIn particular the printed form holds when .
Put with a prime number, and . If , the corrected bound is simply the total number of -sets. Assume henceforth . For an integer , consider the residue detectorFor nonnegative upper arguments, the Lucas theorem and the fact that every base- digit of equals show that is one when and zero otherwise. The assertion also holds for negative upper arguments, using integer-valued generalized binomial coefficients. Indeed the coefficient of in is periodic in the integer exponent modulo : in characteristic , , so multiplying even a formal power series by does not change coefficients of degrees below . Reduce any exponent modulo to obtain the stated detector.
For each , apply that detector to . Its evaluations on form the identity matrix, since the diagonal intersection is and every off-diagonal intersection has a different residue. The detector is represented on Boolean vectors by the multilinear polynomialTo check this expression, evaluate at the characteristic vector of : summing by gives by the coefficient identity for .
Here is the necessary low-degree evaluation rank on a uniform layer, with care about characteristic . Let be the integer incidence matrix whose rows are subsets of size at most , whose columns are all -sets , and whose entries are . Over the rational numbers, for its row satisfiesThus its rational matrix rank is at most . Every larger square minor has integer determinant zero; reducing those determinants modulo gives too. This argument does not divide by a potentially zero element of the finite field. The identity evaluation matrix factors through these incidence rows, so its rank is at most . This proves the qualified bound.
Choose the two-applications alternative. First, the polynomial method in combinatorics yields a constructive lower bound for a diagonal Ramsey number. Let be prime, set , and use all -subsets of as vertices of a complete graph. Color a pair red when its intersection size is modulo , and blue otherwise. A blue clique has size at most by the proved bound with modulus . In a red clique, all distinct intersections belong toFor each vertex of that clique, the polynomial vanishes at all the other vertices' characteristic vectors and is nonzero at its own. Replace repeated powers by on Boolean vectors. Its degree is at most , so the rational version of the same incidence-rank argument bounds a red clique by as well. Therefore this two-coloring has neither color containing a clique of size , andThe usual estimates give and . Thus along this explicit sequence the diagonal Ramsey number exceeds for some absolute . This is substantially larger than any fixed power of .
Second, obtain an exponential lower bound for the chromatic number of Euclidean space. Let , and join two -subsets exactly when their intersection has size . An independent set in this graph avoids that intersection. Among the possible distinct intersection sizes , the only one congruent to modulo is . Hence every independent set has size at most . Embed each vertex as in Euclidean space. Thenso the graph's edges have exactly Euclidean distance one. Each color class must be an independent set, givingThe Stirling formula makes the logarithm of this ratio , where . Since , this is an exponential dimensional lower bound for the chromatic number of Euclidean space. Both applications lie in the valid parameter range of the proved modular bound.
Past exam of the mathematics course of the University of Cambridge 2010 iii Paper 30 4 a Solution Created 2026-10-03 Updated 2026-10-14
The objective approximates the logarithm of the product-form stationary distribution of a loss network. To make the approximation precise, multiply arrival rates and capacities by and write . The Stirling formula gives, uniformly on the feasible compact set,with . The feasible set is . Positive capacities and a nonempty route for each class make compact with a strictly positive feasible point. Since is a strictly concave function, its maximizer is unique; its infinite inward derivative at makes every component positive.
The Karush-Kuhn-Tucker conditions give nonnegative link Lagrange multipliers satisfyingFor any neighborhood of , continuity and uniqueness give a strictly positive objective gap outside it. There are only polynomially many feasible lattice states, while their weights differ exponentially in . The feasible point has objective tending to . It follows that the stationary law concentrates at on the scale ; in particular,Thus NETWORK predicts the dominant occupancy and mean occupancy in a large loss network. For unscaled inputs it gives a continuous approximation to the modal integer state.
