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On some hyperelliptic Hurwitz–Hodge integrals

Published online by Cambridge University Press:  23 February 2023

DANILO LEWAŃSKI*
Affiliation:
Università di Trieste, Dipartimento di Matematica e Geoscienze, via Valerio 12/1, 34127, Trieste, Italy. Université de Genève, Section des Mathématiques, rue de Conseil General 7, 1206, Genève, Switzerland. e-mail: danilo.lewanski@ihes.fr
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Abstract

We address Hodge integrals over the hyperelliptic locus. Recently Afandi computed, via localisation techniques, such one-descendant integrals and showed that they are Stirling numbers. We give another proof of the same statement by a very short argument, exploiting Chern classes of spin structures and relations arising from Topological Recursion in the sense of Eynard and Orantin.

These techniques seem also suitable to deal with three orthogonal generalisations: (1) the extension to the r-hyperelliptic locus; (2) the extension to an arbitrary number of non-Weierstrass pairs of points; (3) the extension to multiple descendants.

Type
Research Article
Creative Commons
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Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of Cambridge Philosophical Society

1. Introduction

Moduli spaces of curves have been proved in the last decades to be of great interest not only for pure Algebraic Geometry, but a key element at the crossroad of Gromov–Witten theory, Integrable Systems, Random Matrix Models, Topological Recursion, and more.

An important task is the computation of intersection numbers. To fix the ideas, one could think of intersection numbers as integrals packed in polynomials P of the following form:

(1·1) \begin{equation}P(x_1, \dots, x_n) = \int_{\mathcal{M}(g,n)} \frac{\mathcal{C}}{\prod_j (1 - \psi_j x_j)} \cdot [\Delta] \in \mathbb{Q}[x_1, \dots, x_n], \qquad \quad \deg P \leq \dim \mathcal{M}(g,n).\end{equation}

Here $\mathcal{M}(g,n)$ is some moduli space of curvesFootnote 1 , either compact or with a virtual fundamental class, $\mathcal{C}$ is a cohomology class of $\mathcal{M}(g,n)$ Footnote 2 , $[\Delta]$ is a locus of curves of $\mathcal{M}(g,n)$ Footnote 3 , $\psi$ -classes are building blocks of $H^*(\mathcal{M}(g,n))$ of complex degree one, and $x_i$ are formal variables.

We study the following intersection numbers, expressable in three different but equivalent ways. We refer to [ Reference Afandi2 , Reference Cavalieri5 , Reference Jonathan17 ] and references therein for an exhaustive state-of-the-art.

  1. (1) In terms of the hyperelliptic locus $\overline{\mathcal{H}}_{g, 2g + 2, a} \subseteq \overline{\mathcal{M}}_{g, 2g + 2}$ of algebraic curves admitting a degree 2 map to $\mathbb{P}^1$ , with $2g+2$ marked Weierstrass points and a pairs conjugated by the involution, and $\lambda_i = c_i(\mathbb{E})$ the ith Chern class of the Hodge bundle (see [ Reference Afandi1 ] for more details):

    (1·2) \begin{equation}\int_{\overline{\mathcal{H}}_{g, 2g + 2, 2^{a}}} \lambda_i \operatorname{br}^*\left( \prod_{j=1}^{2g + 2+a} \frac{1}{(1 - \psi_j x_j)} \right) ,\end{equation}
    where $\operatorname{br}$ is the map associating to each hyperelliptic curve its target.
  2. (2) In terms of admissible covers and the Hodge class (see [ Reference Johnson, Pandharipande and Tseng15 ] for more details):

    (1·3) \begin{equation}\int_{\overline{\mathcal{M}}_{0, \emptyset - (1^{2g + 2}, 0^{a)}}(\mathbb{B}\mathbb{Z}_r)} \frac{\lambda_i,}{\prod_{j=1}^{2g + 2+a} (1 - x_j\psi_j) } , \qquad \qquad \text{ for } r=2.\end{equation}
  3. (3) In terms of the moduli space of stable curves and the $\Omega$ -CohFT (see [ Reference Lewanski, Popolitov, Shadrin and Zvonkine18 ] and Section 2):

    (1·4) \begin{equation}\int_{\overline{\mathcal{M}}_{0, 2g + 2 + a}} \frac{[\deg_{H^{*}} = i].\Omega(r,0;\; \overbrace{1, \dots, 1}^{2g + 2+a}, \overbrace{0, \dots, 0}^{a})}{\prod_{j=1}^{2g + 2} (1 - \psi_j x_j)}, \qquad \qquad \text{ for } r=2.\end{equation}

The equivalence between the first and the second is well known, the equivalence between the second and the third, for arbitrary r, is achieved in [ Reference Lewanski, Popolitov, Shadrin and Zvonkine18 ]. This restatement was then employed to address a problem by Goulden–Jackson–Vakil over the existence of an ELSV formula for double Hurwitz numbers with one total ramification [ Reference Do and Lewanski8 ]. A really useful Sage package has recently been developed to perform intersection theoretic calculations otherwise by far out of reach with traditional methods [ Reference Delecroix, Schmitt and van Zalm7 ].

1·1. Results

Progress on the evaluation of these integrals was recently made in the following formula:

Theorem 1·1 ([ Reference Afandi1 ]). Linear-Hodge one-descendant integrals over the hyperelliptic locus evaluate to:

\begin{align*}& \int_{\overline{\mathcal{H}}_{g, 2g + 2}}\operatorname{br}^*\left( \psi_1^{2g - 1 - i} \right) \lambda_i = \frac{1}{2} \cdot e_i\left(0 + {1}/{2}, 1 + {1}/{2}, \ldots, g-1 + {1}/{2} \right), \\[5pt] & \int_{\overline{\mathcal{H}}_{g, 2g + 2, 2}}\operatorname{br}^*\left( \psi_{2g + 3}^{2g - i} \right) \lambda_i = \frac{1}{2} \cdot e_i(1, 2, \ldots, g).\end{align*}

Here $ e_i(x_1, \ldots, x_n)$ is the $i{th}$ elementary symmetric polynomial. Footnote 4

The theorem is achieved via virtual localisation techniques. We provide a very short new proof in Section 3, exploiting $\Omega$ -classes and certain vanishings arising from the theory of Topological Recursion in the sense of Eynard and Orantin, introduced in Section 2.

This result opens up natural questions about its generalisations in at least three ‘orthogonal’ directions:

  1. (Q1) What happens to the integrals over hyperelliptic loci with an arbitrary number of non-Weierstrass pairs of points $\overline{\mathcal{H}}_{g, 2g + 2, 2^a}$ ?

