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Celebratio Mathematica

Yakov M. Eliashberg

Tight and overtwisted contact structures

by John B. Etnyre

1.  Introduction

Figure 1.  Yasha at a conference in the late 1970s when several of the ideas leading to the tight versus overtwisted dichotomy were being developed.
The tight versus over­twisted di­cho­tomy has been an es­sen­tial or­gan­iz­ing prin­ciple and driv­ing force in three-di­men­sion­al con­tact geo­metry since its in­cep­tion around 1990. In this art­icle, we will dis­cuss the gen­es­is of this di­cho­tomy in Yasha’s sem­in­al work and his in­flu­en­tial con­tri­bu­tions to the the­ory. We will fo­cus on his clas­si­fic­a­tion of over­twisted con­tact struc­tures, his char­ac­ter­iz­a­tion of tight­ness (and hence the birth of the di­cho­tomy), and his work with Thur­ston, which al­lowed for the con­struc­tion of new tight con­tact man­i­folds that have many ap­plic­a­tions to low-di­men­sion­al to­po­logy. Along the way, we will dis­cuss fur­ther de­vel­op­ments by Yasha and oth­ers, as well as ap­plic­a­tions of this work out­side of con­tact geo­metry. We will end with his re­cent break­through with Bor­man and Murphy de­fin­ing over­twisted con­tact struc­tures in high­er di­men­sions. We will also dis­cuss the fur­ther de­vel­op­ment of the field in the work of Yasha and many oth­ers. This dis­cus­sion is not meant to be com­pre­hens­ive, but to give a good in­dic­a­tion of the depth, breadth, and pro­found im­pact of Yasha’s work. We will oc­ca­sion­ally sketch proofs to give a small in­dic­a­tion of what goes in­to the res­ult (many will be brief sketches based on an amaz­ing class of Yasha’s that the au­thor at­ten­ded in the fall of 2000 at Stan­ford), al­though we refer to the rel­ev­ant pa­pers for full de­tails of the proofs.

Throughout this art­icle we will as­sume the read­er is fa­mil­i­ar with ba­sic no­tions from con­tact geo­metry, such as the defin­i­tion of a con­tact struc­ture and char­ac­ter­ist­ic fo­li­ation, what Le­gendri­an and trans­verse knots are, and what their clas­sic­al in­vari­ants are. All this can be found in many places, such as [e29], [e39], [e46]. (Sev­er­al of the fig­ures in­cluded be­low are taken from Yasha’s ori­gin­al pa­pers.)

2.  Precursors and the birth of modern contact topology

Figure 2.  Overtwisted disk from [1].

In this sec­tion we will con­fine ourselves to di­men­sion 3. A fun­da­ment­al ques­tion one can ask is if any ori­ented 3-man­i­fold ad­mits a con­tact struc­ture (note, in di­men­sion 3 a man­i­fold must be ori­ented to ad­mit a con­tact struc­ture). This ba­sic ques­tion was answered in 1970 by Mar­tin­et [e4] when he showed that in­deed any ori­ented 3-man­i­fold ad­mits at least one con­tact struc­ture. The proof re­lies on the work of Lick­or­ish [e2] and Wal­lace [e1] who showed that any ori­ented 3-man­i­fold \( M \) was ob­tained from \( S^3 \) by sur­gery on some link. To con­struct a con­tact struc­ture on the man­i­fold one can real­ize the link as a trans­verse link in the stand­ard con­tact struc­ture \( \xi_{\mathrm{std}} \) on \( S^3 \). The con­tact struc­ture \( \xi_{\mathrm{std}} \) can be taken to be stand­ard in a neigh­bor­hood of each of the com­pon­ents and when per­form­ing sur­gery on the link, the neigh­bor­hood is re­moved and a new sol­id tor­us is glued in its place. One can eas­ily ex­tend the con­tact struc­ture over this glued-in tor­us to ob­tain a con­tact struc­ture on \( M \).

The next ba­sic ques­tion that arises is wheth­er a man­i­fold can sup­port more than one con­tact struc­ture. A few years after Mar­tin­et’s work, Lutz [e5] showed that there are con­tact struc­tures in dif­fer­ent ho­mo­topy classes of plane fields on a giv­en man­i­fold. He did this by in­tro­du­cing what is now called a Lutz twist. The key to Lutz’s proof is that a Lutz twist can change the ho­mo­topy class of the plane field. That is, if \( \xi_T \) is ob­tained from \( \xi \) by a Lutz twist, then \( \xi_T \) and \( \xi \) will not be ho­mo­top­ic as plane fields and thus can­not be iso­top­ic as con­tact struc­tures (and for most choices of \( T \) not even con­tacto­morph­ic). Since it is known that there are in­fin­itely many ho­mo­topy classes of plane fields on any giv­en ori­ented 3-man­i­fold (see be­low), we can use the Lutz twist to see that every ori­ented 3-man­i­fold ad­mits in­fin­itely many dis­tinct con­tact struc­tures.

