Abstract
We study the eigenforms of the action of A. Baker’s Hecke operators on the holomorphic elliptic homology of various topological spaces. We prove a multiplicity one theorem (i.e., one-dimensionality of the space of these “topological Hecke eigenforms” for any given eigencharacter) for some classes of topological spaces, and we give examples of finite CW-complexes for which multiplicity one fails. We also develop some abstract “derived eigentheory” whose motivating examples arise from the failure of classical Hecke operators to commute with multiplication by various Eisenstein series, or non-cuspidal holomorphic modular forms in general. Part of this “derived eigentheory” is an identification of certain derived Hecke eigenforms as the obstructions to extending topological Hecke eigenforms from the top cell of a CW-complex to the rest of the CW-complex. Using these obstruction classes together with our multiplicity one theorem, we calculate the topological Hecke eigenforms explicitly, in terms of pairs of classical modular forms, on all 2-cell CW complexes obtained by coning off an element in \(\pi _n(S^m)\) which stably has Adams–Novikov filtration 1.
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Notes
In [4], Baker remarks “Because our operations are merely additive (and not multiplicative...) they appear to be hard to compute explicitly except in a few simple situations.” In A. Ranicki’s review of [4] on the AMS’s Mathematical Reviews service, Ranicki includes that quotation from Baker’s paper, evidently to emphasize that it indeed seems difficult to calculate Baker’s topological Hecke operators. Part of the purpose of this paper is to remedy this situation, by demonstrating how to calculate the action of Baker’s topological Hecke operators on the elliptic homology of various CW-complexes—specifically, those whose attaching maps are identifiable as classes in the Adams–Novikov spectral sequence with known cocycle representatives in the cobar complex for Brown–Peterson homology—and giving explicit results in a certain reasonable class of examples.
See Proposition 4.6 for a detailed statement.
By convention, we do not count the basepoint as a 0-cell when we say that a 2-cell complex has “two cells”.
Since Baker’s topological Hecke operators are stable operations, we are free to use methods from stable homotopy throughout this paper. Consequently, in the rest of this paper after the introduction, we drop the superscript \({}^{st}\) to indicate stability, and we simply write \(\pi _{*}\) for stable homotopy groups.
Both \(v_1\in \pi _{2p-2}(BP)\) and \(\alpha _1\in \pi _{2p-3}^{st}(S^0)\) depend on the choice of prime p, but the prime p is suppressed from the notation for \(v_1\) and \(\alpha _1\).
BP denotes p-local Brown–Peterson homology, which depends on the prime p, but the prime p is traditionally suppressed from the notation BP. A standard reference is the book [25].
Since 2 and 3 are already inverted in elliptic homology, we need only consider odd primes.
It is a known fact that the kernel of the map \(\pi _*(MU)[1/6]\rightarrow { ell}_*\) is generated by a regular sequence, but it seems to have folklore status: as far as we can tell, at present a proof does not appear in the published literature. It is mentioned preceding Proposition 2.8 in Strickland’s paper [32], and Strickland has written out a proof on the Web [31].
This requires, in particular, that “multiplication by \(p^{-k}\)” is defined on \(E^{2k}(S^0)\). When this happens, it is usually because either \(E^n(S^0)\) is trivial for \(n>0\), or because \(E^*({{\,\mathrm{{pt.}}\,}})\) is a \({\mathbb {Z}}[\frac{1}{p}]\)-module.
To be careful: since these maps of spectra are constructed using Brown representability, they are only defined up to homotopy.
To be absolutely clear about the terminology: when a CW-complex is called “finite-dimensional,” this means it is required to have cells in only finitely many dimensions, although it is allowed to have infinitely many cells in individual dimensions. When a CW-complex is “finite,” this means it has only finitely many cells tout court.
This same result remains true under the weaker assumption that X splits as a finite wedge of spheres after inverting the primes in P.
We remind the reader that here, and everywhere else throughout this paper, all modular forms are assumed to be of level 1. Analogous results at higher level are provable by similar methods.
Since elliptic homology is a generalized homology theory and Baker’s Hecke operations are stable operations, we have a natural isomorphism \({ ell}_*(\Sigma X) \cong { ell}_{*-1}(X)\), i.e., \({ ell}^*\) turns (de)suspensions into shifts of grading, and consequently the collection of Hecke eigenforms over X is a stable homotopy invariant of X. In particular, only the stable homotopy class of an attaching map in a CW-complexes has an effect on the Hecke eigenforms over that CW-complex.
Throughout, we will write “comodule” as shorthand for “left comodule.” Recall that, given a commutative Hopf algebroid \((A,\Gamma )\), a left \(\Gamma \)-comodule is a left A-module M equipped with a left A-linear map \(M \rightarrow \Gamma \otimes _AM\) which is counital and coassociative. If \(\Gamma \) is flat over A, then the category of left \(\Gamma \)-comodules is abelian and has enough relative injectives. Appendix 1 of [25] is the standard reference for these definitions and results.
Possibly more than one, since the ANSS at \(p=2\) has many nonzero differentials, and at odd primes the ANSS has nonzero differentials starting with the \(E_{2p-1}\)-term.
Since this paper may have readers who are number theorists and not topologists, we remark that at each prime p the divided alpha-family is the first and shortest-period of an infinite family of quasiperiodic families—the beta-family, the gamma-family, etc.—of p-power-torsion elements in the stable homotopy groups of spheres. These do not exhaust the stable homotopy groups of spheres, but they play an important role, partly because the nth Greek letter family is the \(2p^n(p-1)\)-quasiperiodic family which appears on the lowest possible line (i.e., the \(s=n\) line) in the Adams–Novikov spectral sequence, and partly because the nth Greek letter family (as well as other \(2p^n(p-1)\)-quasiperiodic families in the Adams–Novikov \(E_2\)-term) is computable from the cohomology of the automorphism group scheme of a height n formal group over \({\mathbb {F}}_p\), via some (very highly nontrivial) spectral sequence calculations. Chapters 5 and 6 of [25] are standard for this material.