  2. (Q2) The hyperelliptic locus ${\overline{\mathcal{H}}_{g, 2g + 2}}$ naturally corresponds to r-admissible covers to the classifying space $B\mathbb{Z}_r$ for $r=2$ . How do these integrals behave for higher r?

  3. (Q3) How does the theory with multiple descendants behave?

We address all three questions with the same techniques with which we give a new proof of the theorem above. We provide and prove answers in certain regimes.

The answer to (Q1) is readily obtained.

Proposition 1·2. The integrals do not depend on the additional number a of non-Weierstrass pairs marked:

\begin{align*}& \int_{\overline{\mathcal{H}}_{g, 2g + 2, 2^a}}\operatorname{br}^*\left( \psi_1^{2g - 1 - i + a} \right) \lambda_i = \frac{1}{2} \cdot e_i\left(0 + {1}/{2}, 1 + {1}/{2}, \ldots, g-1 + {1}/{2} \right), \\[5pt] & \int_{\overline{\mathcal{H}}_{g, 2g + 2, 2^{a+1}}}\operatorname{br}^*\left( \psi_{2g + 3}^{2g - i + a} \right) \lambda_i = \frac{1}{2} \cdot e_i(1, 2, \ldots, g).\end{align*}

The answer to Q2 is obtained under certain restrictions on the parametrisations, which we show to be in general sharp.

Theorem 1·3. For arbitrary r and one descendant, if

(1·5) \begin{equation}\max \limits_{i \neq j} (b_i + b_j) \leq r, \end{equation}

then

(1·6) \begin{align}& \int_{{\overline{\mathcal{M}}}_{0,1 + \ell}}\!\!\!\! [\deg_{H^*} = i].\Omega_{0,n}^{[-1]}(r,0;\; -\overline{\mu_1}, b_1, \dots, b_{\ell}) \psi_1^{\ell - 2 -j} = \nonumber\\[5pt] &\frac{1}{r} e_i\left( \frac{\langle \mu \rangle}{r}, \frac{\langle \mu \rangle}{r} + 1, \dots, \frac{\langle \mu \rangle}{r} + [b] - 1 \right).\end{align}

Here $\sum_j b_j = b = [b]r + \langle b \rangle$ , with $0 \leq \langle b \rangle \leq r-1$ by Euclidean division, similarly for $\mu$ . Moreover, $-\overline{\mu_i}$ is the only representative of $-\mu_i$ modulo r between zero and $r-1$ .Footnote 5

The answer to (Q3) can be given for both generalisations at the same time – that is, for arbitrarily many descendants and for arbitrary r – but imposing $b=\emptyset$ . The formula to compute these integrals is achieved simply by chaining together several existing results, and then simplifying the outcome by the genus-zero restriction. We explain and combine these results in Section 3. Meanwhile we give here a temporary statement.

Proposition 1·4. Let $2g - 2 + n \gt0$ and let r be a positive integer. Fix remainder classes

\begin{align*} -\overline{\mu_1}, \dots, -\overline{\mu_n} \in \{0, \dots, r-1\}. \end{align*}

Then for $\mu_i = \langle \mu_i \rangle + r[\mu_i]$ with $\langle \mu_i \rangle = r - (\!-\!\overline{\mu_i}) $ we have:

(1·7) \begin{equation}\int_{{\overline{\mathcal{M}}}_{0,n}}\frac{\Omega_{0,n}(r,0;\; -\overline{\mu_1}, \dots, -\overline{\mu_n})}{\prod_{i}(1 - \frac{\mu_i}{r}\psi_i)} = \left(\prod_{i=1}^{n} \frac{\left(\frac{\mu_i}{r}\right)^{[\mu_i]}}{[\mu_i]!} \right)^{-1} \!\! \cdot c\sum_{P \in CP}^{\text{finite}} \prod_{l=1}^{\text{finite}} (|I_{l}^{P}||L_{l}^{P}| - |J_{l}^{P}||K_{l}^{P}|).\end{equation}

Here c is an explicit combinatorial prefactor, and $|I_{l}^{P}| \;:\!=\; \sum \mu_{i_l}$ for $i_l$ belonging to the subset $I^{P}_l \subset \{1, \dots, n\}$ .

Moreover, there exists a polynomial $P_{\overline{\mu}}(x_1, \dots, x_n)$ of degree $n-3$ depending on the remainder classes $\overline{\mu_i}$ such that the evaluation $P_{\overline{\mu}}(\mu_1, \dots, \mu_n)$ recovers the expression above.

1·2. Plan of the paper

In the next section we provide the necessary background on $\Omega$ -classes and in Section 3 we prove the four statements above. In Section 4 we provide examples and counterexamples of the statements above.

2. Background

In [ Reference Mumford20 ], Mumford derived a formula for the Chern character of the Hodge bundle on the moduli space of curves $\overline{\mathcal{M}}_{g,n}$ in terms of tautological classes and Bernoulli numbers. Such class appears in the celebrated ELSV formula [ Reference Ekedahl, Lando, Shapiro and Vainshtein10 ], named after its four authors Ekedahl, Lando, Shapiro, Vainshtein, that is an equality between simple Hurwitz number and an integral over the moduli space of stable curves.

A generalisation of Mumford’s formula was computed in [ Reference Chiodo6 ]. The moduli space $\overline{\mathcal{M}}_{g,n}$ is substituted by the proper moduli stack $\overline{\mathcal{M}}_{g;\;a}^{r,s}$ of rth roots of the line bundle

(2·1) \begin{equation} \omega_{\log}^{\otimes s}\biggl(-\sum_{i=1}^n a_i p_i \biggr),\end{equation}

where $\omega_{\log} = \omega(\sum_i p_i)$ is the log-canonical bundle, r and s are integers with r positive, and $a = (a_1, \ldots, a_n) \in \{ 0,\ldots,r-1 \}^n$ is an integral n-tuple satisfying the modular constraint

(2·2) \begin{equation}a_1 + a_2 + \cdots + a_n \equiv (2g-2+n)s \pmod{r}.\end{equation}

This condition guarantees the existence of a line bundle whose r-th tensor power is isomorphic to $\omega_{\log}^{\otimes s}(\!-\!\sum_i a_i p_i)$ . Let $\pi \colon \overline{\mathcal{C}}_{g;\;a}^{r,s} \to \overline{\mathcal{M}}_{g;\;a}^{r,s}$ be the universal curve, and $\mathcal{L} \to \overline{\mathcal C}_{g;\;a}^{r,s}$ the universal rth root. In complete analogy with the case of moduli spaces of stable curves, one can define $\psi$ -classes and $\kappa$ -classes. There is moreover a natural forgetful morphism

(2·3) \begin{equation}\epsilon \colon\overline{\mathcal{M}}^{r,s}_{g;\;a}\longrightarrow\overline{\mathcal{M}}_{g,n}\end{equation}

which forgets the line bundle, otherwise known as the spin structure. It can be turned into an unramified covering in the orbifold sense of degree $2g - 1$ by slightly modifying the structure of $\overline{\mathcal{M}}_{g,n}$ , introducing an extra ${\mathbb{Z}}_r$ stabilizer for each node of each stable curve (see [ Reference Janda, Pandharipande, Pixton and Zvonkine13 ]).