It also gives an exact useful change of variables. Substituting into the equilibrium weights yieldsThis is Poisson exponential tilting for a loss network: independent Poisson random variables centered at the predicted occupancies, restricted to the feasible region and penalized for slack in positively priced resources. It explains why an unconstrained Gaussian approximation should not automatically be applied at a saturated capacity boundary.
Past exam of the mathematics course of the University of Cambridge 2010 iii Paper 44 3 Solution Created 2026-10-03 Updated 2026-10-20
Locally in the space of worldsheet metrics, divide out the volume of worldsheet diffeomorphisms and Weyl transformations. With stabilizer zero modes omitted, the inverse Faddeev-Popov determinant at a metric isThis is the linearized orbit integral: the delta functional is the product of the metric-component delta functions, and its Jacobian is the inverse determinant of the gauge-orbit map. The omitted zero modes and any metric moduli must be handled separately; this local formula is not an integration over the physical moduli themselves.
The trace elimination in string Faddeev-Popov gauge fixing is essential. In two dimensions, split the variation asThe second term is trace-free. Integration over removes the trace delta function, leaving , with the measure understood through the metric inner products. Equivalently, a Fourier representation of the metric delta functional introduces a commuting symmetric tensor . Integration over enforces , and the remaining exponent is proportional to . This gives the same inverse Faddeev-Popov determinant and explains why its tensor variable must be trace-free.
For the Polyakov path integral, insert the gauge-fixing identitywhere is a representative depending on the worldsheet moduli . Gauge invariance of the action, measure, and Faddeev-Popov determinant lets us change variables along the gauge orbit. Its volume cancels the original gauge-group denominator, leaving an integral over , the moduli, and the determinant evaluated at . This is how the determinant enters the numerator of the gauge-fixed integral, despite the inverse determinant occurring in the orbit integral above.
A fermionic Gaussian integral exponentiates using an anticommuting vector and an anticommuting symmetric trace-free tensor :The constant can be absorbed into . In local complex conformal gauge, trace-freeness sets . The only surviving components of the worldsheet diffeomorphism ghost operator are proportional to and . Rescaling the antighost therefore gives exactly the chiral worldsheet ghost actionThe chiral bc ghost system has weights , , with . Its worldsheet stress tensor is . Fermionic double Wick contractions in give the fourth-order coefficient , hence central charge . More generally this calculation gives . Each embedding scalar contributes one, so the total chiral central charge is . The gauge-fixed quantum theory must have no worldsheet Weyl anomaly; consequently the critical dimension of the bosonic string is . Zero-mode insertions for Conformal Killing vector fields and moduli do not change this local anomaly calculation.
For the Veneziano amplitude, first examine an ordered beta-function term. A pole occurs when , with , so the exchanged masses follow the open bosonic string mass spectrumThere is a tachyon at level zero, a massless vector at level one, then an infinite tower with equally spaced squared masses. In oscillator quantization these levels are ; the poles alone do not determine all oscillator degeneracies or all states that might fail to couple to the chosen external particles.
The Veneziano amplitude pole residue gives considerably more information than a pole position. Near , use and . The finite gamma function ratio is a product of linear factors. Thus, for generic ,The empty product at is one. This degree- angular polynomial decomposes into spin partial waves; it reveals the spins that couple, up to maximal spin in the ordered channel, and the corresponding products of three-point couplings. For example, the level-one linear residue encodes vector exchange. A single external-state amplitude need not separate all states with the same mass and spin.
There is a qualification specific to the sum printed in the question. For four identical on-shell tachyons, . At , put . Then , and reversing the product gives . The beta-function term is regular at a generic -channel pole. The residue of the full symmetric amplitude is therefore proportional toThis is odd-level pole cancellation in the symmetric Veneziano amplitude. The fully symmetrized identical-tachyon amplitude has only even-level poles at generic angle, including the tachyon but not the massless vector. This is an external-state selection rule, not removal of odd-level states from the string theory. Ordered amplitudes, or suitable amplitudes with color factors and different external states, retain those exchanges. Thus interpreting every candidate gamma function pole as a pole of the printed sum would give a false inference about that amplitude.