It is standard that, whenever E is a ring spectrum with \(E_*E\) flat over \(E_*\), and whenever X is a spectrum, we have a coaction of \(E_*E\) on \(E_*X\) given by applying \(\pi _*\) to the map of spectra \(E\wedge X {\mathop {\longrightarrow }\limits ^{{{\,\mathrm{{id}}\,}}_E \wedge \eta \wedge {{\,\mathrm{{id}}\,}}_X}} E\wedge E\wedge X\), where \(\eta : S\rightarrow E\) is the unit map of the ring spectrum E.
By convention, given an element \(a\in A\), we also write a to denote the element \(\eta _L(a)\) in \(\Gamma \). That is, we treat the left unit map \(\eta _L\) as a canonical embedding of A into \(\Gamma \).
The “Moore complex” of a cosimplicial abelian group \(X^{\bullet }\) is the alternating sign cochain complex of \(X^{\bullet }\), i.e., the cochain complex whose group of n-cochains is \(X^n\) and whose differential \(X^n \rightarrow X^{n+1}\) is the alternating sum of the coface maps \(X^n \rightarrow X^{n+1}\) in \(X^{\bullet }\).
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Appendix A Appendix on cobar complexes
Appendix A Appendix on cobar complexes
In this paper, we occasionally must refer to cocycles in the cobar complex of a Hopf algebroid \((A,\Gamma )\) with coefficients in a left \(\Gamma \)-comodule M. The standard reference for Hopf algebroids is Appendix 1 of [25], and the (two-sided) cobar complex of \((A,\Gamma )\) is defined in Definition A1.2.11 of [25]. For convenience, we recall the one-sided version of that definition here, as well as a simplification that occurs when the coefficient comodule M is A itself.
Definition A.1
Let \((A,\Gamma )\) be a Hopf algebroid with left unit map \(\eta _L:A \rightarrow \Gamma \), right unit map \(\eta _R:A \rightarrow \Gamma \), and coproduct \(\Delta : \Gamma \rightarrow \Gamma \otimes _A \Gamma \). Let M be a left \(\Gamma \)-comodule with structure map \(\psi : M \rightarrow \Gamma \otimes _A M\). Then the (one-sided) cobar complex of \((A,\Gamma )\) with coefficients in M is the Moore complexFootnote 21
whose 0th coface map \(C^n \rightarrow C^{n+1}\) is \(\Delta \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A {{\,\mathrm{{id}}\,}}_M\), whose 1st coface map \(C^n \rightarrow C^{n+1}\) is \({{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A\Delta \otimes _A{{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A {{\,\mathrm{{id}}\,}}_M\), and so on, up through its \((n-1)\)st coface map \(C^n \rightarrow C^{n+1}\) given by \({{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A\Delta \otimes _A {{\,\mathrm{{id}}\,}}_M\), and with its last (that is, nth) coface map \(C^n \rightarrow C^{n+1}\) given by \({{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \psi \).
When \(M = A\), the above simplifies, and (46) is isomorphic to the cosimplicial abelian group
whose 0th coface map \(\tilde{C}^0 \rightarrow \tilde{C}^1\) is \(\eta _R\), and whose 1st coface map \(\tilde{C}^0 \rightarrow \tilde{C}^1\) is \(\eta _L\); and, when \(n>0\), whose 0th coface map \(\tilde{C}^n \rightarrow \tilde{C}^{n+1}\) sends \(x_1\otimes \dots \otimes x_n\) to \(1\otimes x_1\otimes \dots \otimes x_n\), whose nth coface map \(\tilde{C}^n \rightarrow \tilde{C}^{n+1}\) sends \(x_1\otimes \dots \otimes x_n\) to \(x_1\otimes \dots \otimes x_n\otimes 1\), and whose intermediate coface maps \(\tilde{C}^n \rightarrow \tilde{C}^{n+1}\) are given by letting the 1st coface map be \(\Delta \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\), letting the 2nd coface map be \({{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A\Delta \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\otimes _A \dots \otimes _A {{\,\mathrm{{id}}\,}}_{\Gamma }\), and so on.
The above conventions are standard, and agree with the more well-known standard conventions when working with Hopf algebras. When working with Hopf algebroids, an extra wrinkle is introduced by having two unit maps: the convention when working with Hopf algebroids is that, when we tensor \(\Gamma \) over A on the left, we use the A-module structure on \(\Gamma \) given by the left unit map \(\eta _L: A\rightarrow \Gamma \), and when we tensor \(\Gamma \) over A on the right, we use the A-module structure on \(\Gamma \) given by the right unit map \(\eta _R:A\rightarrow \Gamma \). So, for example, since \(\eta _L(v_1) = v_1\) and \(\eta _R(v_1) = v_1 + pt_1\) in the Hopf algebroid \((BP_*,BP_*BP)\) of stable co-operations in Brown–Peterson homology, we have that
With these conventions in place, it is an exercise to verify that (32) is a 1-cocycle in \(\tilde{C}^{\bullet }\).
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Candelori, L., Salch, A. Topological Hecke eigenforms. Math. Z. 307, 75 (2024). https://doi.org/10.1007/s00209-024-03552-2
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DOI: https://doi.org/10.1007/s00209-024-03552-2