Let $B_m(x)$ denote the mth Bernoulli polynomial, that is the polynomial defined by the generating series

(2·4) \begin{equation}\frac{te^{tx}}{ e^t - 1} = \sum_{m=0}^{\infty} B_{m}(x)\frac{t^m}{m!}.\end{equation}

The evaluations $B_m(0) = (\!-\!1)^m B_m(1) = B_m$ recover the usual Bernoulli numbers. The following formula provides an explicit formula for the Chern characters of the derived pushforward of the universal rth root $\operatorname{ch}_m(r,s;\;a) = \operatorname{ch}_m(R^{\bullet} \pi_{\ast}{\mathcal L})$ . The formula was obtained by Mumford for $r=1$ and $s=1$ [ Reference Bini3 ], then generalised by Bini to arbitrary integers s [ Reference Bini3 ], then generalised by Chiodo to arbitrary positive integers r.

Theorem 2·1 ([ Reference Chiodo6 ]). The Chern characters $\operatorname{ch}_m(r,s;\;a)$ of the derived pushforward of the universal rth root have the following explicit expression in terms of $\psi$ -classes, $\kappa$ -classes, and boundary divisors:

(2·5) \begin{equation} \operatorname{ch}_m(r,s;\;a)= \frac{B_{m+1}(\tfrac{s}{r})}{(m+1)!} \kappa_m - \sum_{i=1}^n \frac{B_{m+1}(\tfrac{a_i}{r})}{(m+1)!} \psi_i^m + \frac{r}{2} \sum_{a=0}^{r-1} \frac{B_{m+1}(\tfrac{a}{r})}{(m+1)!} \, j_{a,\ast} \frac{(\psi')^m - (\!-\!\psi'')^m}{\psi' + \psi''}.\end{equation}

Here $j_a$ is the boundary morphism that represents the boundary divisor with multiplicity index a at one of the two branches of the corresponding node, and $\psi',\psi''$ are the $\psi$ -classes at the two branches of the node.

We can then consider the family of Chern classes pushforwarded on the moduli spaces of stable curves

(2·6) \begin{equation} \Omega_{g,n}^{[x]}(r,s;\;\vec{a}) = \epsilon_{\ast} \exp{\Biggl( \sum_{m=1}^\infty (\!-\!1)^m x^{m} (m-1)! \, \operatorname{ch}_m(r,s;\;\vec{a}) \Biggr)} \in H^{\text{even}}(\overline{\mathcal{M}}_{g,n}).\end{equation}

We will omit the variable x when $x = 1$ .

Corollary 2·2. [Reference Janda, Pandharipande, Pixton and Zvonkine13] The class $\Omega_{g,n}^{[x]}(r,s;\;\vec{a})$ is equal to

\begin{align*} \hspace{-1pt}\sum_{\Gamma\in {\textsf{G}}_{g,n}} \sum_{w\in {\textsf{W}}_{\Gamma,r,s}}\!\frac{r^{2g-1-h^1(\Gamma)}}{|\operatorname{Aut}(\Gamma)| }\;\xi_{\Gamma *}\!\Bigg[ \!\prod_{v \in V(\Gamma)} \!e^{-\sum\limits_{m = 1} (\!-\!1)^{m-1} x^m \frac{B_{m+1}(s/r)}{m(m+1)}\kappa_m(v)} \! \cdot \prod_{i=1}^n e^{\sum\limits_{m = 1}(\!-\!1)^{m-1} x^m \frac{B_{m+1}(a_i/r)}{m(m+1)} \psi^m_{i}} \cdot \\[5pt] \hspace{+10pt}\prod_{\substack{e\in E(\Gamma) \\ e = (h,h')}}\frac{1-e^{\sum\limits_{m \geq 1} (\!-\!1)^{m-1} x^m \frac{B_{m+1}(w(h)/r)}{m(m+1)} [(\psi_h)^m-(-\psi_{h'})^m]}}{\psi_h + \psi_{h'}} \Bigg]\, .\end{align*}

Here $B_{m+1}(y)$ are Bernoulli polynomials, ${\textsf{G}}_{g,n}$ is the finite set of stable graphs of genus g with n legs, ${\textsf{W}}_{\Gamma,r,s}$ is the finite set of decorating the leg i with $a_i$ and any other half-edge with an integer in $\{0, \dots, r-1\}$ in such a way that decorations of half-edges of the same edge ( $e \in E(\Gamma)$ ) sum up to r and locally on each vertex ( $v \in V(\Gamma)$ ) the sum of all decorations is congruent to $(2g - 2 + n)s$ modulo r.

Remark 2·3. By looking at the formula above is it easy to deduce a few properties of the classes $\Omega$ , see [ Reference Giacchetto, Lewanski and Norbury12 ] for a more exhausive list. For instance, $\Omega^{[x]}(r,r;\;\vec{a}) = \Omega^{[x]}(r,0;\;\vec{a})$ , as Bernoulli polynomials satisfy $B_{m+1}(0) = B_{m+1}(1) = B_{m+1}$ . Similarly by $B_{m+1}(1 - X) =$ $(\!-\!1)^{m+1}B_{m+1}(X)$ and Newton identities one can show that $\Omega^{[x]}(r,s;\;a_1, \dots, a_i + r, \dots, a_n) = \Omega^{[x]}(r,s;\;a_1, \dots, a_n) \cdot \left( 1 + \frac{a_i}{r}\psi_i \right)$ .