At high energy with fixed, the gamma function reflection formula followed by the Stirling formula gives the fixed-angle softness of an open-string amplitude:up to oscillatory factors and possible additional cancellations. The bracket is positive at a genuinely nonforward fixed angle. This is the envelope away from resonance poles, or the corresponding analytically continued asymptotic regime; it is not a uniform bound through real-axis poles. String scattering is exponentially soft at fixed angle, unlike the typical power-law behavior of point-particle interactions. The finite string length distributes a hard collision over an extended object. This is evidence of improved ultraviolet behavior, not by itself a proof that every loop amplitude is finite. The fixed-angle limit also differs from the fixed- Regge limit.
Past exam of the mathematics course of the University of Cambridge 2012 iii Paper 29 1 Solution Created 2026-10-03 Updated 2026-10-07
Let be the Möbius function. Its Möbius divisor-sum identity isIndeed, for the sum is the expansion of ; nonsquarefree divisors contribute zero. Thus, for arithmetic functions ,To prove Möbius inversion, substitute the first formula into the second and collect the coefficient of . It is , which is one for and zero otherwise. Conversely the same divisor interchange recovers from the displayed formula for . In Dirichlet convolution notation this is simply , where is supported at one.
The Prime number theorem with classical zero-free-region error states that some absolute satisfiesHere is the Von Mangoldt function. An equivalent prime-counting form, after decreasing if needed, is . The contributions of proper prime powers are and can be absorbed into this error. We use to keep it distinct from the Fourier transform appearing in Question 5.
Here is a direct deduction of the requested Mertens bound from a log-integrable Chebyshev error from the stated Prime number theorem. First, the divisor identity givesSecond, the exact Dirichlet convolution identityfollows from : multiplication of a Dirichlet convolution by differentiates its two factors, so applying it to and convolving again with gives this formula. Summing it yieldsThe last harmonic sum is . To see this without an endpoint approximation, split into dyadic ranges . In each range , and its exponential factor is at most . Their sum over converges. The finitely many terms with obey the same estimate after adjusting the constant in the prime-number-theorem error. ThereforeFor the Mertens function ,The second sum has absolute value at most , by an integral comparison or the Stirling formula. ConsequentlyThe absolute value in this conclusion is present in the original PDF.
Past exam of the mathematics course of the University of Cambridge 2012 iii Paper 9 3 i Solution Created 2026-10-03 Updated 2026-10-07
Assume , as required for this nontrivial subcritical binomial random graph. Put . A breadth-first exploration of a binomial random graph is dominated by a Galton-Watson process whose offspring counts are independent random variables with law . If its total progeny is at least , the first offspring counts sum to at least . Their moment-generating function is bounded by that of a Poisson distribution of mean . The exponential Markov inequality, optimized at , yieldsTaking for any fixed , a union bound over all starting vertices gives .
For the matching lower bound, let count tree components of order . The tree-component expectation in the Erdős-Rényi model is exactlyFor , the Stirling formula givesChoose , with . Then . Distinct overlapping vertex sets cannot both be graph components. For disjoint sets, the joint probability differs from the product only because the between-set edges were counted twice as absent. ThusIt follows that . The second moment method gives with high probability. Combining both bounds, and then taking arbitrarily small fixed , proves the sharp subcritical largest-component scaleFinally the Taylor expansion of gives . The endpoint has no edges and is excluded from this logarithmic asymptotic.
Past exam of the mathematics course of the University of Cambridge 2013 iii Paper 67 1 b Solution Created 2026-10-03 Updated 2026-10-07
Watson's lemma applies to Laplace-type endpoint integrals such as as , when has a local algebraic expansion with and suitable integrability or exponential-growth control away from the endpoint. Each term contributes . The exponential selects a neighborhood of .