We are ready to define an over­twisted con­tact struc­ture. A disk \( D \) in a con­tact man­i­fold \( (M,\xi) \) is an over­twisted disk if the char­ac­ter­ist­ic fo­li­ation on \( D \) has \( \partial D \) as a leaf and one sin­gu­lar point in­side of \( D \). See Fig­ure 2. A con­tact struc­ture \( \xi \) on \( M \) is called over­twisted if there is an over­twisted disk in­side of \( M \). The Lutz twist con­struc­tion above al­ways pro­duces such a disk. Thus all the in­fin­itely many dis­tinct con­tact struc­tures giv­en by Lutz’s con­struc­tion on a giv­en man­i­fold are over­twisted.

At this point, one might think all con­tact struc­tures are over­twisted and it might also be true that there is a unique con­tact struc­ture in each ho­mo­topy class of plane field. (We should point out at this point in the his­tor­ic­al de­vel­op­ment of the sub­ject, the defin­i­tion of over­twisted did not yet ex­ist; so our telling of the story is a bit ana­chron­ist­ic.) While this is not the case, it took the ground­break­ing work of Ben­nequin [e8] in 1983 to show it was not.

In [e8], Ben­nequin es­tab­lished the fam­ous Ben­nequin in­equal­ity that says if \( T \) is any knot trans­verse to the stand­ard con­tact struc­ture \( \xi_{\mathrm{std}} \) on \( \mathbb{R}^3 \) (or \( S^3 \)) then its self-link­ing num­ber sat­is­fies \[ \mathrm{sl}(T) \leq -\chi(\Sigma), \] where \( \Sigma \) is any sur­face with \( \partial \Sigma=T \). The self-link­ing num­ber is the re­l­at­ive Euler class of the con­tact struc­ture (re­l­at­ive to a nat­ur­al sec­tion of \( \xi \) along \( T \) com­ing from the char­ac­ter­ist­ic fo­li­ation on \( \Sigma \)). The only thing we need to know about the self-link­ing num­ber here is that if one per­turbs the bound­ary of an over­twisted disk ap­pro­pri­ately, then one will ob­tain a trans­verse un­knot with self-link­ing \( +1 \). Since this clearly vi­ol­ates the Ben­nequin in­equal­ity, the con­tact struc­ture ob­tained from a Lutz twist on \( S^3 \) in the same ho­mo­topy class of plane field as \( \xi_{\mathrm{std}} \) is not iso­top­ic or con­tacto­morph­ic to \( \xi_{\mathrm{std}} \). So, after Ben­nequin, we knew that not all con­tact struc­tures were over­twisted.

Ben­nequin’s proof of this in­equal­ity was in­geni­ous. He took a trans­verse knot and iso­toped it un­til it was the clos­ure of a braid. He then looked at the sin­gu­lar fo­li­ation on the sur­face \( \Sigma \) in­duced by the braid ax­is and the con­stant \( \theta \)-half planes. (Here we are think­ing of \( \mathbb{R}^3 \) with cyl­indric­al co­ordin­ate \( (r,\theta, z) \) where the \( z \)-ax­is is the braid ax­is, and a knot is a closed braid if the \( \theta \)-co­ordin­ate re­stric­ted to it has no crit­ic­al points.) Ben­nequin then iso­toped the fo­li­ation to sim­pli­fy it and even­tu­ally showed that, for ex­ample, if \( \Sigma \) was a disk then one could ar­range, by pos­sibly chan­ging \( T \), but only so that \( \mathrm{sl}(T) \) in­creased, that the fo­li­ation on \( \Sigma \) con­tained one sin­gu­lar point and ra­di­al lines on the disk. From here one can eas­ily con­clude that \( \mathrm{sl}(T)=-1 \) and of course \( \chi(\Sigma)=1 \).