2·1. Riemann–Roch for $\Omega$ -classes

The Riemann–Roch theorem for an r-th root L of $\omega_{\log}^{\otimes s}(\!-\!\sum_i a_i p_i)$ provides the following relation:

(2·7) \begin{equation} \frac{(2g - 2 + n)s - \sum_i a_i}{r} - g + 1 = h^0(C,L) - h^1(C,L).\end{equation}

In some cases, i.e. for particular parametrisations of $r,s,a_i$ and for topologies (g,n), it can happen that either $h^0$ or $h^1$ vanish, turning $\Omega$ into an actual total Chern class of a vector bundle, so that the Riemann–Roch equation provides the rank of this bundle. If that happens, the Riemann–Roch equation provides a bound for the complex cohomological degree of $\Omega$ :

(2·8) \begin{equation}[\!\deg_{H^*} = k].\Omega_{g,n}(r,s;\;\vec{a}) = 0, \qquad \qquad \text{ for } k \gt \operatorname{rank}(R^{\bullet} \pi_{\ast}{\mathcal L}),\end{equation}

which are usually trivial or not depending on whether the rank $\lt 3g - 3 + n$ . One of these instances of parametrisations is provided by the following result of Jarvis, Kimura, and Vaintrob.

Theorem 2·4 ([ Reference Jarvis, Kimura and Vaintrob14 , proposition 4.4]). Let $g=0$ , let $s=0$ , let $n \geq 3$ , consider $a_i$ all strictly positive except at most a single $a_j$ which can be positive, or zero, or equal to $-1$ . Then the rth universal root does not have any global section, that is, we have

\begin{align*} h^0 = 0. \end{align*}

Under the condition of the theorem above, the rank of $R^{\bullet} \pi_{\ast}{\mathcal L}$ equals $h^1$ , and therefore one gets:

(2·9) \begin{equation}[\deg_{H^*} = k].\Omega_{0,n}(r,s;\;\vec{a}) = 0, \qquad \qquad \text{ for } k \gt \frac{\sum_i a_i }{r} - 1.\end{equation}

2·2. String equation for $\Omega$ -classes

It is known [ Reference Giacchetto, Lewanski and Norbury12 , Reference Lewanski, Popolitov, Shadrin and Zvonkine18 ] that if $0 \leq s \leq r$ then

(2·10) \begin{equation}\Omega(r,s;\; a_1, \dots, a_{n}, a_{n+1} = s) = \pi^{*}\Omega(r,s;\; a_1, \dots, a_{n}).\end{equation}

By projection formula, this implies the string equation:

(2·11) \begin{equation}\int_{\overline{\mathcal{M}}_{g, n+1}} \frac{\Omega(r,s;\; a_1, \dots, a_{n}, a_{n+1} = s)}{\prod_{i=1}^n (1 - x_i \psi_i)} = (x_1 + \dots + x_n) \int_{\overline{\mathcal{M}}_{g, n}} \frac{\Omega(r,s;\; a_1, \dots, a_{n})}{\prod_{i=1}^n (1 - x_i \psi_i)}.\end{equation}

By Remark 2·3, $s=r$ and $s=0$ are interchangeable.

2·3. Relations for integrals of $\Omega$ -classes arising from Topological recursion

Topological recursion is a universal recursive procedure that produces solutions of enumerative geometric problems (see e.g. [ Reference Eynard11 ] for an introduction). Let us very briefly mention how this can be useful to produce relations between integrals of the $\Omega$ -classes. In [ Reference Borot, Do, Karev, Lewanski and Moskovsky4 ], this machinery was employed to generate double Hurwitz numbers. Although they are by definition polynomials in some formal variables $q_1, \dots, q_r$ taking care of ramification conditions, what is generated by topological recursion are formal power series containing poles in exactly one of these variables, namely $q_r$ . Polynomiality implies that the coefficient of $q_r^{-k}$ for $k \gt 0$ , which can be expressed as linear combinations of $\Omega$ -classes integrals, vanishes. For more details on why $\Omega$ -classes integrals appear in double Hurwitz numbers (relation known as ELSV-type formulae) see e.g. [ Reference Lewanski, Popolitov, Shadrin and Zvonkine18 ]. These vanishing result in the following statement.

Theorem 2·5 ([ Reference Borot, Do, Karev, Lewanski and Moskovsky4 ]). Let $2g - 2 + n + \ell \gt 0$ and let r be a positive integer, and $s=0$ .

  1. (i) Let $1 \leq \mu_1, \dots, \mu_n \leq r$ , and let $\mu$ be their sum.

  2. (ii) Let $1 \leq b_1, \dots, b_{\ell} \leq r-1$ , and let b be their sum.

  3. (iii) Impose $b \equiv \mu \; (\!\!\!\! \mod r)$ . Then we can write $b = \mu + r \cdot \delta$ for some integer $\delta$ .

If

(2·12) \begin{equation}\mu \lt b, \text{ or equivalently, } \delta \gt 0 \qquad \qquad \text{ (negativity), }\end{equation}

then the following finite linear combination of $\Omega$ -integrals vanishes:

(2·13) \begin{align} & \sum_{t = 1}^{\ell} \frac{(\!-\!1)^{\ell - t}}{t!} \!\!\!\sum_{\substack{\boldsymbol{\rho} \in (\mathscr{\tilde{P}}_{r - 1})^{k} \\ \sqcup_{\kappa} \rho^{(\kappa)} = \textbf{b}^{\vee}}}\prod_{\kappa = 1}^{t} \frac{\big[\frac{r - |\rho^{(\kappa)}|}{r}\big]_{\ell(\rho^{(\kappa)}) - 1}}{|\operatorname{Aut}{\rho^{(\kappa)}}|} \nonumber \\[5pt] & \int_{\overline{\mathcal{M}}_{g,n + t}} \!\!\!\!\! \frac{\Omega(r,0;\; - \overline{\mu_1},\dots, - \overline{\mu_n},\dots, r - |{\rho}^{(1)}|, \dots, r - |{\rho}^{(t)}|)}{\prod_{i = 1}^n \big(1 - \frac{\mu_i}{r}\psi_i\big)} = 0.\end{align}

Here $\mathscr{\tilde{P}}_{r - 1}$ is the set of partitions of size at most $r-1$ , the Pochhammer symbol $[x]_a \;:\!=\; x(x-1) \cdots (x- a+1)$ stands for the descending factorial, and $\textbf{b}^{\vee} = (r - b_1, \dots, r - b_{\ell})$ .