Laplace method instead treats by locating the dominant maxima of a real phase . A smooth nondegenerate interior maximum produces a neighborhood governed by a Gaussian function of width ; endpoint or degenerate maxima require their corresponding local scaling. Contributions away from a strict dominant maximum must be smaller. These methods overlap after suitable changes of variable, but their usual starting forms emphasize an endpoint amplitude expansion and an exponential maximum, respectively.
For the Gamma function, put . ThenThe phase has its unique maximum at , with value and second derivative . Set . Near this maximum,Combining the amplitude and exponential expansions in Laplace method givesLocalization near justifies extending the limits for the Gaussian integral; the distant endpoint is not being expanded uniformly by this local series. Odd terms integrate to zero. The moments of the Gaussian integral satisfy , , , so the relative correction isThe two terms of the Stirling formula, obtained by the Stirling correction by Gaussian moments, are therefore
Past exam of the mathematics course of the University of Cambridge 2016 ib Paper 1 20H a Solution Created 2026-09-24 Updated 2026-10-06
A Markov chain is irreducible if every state can reach every other state in finitely many steps with positive probability. It is a recurrent Markov chain if, starting at any state, it returns to that state with probability one; for an irreducible chain this property is shared by all states.
For the simple symmetric random walk on , taking steps all in the appropriate direction reaches from with probability . Thus the chain is irreducible. Its return probabilities areBy Stirling formula, , so their sum diverges. The standard recurrence criterion therefore proves the walk is recurrent.
The printed hint's constant is erroneous: the actual limit of is . Its positivity is what the recurrence argument requires, but the reciprocal is necessary for the correct numerical value.
Past exam of the mathematics course of the University of Cambridge 2016 iii Paper 306 3 ii Solution Created 2026-10-03 Updated 2026-10-06
In a point-particle description of quantum gravity, interactions of a massless spin-two field occur at localized vertices of Feynman diagrams. The gravitational coupling has negative mass dimension for spacetime dimension greater than two, so short-distance loop integrations generate higher-derivative counterterms that cannot all be absorbed into the Einstein action. A string worldsheet instead joins incoming and outgoing strings by a smooth surface. In particular, a closed string splits or joins through a smooth pair-of-pants surface. There is no invariantly distinguished point at which every part of an extended string interacts. The choice of a time slicing can draw a joining point, but it is not a physical pointlike vertex. This removes the point-interaction geometry responsible for arbitrarily localized interactions and introduces the string length .
This geometric explanation is supported by the organization of the Polyakov path integral. Introducing a worldsheet metric makes the Nambu–Goto action amenable to gauge fixing. In the Euclidean integral, metrics on a fixed oriented surface are divided by worldsheet diffeomorphisms and Weyl transformations. What remains is a Riemann surface with a conformal structure, together with finitely many worldsheet moduli and the positions of external string vertex operators. The determinants from fixing the metric are represented by Faddeev-Popov ghosts. Schematically, for closed-string external states,Here is the moduli space of genus- punctured surfaces. The dilaton weights a surface by its Euler characteristic , giving before the normalization of external states. Every additional handle multiplies the contribution by . The string genus expansion therefore plays the role of the ordinary loop expansion, with the sphere giving tree level and the torus giving one loop. The critical dimension cancels the worldsheet Weyl anomaly, making this reduction to conformal geometry consistent.
The massless symmetric traceless closed-string state is a graviton, and its long-wavelength interactions reproduce gravity. At distances comparable with , however, an infinite tower of excited states contributes. This is more than a single particle form factor: the same amplitude contains graviton exchange, massive higher-spin exchange and string-scale softness.
The dimensionless variables in the given Virasoro–Shapiro amplitude correspond to , , , where capital letters denote the usual dimensionful Mandelstam invariants. Its constraint identifies the external particles as the closed bosonic tachyons, not four gravitons. Nevertheless its intermediate massless pole directly exhibits graviton exchange. The overall normalization will be suppressed below; no additional copy of the amplitude formula is needed.