This res­ult is really the birth of mod­ern con­tact to­po­logy and the first hint of many subtle con­nec­tions between con­tact geo­metry and the to­po­logy of 3-man­i­folds. More spe­cific­ally, it is at this point that we fi­nally know that con­tact struc­tures are not just de­term­ined by their ho­mo­topy data, so there is something deep­er about their struc­ture than “just al­geb­ra­ic to­po­logy”. In ad­di­tion, we see that the Ben­nequin in­equal­ity shows that one may use con­tact geo­metry to bound \( \;-\chi(\Sigma) \) for any Seifert sur­face for \( T \), and since \( \,-\chi(\Sigma)=2g(\Sigma)-1 \) (where \( g(\Sigma) \) is the genus of \( \Sigma) \) we see that con­tact geo­metry can give a lower bound on the genus of a Seifert sur­face for a knot. De­term­in­ing the min­im­al genus is a dif­fi­cult prob­lem that only re­cently has a fairly tract­able solu­tion.

Over­twisted con­tact struc­tures (ana­chron­ist­ic­ally) ap­peared in a few oth­er works, such as [e7] and [e10], but apart from Ben­nequin’s work, where the ex­ist­ence of an over­twisted disk was key, the over­twisted disk seemed more a byproduct of a con­struc­tion rather than a key fea­ture.

We now come to the sem­in­al work of Yasha, where he first defines what it means for a con­tact struc­ture to be over­twisted and then com­pletely clas­si­fies over­twisted con­tact struc­tures. This oc­curred in his 1989 pa­per [1]. We will dis­cuss this res­ult in de­tail be­low, but now con­tin­ue the jour­ney to the tight versus over­twisted di­cho­tomy.

To this end, Yasha no­ticed that a gen­er­al­iz­a­tion of the Ben­nequin in­equal­ity for close sur­faces, which he es­tab­lished in [5], was very re­min­is­cent of in­equal­it­ies for taut fo­li­ations. Yasha thought the word “taut” was over­used so de­cided to call such con­tact struc­tures tight. Spe­cific­ally, in 1992 Yasha [5] defined a tight con­tact struc­ture to be one that con­tained no disks whose char­ac­ter­ist­ic fo­li­ation con­tained a lim­it cycle. In that same pa­per, he proved that if a con­tact struc­ture was not tight it was over­twisted. Hence the birth of the tight versus over­twisted di­cho­tomy. In his pa­per [6], Yasha also shows a con­tact struc­ture is tight if and only if the Ben­nequin in­equal­ity is true and, in the pa­per [5], that \( S^3 \) has a unique tight con­tact struc­ture (thus Yasha com­pletely clas­si­fied all con­tact struc­tures on \( S^3 \)).

It is im­port­ant to ap­pre­ci­ate Yasha’s clas­si­fic­a­tion of con­tact struc­tures on \( S^3 \). After Ben­nequin’s work, it was thought that this was just the first ex­ample of a “zoo” of nonequi­val­ent con­tact struc­tures on \( S^3 \) in the giv­en ho­mo­topy class of plane field. Quot­ing from Yasha’s pa­per [5], “Twenty years ago Jean Mar­tin­et (see [e4]) showed that any ori­ent­able closed 3-man­i­fold ad­mits a con­tact struc­ture. Three years later after the work of R. Lutz (see [e5]) and in the wake of the tri­umph of Gro­mov’s \( h \)-prin­ciple, it seemed that the clas­si­fic­a­tion of closed con­tact 3-man­i­folds was at hand. Ten years later in the sem­in­al work [e8], D. Ben­nequin showed that the situ­ation is much more com­plic­ated and that the clas­si­fic­a­tion of con­tact struc­tures on 3-man­i­folds, and even on \( S^3 \), was not likely to be achieved.” Yasha’s work in [1], [5] showed that (1) any ho­mo­topy class of plane field has a unique over­twisted con­tact struc­ture, and (2) there is ex­actly one ho­mo­topy class that has an­oth­er con­tact struc­ture. So the “zoo of con­tact struc­tures” on \( S^3 \) turns out to be quite well-be­haved!