In particular, if the condition

(2·14) \begin{equation}\max \limits_{i \neq j}(b_i + b_j) \leq r \qquad \qquad \text{ (boundedness) }\end{equation}

is satisfied, then all summands but a single one (the term for $t=\ell$ and for $|{\rho}^{(\kappa)}| = 1$ for $\kappa = 1, \dots, \ell$ ) straighforwardly disappear in the relation above. In this case we obtain: Footnote 6

(2·16) \begin{equation}\int_{\overline{\mathcal{M}}_{g, n+\ell} } \frac{\Omega(r,0;\; -\overline{\mu_1}, \dots, -\overline{\mu_n}, b_1, \dots, b_{\ell})}{\prod_{i=1}^n (1- \frac{\mu_i}{r}\psi_i)} = 0.\end{equation}

2·3·1. The $r=2$ case

Let us briefly discuss the specialisation of the result above to $r=2$ .

  1. (1) All $b_j$ must equal to one, and therefore $b = \ell$ .

  2. (2) The boundedness condition is always satisfied.

  3. (3) The negativity condition reads $\mu \lt \ell$ .

  4. (4) The strong negativity condition reads $\mu + \delta \lt \ell$

  5. (5) Strong negativity and negativity are equivalent, as $\delta = (\ell - \mu)/2$ .

If (3) or equivalently (4) are satisfied, we have

(2·17) \begin{equation} \int_{\overline{\mathcal{M}}_{g,n + \ell}} \frac{\Omega(2,0;\; -\!\overline{\mu_1}, \dots, -\overline{\mu_n}, 1, 1, \dots, 1)}{\prod_{i=1}^n(1 - \frac{\mu_i}{2}\psi_i)} = 0, \end{equation}

where $-\overline{\mu_i}$ in this case simplifies to the parity of $\mu_i$ (it is one if $\mu_i$ odd, else zero).

3. Proofs

We are now armed to prove the statements presented in the introduction.

3·1. New proof of Theorem 1·1

Proof. Let us first recast Theorem 1·1 as in form of Equation (1.4).

Lemma 3·1. Let x be a formal variable. Theorem 1·1 is equivalent to the following statements.

(3·1) \begin{align}\int_{\overline{\mathcal{M}}_{0,2g + 2}} \frac{\Omega(2,2;\; \overbrace{1, 1, \dots, 1)}^{2g+2}}{(1 - \frac{x}{2}\psi_1)} &= \frac{x^{g-1}}{2^{2g}}\prod_{k=1}^{g}(x - (2k-1)),\end{align}
(3·2) \begin{align}\int_{\overline{\mathcal{M}}_{0,2g + 3}} \frac{\Omega(2,2;\; 0, \overbrace{1,\dots, 1}^{2g+2})}{(1 - \frac{x}{2}\psi_1)} &= \frac{x^{g}}{2^{2g+1}}\prod_{k=1}^{g}(x - 2k). \end{align}

Proof. Simply multiply both sides of both statements of Theorem 1·1 by $(\!-\!1)^i x^i$ and sum over i, then use the general fact for polynomial roots $\prod_{j=1}^d(x - \alpha_j) = \sum_{j=0}^d x^j e_{d-j}(\alpha_i)$ $(\!-\!1)^{d-j}$ , and recast the obtained statements in terms of moduli space of stable curves (from integrals in (1·2) to integrals in (1·4)). This concludes the proof of the Lemma.

Let us now prove Equation (3·1). The LHS in (3·1) is a polynomial $P(x) = c\cdot \prod_{i=1}^{2g-1} (x - \alpha_i)$ , where $\alpha_i$ are the roots. The constant c is immediately computed as $c = [x^{2g-1}].P(x) = 2^{-(2g - 1)} \int_{\overline{\mathcal{M}}_{0,2g + 2}} \psi_1^{2g-1} 2^{-1}= 2^{-2g}$ . It remains to show that zero is a zero of P(x) of order $g-1$ and that $2k-1$ is a simple zero of P(x) for $k = 1, \dots, g$ . The first condition is equivalent to the fact that $\Omega$ has non-trivial cohomological degree at most g. This is indeed true and proved by the Riemann-Roch computation for $\Omega$ in genus zero performed in (2·9): $({2g+2})/{2}-1 =g$ . It only remains to show that $P(2k-1)=0$ for all $k=1, \dots, g$ (in fact, if so, their multiplicity cannot be greater than one by degree constraint). Explicitly, the proof boils down to the following g relations:

(3·3) \begin{equation}\int_{\overline{\mathcal{M}}_{0,2g + 2}} \frac{\Omega(2,2;\; \overbrace{1, 1, \dots, 1)}^{2g+2}}{(1 - \frac{2k-1}{2}\psi_1)} = 0, \qquad \text{ for } k=1, \dots, g.\end{equation}

These relations are immediately implied by Theorem 2·5 specialised as in Equation (2·17), then further specialised to $n=1$ : the vanishing holds for positive odd $\mu_1 \lt 2g + 1$ , or in other words, for $\mu_1 = 2k-1$ for $k=1, \dots, g$ .Footnote 7 Equation (3·2) is proved similarly. This concludes the proof of Theorem 1·1.Footnote 8

3·2. Proofs of Proposition 1·2, Theorem 1·3 and Proposition 1·4

Proof of Proposition 1·2. Again, we start by recasting the result.

Lemma 3·2. Let x be a formal variable. Proposition 1.2 is equivalent to the following statements:

(3·5) \begin{align}\int_{\overline{\mathcal{M}}_{0,2g + 2 + a}} \frac{\Omega(2,2;\; \overbrace{1, \dots, 1}^{2g+2}, \overbrace{0, \dots, 0}^{a})}{(1 - \frac{x}{2} \psi_1)} &= \frac{x^{g-1+a}}{4^{g}}\prod_{k=1}^{g}(x - (2k-1)), \end{align}
(3·6) \begin{align} \int_{\overline{\mathcal{M}}_{0,2g + 3 + a}} \frac{\Omega(2,2;\; 0, \overbrace{1,\dots, 1}^{2g+2}, \overbrace{0, \dots, 0}^{a})}{(1 - \frac{x}{2}\psi_1)} &= \frac{x^{g+a}}{2^{2g+1}}\prod_{k=1}^{g}(x - 2k). \end{align}

Both expressions are polynomials in x of degree equal to the dimension of the moduli spaces, that is, of degree $2g-1+a$ and $2g+a$ respectively.

Proof. The proof is the same as in Lemma 3·1. This concludes the proof of the Lemma.