First, the amplitude is symmetric under permutations of , expressing crossing symmetry. The poles in any channel areFor generic , the residue can be calculated with the Gamma function pole at and its recurrence:The product is when . Indeed, the pole factor contributes , while the two remaining Gamma ratios contribute . A residue polynomial of degree shows exchange of spins up to , with leading Regge trajectory . At , the massless residue is , containing the spin-two exchange. By crossing, the massless -channel pole isfor generic . Thus at large the pole behaves as , the characteristic energy dependence of graviton exchange. Its massless propagator produces the long-range gravitational interaction. At low energies the massive poles can instead be expanded into local higher-derivative corrections to the effective gravitational action.
At the string scale one must retain the whole tower. The Gamma reflection formula rewrites the amplitude exactly asAt large and fixed , away from the resonance poles or with a specified complex continuation, the Gamma ratio scales as . Hence the Regge limit scales as , up to the signature factor and the displayed -dependent coefficient. In particular, a fixed nonzero momentum transfer changes the point-graviton power law by a factor : the graviton belongs to an entire trajectory rather than remaining an isolated spin-two exchange at arbitrarily high energy.
There is stronger suppression when the scattering angle is fixed. Put , with . Applying Stirling formula to the Gamma functions, after the same treatment of real-axis poles, gives the leading smooth envelopeThe leading terms cancel and the remaining entropy-like combination is negative. In physical units the exponent is . This fixed-angle softness of the closed-string amplitude is absent for an elementary pointlike gravitational vertex. Equivalently, short-distance gravitational scattering probes additional string degrees of freedom. In a four-dimensional long-distance effective setting, a massive exchanged mode contributes a Yukawa-type correction proportional to , with couplings and tensor factors depending on the external states. Such terms are suppressed for and become relevant for . The amplitude establishes the spectrum and short-distance change; it does not by itself give a universal static potential for arbitrary sources. Its bosonic tachyon also signals an unstable vacuum, so it must not be treated as a complete stable model of a gravitational force.
Finally, the modular group prevents overcounting equivalent surfaces and reorganizes the loop ultraviolet region. A torus is with . A change of lattice basis identifiesThus the one-loop integral uses a fundamental domain for , for exampleThe measure is invariant, and the physical integrand, including matter, ghosts and external insertions, must respect torus modular invariance. In this domain . The region of arbitrarily small proper time that causes ultraviolet divergences in a particle loop is therefore not an independent part of the string integral; a modular transformation relates it to another description already represented in the domain.
This does not remove every possible divergence. The cusp is a long tube, and factorization through it can produce infrared divergences, massless tadpoles or the bosonic tachyon divergence. At higher genus, degenerating cycles similarly factorize into propagating intermediate string states. The essential improvement is the relation between worldsheet geometry, the full spectrum and the quotient by large diffeomorphisms; infrared and unstable-background problems remain separate questions. A short-distance expansion that keeps only the graviton discards precisely this structure.
Past exam of the mathematics course of the University of Cambridge 2017 ib Paper 4 9H Solution Created 2026-09-24 Updated 2026-10-05
Let and let each increment of the simple symmetric random walk be uniformly chosen from . A return requires an even number of steps. In steps returning to zero, let be the respective numbers of positive steps in the three directions; there must also be negative steps, so . Counting step sequences givesThe terms form a multinomial distribution, so . The permitted combinatorial inequalities give and for . The second bound also follows by noting that the largest multinomial coefficient occurs when differ by at most one and then applying Stirling formula. ThusTo prove the origin is a transient state, let be the probability of at least one return after time zero. The Strong Markov property at successive returns gives for the number of later returns. Therefore would be infinite if . The bound forces , proving that the origin is a transient state. Translation invariance gives the same conclusion at every lattice point. The coordinate walks need not be treated as independent; the counting via multinomial coefficients already incorporates their dependence.