Now it suffices to apply String Equation (2·11) to each of the last a marked points:

(3·7) \begin{equation}\int_{\overline{\mathcal{M}}_{0,2g + 2 + a}} \frac{\Omega(2,2;\; \overbrace{1, \dots, 1}^{2g+2}, \overbrace{0, \dots, 0}^{a})}{(1 - \frac{x}{2} \psi_1)} = x^a \cdot \int_{\overline{\mathcal{M}}_{0,2g + 2}} \frac{\Omega(2,2;\; \overbrace{1, \dots, 1}^{2g+2})}{(1 - \frac{x}{2} \psi_1)}.\end{equation}

This concludes the proof of the Proposition.

Proof of Theorem 1·3. Consider the polynomial

(3·8) \begin{equation}P (x) \;:\!=\; \int_{{\overline{\mathcal{M}}}_{0,1 + \ell}}\frac{\Omega_{0,n}(r,0;\; -\overline{\mu_1}, b_1, \dots, b_{\ell})}{(1 - \frac{x}{r}\psi_1)} = c\cdot \prod_{i} (x - \alpha_i).\end{equation}

It is a polynomial of degree $\deg(P) = \dim_{\mathbb{C}}({\overline{\mathcal{M}}}_{0,1 + \ell}) = \ell - 2$ , and its leading coefficient can be easily computed as

\begin{align*} c = \int_{{\overline{\mathcal{M}}}_{0,1 + \ell}} \Omega_{0,n}(r,0;\; -\!\overline{\mu_1}, b_1, \dots, b_{\ell})\frac{\psi_1^{\ell-2}}{r^{\ell-2}} = \frac{1}{r^{\ell-2}\cdot r} \int_{{\overline{\mathcal{M}}}_{0,1 + \ell}} \psi_1^{\ell-2} = \frac{1}{r^{\ell - 1}}. \end{align*}

Since $\mu_1 = \mu \equiv b$ modulo r, we must have that $\langle \mu \rangle = \langle b \rangle$ , and therefore $\bar{-\mu_1} = r - \langle \mu \rangle$ . The lowest degree in x of P(x) can be computed as

\begin{align*}\deg(P) - \operatorname{maxdeg}_{H^{*}}\Omega_{0,n}(r,0;\; -\!\overline{\mu_1}, b_1, \dots, b_{\ell}) & = \ell - 2 - \left( \frac{ r - \langle \mu \rangle + [b]r + \langle b \rangle }{r} - 1\right) \\[5pt] & = \ell - 2 - [b]. \end{align*}

So far we achieved to show that P has the form

\begin{align*} P(x) = \frac{x^{\ell - 2 - [b]}}{r^{\ell - 1}}\prod_{i=1}^{[b]}(x - \alpha_i).\end{align*}

for some suitable roots $\alpha_i$ . The question is whether the TR vanishing (2·16) can guarantee at least (and therefore all) [b] roots.Footnote 9 Assuming boundedness, we only have to worry about negativity $\mu \lt b$ holding true, which means that

\begin{align*} \langle \mu \rangle + rk \lt \langle b \rangle + r[b] \end{align*}

for a few possible non-negative integers k. As $\langle \mu \rangle = \langle b \rangle$ , negativity holds true for the values $k=0, \dots, [b]-1$ , which amounts to [b] different values of $\mu$ providing [b] simple roots $P(\langle \mu \rangle + rk) =0$ as required. This concludes the proof of the Theorem.

Proof of Proposition 1·4. As anticipated in the introduction, the proposition is simply obtained by a chain of several known results, simplified in genus zero.

  1. (1) By [ Reference Lewanski, Popolitov, Shadrin and Zvonkine18 , section 5] we have:

    \begin{align*} \int_{{\overline{\mathcal{M}}}_{g,n}}\frac{\Omega_{g,n}(r,0;\; -\overline{\mu_1}, \dots, -\overline{\mu_n})}{\prod_{i}(1 - \frac{\mu_i}{r}\psi_i)} = \int_{{\overline{\mathcal{M}}}_{g,\emptyset - \mu}(\mathcal{B}\mathbb{Z}_r)}\frac{\sum_{i=0} (\!-\!1)^i \lambda_i^U}{\prod_{i}(1 - \frac{\mu_i}{r}\bar{\psi}_i)} \end{align*}
    for U the representation of the cyclic group $\mathbb{Z}_r$ sending 1 to $e^{2\pi i/r}$ .
  2. (2) By [ Reference Johnson, Pandharipande and Tseng15 , theorem 1] we have:

    \begin{align*} h_{g,\mu}^{(r), \circ}= r^{2g - 2 + n + \frac{|\mu|}{r}}\left(\prod_{i=1}^{n} \frac{\left(\frac{\mu_i}{r}\right)^{[\mu_i]}}{[\mu_i]!} \right) \cdot \int_{{\overline{\mathcal{M}}}_{g,\emptyset - \mu}(\mathcal{B}\mathbb{Z}_r)}\frac{\sum_{i=0} (\!-\!1)^i \lambda_i^U}{\prod_{i}(1 - \frac{\mu_i}{r}\bar{\psi}_i)}, \end{align*}
    where $h_{g,\mu}^{(r), \circ}$ are Hurwitz numbers enumerating connected genus g degree $d = |\mu|$ ramified covers of the Riemann sphere with $b = b(g) = 2g - 2 + {|\mu|}/{r} + n$ simple ramifications, except the ramification with profile $(r,r,\dots, r)$ above zero and the ramification with profile $(\mu_1, \dots, \mu_n)$ above infinity, with $n = \ell(\mu)$ . Moreover, the integral is a polynomial of degree $3g - 3 + n$ in the $\mu_i$ depending on the remainder classes $\langle \mu_i \rangle$ modulo r, whereas the exponential prefactor is manifestly not polynomial in the parts $\mu_i$ . This property is known as quasi-polynomiality, and has been shown independently in [ Reference Dunin-Barkowski, Lewanski, Popolitov and Shadrin9 ] in the framework of Topological Recursion.
  3. (3) By Okounkov [ Reference Giacchetto, Lewanski and Norbury12 ] and Okounkov and Pandharipande [ Reference Okounkov and Pandharipande21 ], we have that Hurwitz numbers can be efficiently written as vacuum expectation of operators in the Fock space, which in this case form a handy algebra closed under commutation relations:

    (3·9) \begin{equation}h_{g, \mu}^{(r), \circ} = \frac{[z_1^2 \cdots z_{b(g)}^2]}{\prod \mu_i \cdot r^{d/r}}\Bigg{\langle} \mathcal{E}_{\mu_1}(0) \dots \mathcal{E}_{\mu_n}(0) \mathcal{E}_{0}(z_1) \dots \mathcal{E}_{0}(z_{b(g)}) \mathcal{E}_{-r}(0)^{d/r} \Bigg{\rangle}^{\circ},\end{equation}
    where $[x^a]f(x)$ selects the coefficient of $x^a$ in the formal power series f(x), $b(g) = 2g - 2 + n + d/r$ is the Riemann–Hurwitz count of simple ramifications, and the following relations hold:
    \begin{align*}[\mathcal{E}_{a}(z), \mathcal{E}_b(w)] = 2\sinh \left(\frac{aw - bz}{2}\right) \mathcal{E}_{a+b}(z + w), \end{align*}
    and
    (3·10) \begin{equation} \bigg{\langle} \mathcal{E}_0(z) \bigg{\rangle} = \frac{1}{2\sinh(z/2)}, \qquad \qquad \qquad \mathcal{E}_{k} \bigg{\rangle} = 0 = \bigg{\langle} \mathcal{E}_{-k} , \qquad \text{ for } k \gt0.\end{equation}
  4. (4) By [ Reference Johnson16 ] we have an algorithm that computes the vacuum expectation explicitly, iteratively commuting the operators $\mathcal{E}$ with negative indices from left to right until they hit the vacuum $\big \rangle$ and vanish. Along the way, they generate a large amount of summands from the commutation relation (intuitively speaking, the number of summands “doubles” at every commutation, although many terms end up vanishing at some further iteration of the algorithm). The algorithm defines a finite sum over P running over the set of Commutation Patterns CP (see [ Reference Johnson16 ]), obtaining

    (3·11) \begin{equation}h_{g, \mu}^{(r)} = \frac{[u^{2g - 2 + n + d/r}]}{\prod \mu_i \cdot r^{d/r}}\frac{1}{2\sinh(u\cdot d/2)} \sum_{P \in CP} \prod_{l=1}^{n-1+d/r} 2\sinh \left((u/2)(|I_{l}^P||L_{l}^P| - |J_{l}^P||K_{l}^P|)\right)\end{equation}

    Here each $I^P_t$ , $J^P_t$ , $K^P_t$ , $I^P_t$ is a sum of a certain subset of the $\mu_i$ .

  5. (5) Restricting to genus zero forces to collect the minimal power of u, that is, to substitute all $\sinh (X)$ simply with their arguments X. We obtain:

    (3·12) \begin{equation}h_{0, \mu}^{(r)} = \frac{1}{\prod \mu_i \cdot r^{d/r} \cdot d} \sum_{P \in CP} \prod_{l=1}^{n-1+d/r} (|I_{l}^P||L_{l}^P| - |J_{l}^P||K_{l}^P|).\end{equation}

Putting everything together, one obtains

\begin{align*} & \int_{{\overline{\mathcal{M}}}_{0,n}} \!\!\!\! \frac{\Omega(r,0;\; -\overline{\mu_1}, \dots, -\overline{\mu_n})}{\prod_{i}(1 - \frac{\mu_i}{r}\psi_i)} = \frac{\left(r^{-1}\right)^{2g - 2 + n + 2\frac{|\mu|}{r}}}{\prod \mu_i \cdot d} \\[5pt] & \left(\prod_{i=1}^{n} \frac{\left(\frac{\mu_i}{r}\right)^{[\mu_i]}}{[\mu_i]!} \right)^{-1} \!\!\! \sum_{P \in CP} \prod_{l=1}^{n-1+d/r} (|I_{l}^P||L_{l}^P| - |J_{l}^P||K_{l}^P|).\end{align*}

This concludes the proof fo the Proposition.

Acknowledgements

The author is supported by the SNSF Ambizione Grant “Resurgent topological recursion, enumerative geometry and integrable hierarchies” hosted at the Section de Mathématique de l’Université de Genève. This work is partly a result of the ERC-SyG project, Recursive and Exact New Quantum Theory (“ReNewQuantum”) which received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme under grant agreement No 810573, hosted, in the case of the author, at the Institut de Physique Thèorique Paris (IPhT), CEA, Université de Saclay, and at the Institut des Hautes Études Scientifiques (IHES), Université de Saclay. The author moreover thanks Adam Afandi and Alessandro Giacchetto for useful discussions, Johannes Schmitt for admcycles package support, and the INdAM group GNSAGA for support.

Appendix A. Examples and counterexamples

The following computations have been run through the admcycles Sage package.Footnote 10

A·1. Theorem 1·1 and Question Q1

For $r=2$ and $\mu = 1 + 2k$ we have:

\begin{align*} \frac{1}{x}\int_{\overline{\mathcal{M}}_{0,7}} \frac{\Omega^{[2]}(2,0;\; 1,1,1,1,1,1,0)}{(1 - x\psi_1)} = \int_{\overline{\mathcal{M}}_{0,6}} \frac{\Omega^{[2]}(2,0;\; 1,1,1,1,1,1)}{(1 - x\psi_1)} = \frac 1 2 x (x-1)(x-3). \end{align*}

Note that in general one can reabsorb several powers of r on both sides of Theorem 1·1 and of Proposition 1·2, by rescaling $x \mapsto rx$ and activating the degree parameter of the $\Omega$ -classes.

A·2. Question Q2

We have seen that for $n=1$ there is enough room for negativity to be satisfied so that enough evaluations of $\mu$ provide vanishing for P to be determined. We want here to test boundedness condition.

Let us for instance choose a prime number $r=13$ , so that it does not possibly factorise with anything else. For $\langle \mu_1 \rangle = 9$ we have $-\overline{\mu_1} = 13 - 9 = 4$ and picking a vector $b = (4,3,6,2,7)$ sharply hitting boundedness ( $6+7 = r$ ) we see a confirmation of our expectations:

\begin{align*}\int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(13,0;\; 4,4,3,6,2,7)}{(1 - \frac{x}{13}\psi_1)} = \frac{x^2}{13^4} (x - \alpha), \qquad \qquad \alpha = 9 = \langle \mu_1 \rangle.\end{align*}

We now wiggle a bit the vector b outside boundedness (though preserving both its size and $\langle \mu_1 \rangle$ ), and the theorem immediately fails:

\begin{align*}\int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(13,0;\; 4,4,3,6,1,8)}{(1 - \frac{x}{13}\psi_1)} &= \frac{x^2}{13^4} (x - 8), \\[5pt] \int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(13,0;\; 4,1,2,9,2,7)}{(1 - \frac{x}{13}\psi_1)} & = \frac{x^2}{13^4} (x - 6).\end{align*}

Other curious things can happen. Here we pick $r=3$ and we again exceed boundedness. For $\langle \mu_1 \rangle = 1$ and b high enough to produce two non-zero roots, we find that one is expected and the other is not:

\begin{align*}\int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(3,0;\; 2,1,2,2,1,1)}{(1 - \frac{x}{3}\psi_1)} = \frac{x^1}{3^4} (x - 1)(x-3).\end{align*}

Here for $\langle \mu_1 \rangle = 2$ and b high enough to produce two non-zero roots, we find one expected root, but with unexpected multiplicity:

\begin{align*}\int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(3,0;\; 1,2,2,2,1,1)}{(1 - \frac{x}{3}\psi_1)} = \frac{x^1}{3^4} (x - 2)^2\end{align*}

Also, when $\delta$ is high enough for $\mu_1 = \langle \mu_1 \rangle$ , it is possible that P does not even factorise in $\mathbb{R}$ anymore:

\begin{align*}\int_{{\overline{\mathcal{M}}}_{0,1+5}}\frac{\Omega(3,0;\; 1,2,2,2,2,2)}{(1 - \frac{x}{3}\psi_1)} = \frac{x^0}{3^4} (x-1) \left(x - \frac{1}{2} + i\frac{\sqrt{11}}{2}\right)\left(x -\frac{1}{2} - i \frac{\sqrt{11}}{2}\right).\end{align*}

Footnotes

1 typically the Deligne–Mumford moduli space of stable curves $\overline{\mathcal{M}}_{g,n}$ , but also moduli spaces with enriched structure, such as the space of r-spin curves, of admissible curves, of stable maps to a specific target. Other examples of compactifications for smooth curves are provided by Hassett moduli spaces, which specialise both to the Deligne–Mumford and to the Losev–Manin compactification.

2 typically Cohomological Field Theories (CohFTs) [ Reference Kontsevich and Manin19 ] or top Chern classes of those, or partial CohFTs, F-CohFTs, and so on. Few examples are: Hodge classes, $\Omega$ -classes, Witten classes, double ramification cycle, classes of holomorphic differentials.

3 for instance the locus of hyperelliptic curves and their generalisations, or partial compactification of the space $\mathcal{M}(g,n)$ , such as the locus of rational tails or of compact type curves inside the Deligne–Mumford compactification.

4 These evaluations are in fact half of $(\!-\!1)^{g} \textsf{s}\bigl( g, g - i, {1}/{2} \bigr)$ and of $(\!-\!1)^{g+1} \textsf{s}\bigl( g+1, g+1 - i, 0 \bigr)$ respectively, the generalised Stirling numbers of the first kind.

5 Again, the RHS can be given in terms of Stirling numbers of the first kind as ${1}/{r}(\!-\!1)^{[b]} \textsf{s}\bigl( [b], [b] - i,$ ${\langle \mu \rangle}/{r} \bigr)$ .

6 Some time before Theorem 2·5, a shadow of this statement – already degenerated under both the negativity and the boundedness condition – was derived in [ Reference Johnson, Pandharipande and Tseng15 , theorem 2]. The entire relation in (2·13) does not make its appearance. On the other hand, [ Reference Kontsevich and Manin19 , theorem 2) carries another sufficient condition for (2·16) to hold: this condition is

(2·15) \begin{equation}\mu + \delta < \ell, \; \text{ or equivalently, }\; \mu < \frac{\sum_{j=1}^{\ell} (r - b_j)}{(r-1)} \qquad \qquad \text{ (strong negativity).}\end{equation}

Strong negativity, as the name suggests, implies negativity. However, strong negativity is not weaker nor stronger than the combination of boundedness and negativity: one can find counterexamples of both phenomena, as well as examples of parametrisations satisfying all three conditions. In fact, for the purpose of this work strong negativity does not provide any new information: whenever strong negativity occurs, boundedness also does, therefore Theorem 2·5 suffices.

7 In fact more is true: the relations produced by Theorem 2·5 specialised this way are all and only the relations needed to determine P(x) completely. In order terms, we have just proved that Theorem 1·1 and the specialisation of Theorem 2·5 to the case $r=2, n=1,$ and $\ell$ odd, are completely equivalent statements, this way reproving Theorem 1·1.

8 As a curiosity, we report on a different proof for the first zero of P(x) different from zero. The first vanishing is in some sense geometrically stronger than the subsequent ones. For example:

(3·4) \begin{equation} P(1) = \int_{\overline{\mathcal{M}}_{0,2g + 2}} \frac{\Omega(2,2;\; \overbrace{1, 1, \dots, 1)}^{2g+2}}{(1 - \frac{1}{2}\psi_1)} = \int_{\overline{\mathcal{M}}_{0,2g + 2}} \Omega(2,2;\; \overbrace{-1, 1, \dots, 1)}^{2g+2} = 0. \end{equation}

The first equality is by definition, the second is by first property of the $\Omega$ -classes in Remark 2·3, the third is by Riemann–Roch as in (2·9). The vanishing occurs by integrating the pure Chern class of a vector bundle with rank strictly smaller than the dimension of the space. The following zero does not enjoy this property as $a_1 = -3$ falls outside of the hypotheses of Jarvis, Kimura and Vaintrob in Theorem 2·4.

9 One could wonder whether strong negativity $\mu + \delta \lt \ell$ can also grant a sufficient condition to determine P completely. Curiously, one finds that in this case strong negativity implies boundedness, therefore not providing anything additional. To see this, expand strong negativity as $k \lt({\ell - \langle b \rangle - [b]})/{(r-1)}$ . The best possible case is given for $ \langle b \rangle = 0$ , for which P is determined if the first b values of $\mu$ for $k \in \{0,1,\dots, [b]-1\}$ give vanishing. Substituting the highest $k = [b]-1$ one finds $b \leq \ell + r-2$ . As the parts of b are at least one, write $b = \ell + |\alpha|$ for $|\alpha|$ the size of a partition of length up to $\ell$ to be distributed over the $b_i = 1 + \alpha_i$ . Then $|\alpha| \leq r-2$ , sharply implying boundedness.

10 For $g=2$ (i.e. $n=6$ ), we have run Lagrange interpolation in x using integer values of x in the right modular residue class, and only after computing enough evaluations and interpolating one is allowed to consider the expression as an abstract polynomial, remembering its residue class dependence.

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