We briefly sketch Yasha’s proof that \( S^3 \) has a unique tight con­tact struc­ture (up to iso­topy). Since Dar­boux’s the­or­em says that con­tact struc­tures are all the same in a neigh­bor­hood of a point, this res­ult fol­lows by show­ing that two tight con­tact struc­tures on the 3-ball \( B^3 \) that in­duce the same char­ac­ter­ist­ic fo­li­ation on the bound­ary are ac­tu­ally iso­top­ic. That is, we need to see that giv­en any tight con­tact struc­ture \( \xi \) on \( B^3 \), there is a fixed tight con­tact struc­ture \( \xi_{m} \) that is iso­top­ic to \( \xi \). To do this, Yasha gives an in­geni­ous con­struc­tion of “mod­el con­tact struc­tures on the ball” giv­en a char­ac­ter­ist­ic fo­li­ation on its bound­ary that could come from a tight con­tact struc­ture. That is, giv­en a sin­gu­lar fo­li­ation \( \mathcal{F} \) on \( \partial B^3 \) he con­structs a mod­el con­tact struc­ture \( \eta_F \) on \( B^3 \) that in­duces \( \mathcal{F} \) on bound­ary. Now giv­en \( \xi \) on the unit ball \( B^3 \) we can let \( \mathcal{F}_t \) be the char­ac­ter­ist­ic fo­li­ation on the bound­ary of the ball \( B_t \) of ra­di­us \( t \) in \( B^3 \), and let \( \eta_t \) be the mod­el con­tact struc­ture on the ball whose bound­ary has char­ac­ter­ist­ic fo­li­ation \( \mathcal{F}_t \). Now we can define con­tact struc­ture \( \xi_t \) to be \( \eta_t \) on \( B_t \) and \( \xi \) on \( B^3-B_t \). No­tice that this is a one-para­met­er fam­ily of con­tact struc­tures on \( B^3 \) that starts with \( \xi \) and ends with \( \eta_1 \). That is, \( \xi \) is iso­top­ic to the mod­el con­tact struc­ture \( \eta_1 \). (Note that there is an is­sue with \( \eta_t \) when \( t \) ap­proaches 0, but we can use Dar­boux’s the­or­em again to make sure \( \xi \) is stand­ard on \( B_\epsilon \) and then run the ar­gu­ment from there). Clearly the key to this proof is the con­struc­tion of the mod­el con­tact struc­tures, but for that we refer the read­er to Yasha’s pa­per [5].

A nat­ur­al ques­tion now is: Are there any more tight con­tact struc­tures? In [3] Yasha proved that any sym­plect­ic­ally fil­lable con­tact struc­ture is tight by show­ing that trans­verse knots in this con­tact struc­ture sat­is­fy the Ben­nequin in­equal­ity (which by an earli­er res­ult of Yasha im­plies that it must be tight). The proof in­volves the ana­lys­is of pseudo­holo­morph­ic disks in the sym­plect­ic filling. See Geiges’ art­icle “Filling by holo­morph­ic disks” in this volume of Cel­eb­ra­tio This res­ult gives a large fam­ily of tight con­tact man­i­folds and there are lots of con­struc­tions of sym­plect­ic­ally fil­lable con­tact struc­tures, see for ex­ample [2], [e19]. Later we will dis­cuss a tech­nique de­veloped by Yasha and Bill Thur­ston to build tight con­tact struc­tures by “per­turb­ing taut fo­li­ations”. Though these con­tact struc­tures are still sym­plect­ic­ally fil­lable, pre­vi­ous con­struc­tions of sym­plect­ic fillings could not ap­proach what can be done with this con­struc­tion.

3.  The classification of overtwisted contact 3-manifolds

We be­gin by stat­ing the simplest ver­sion of Yasha’s clas­si­fic­a­tion of over­twisted con­tact struc­tures on 3-man­i­folds. To this end, we let \( \operatorname{Dist}(M) \) be the space plane fields on \( M \) and \( \operatorname{Cont}_{ot}(M) \) be the space of over­twisted con­tact struc­tures on \( M \). Clearly there is an in­clu­sion of \( \operatorname{Cont}_{ot}(M) \) in­to \( \operatorname{Dist}(M) \). Yasha’s main res­ult in [1] is that this in­clu­sion in­duces a bijec­tion \[ i_*:\, \pi_0(\operatorname{Cont}_{ot}(M))\to \pi_0 (\operatorname{Dist}(M)). \] That is every ho­mo­topy class of plane field con­tains a unique iso­topy class of over­twisted con­tact struc­ture (re­call that con­tact struc­tures that are ho­mo­top­ic through con­tact struc­tures are iso­top­ic).

Un­der­stand­ing ho­mo­topy classes of plane fields is fairly straight­for­ward and so Yasha’s work gives an ef­fect­ive and com­plete clas­si­fic­a­tion of over­twisted con­tact struc­tures. We now elab­or­ate on ho­mo­topy classes of plane fields. One can show, see [e19], that there is a map (that re­quires choices) \[ f:\, \pi_0 (\operatorname{Dist}(M))\to H_1(M), \] and that \( f^{-1}(h)=\mathbb{Z}/(2d(h)) \) where \( d(h) \) is the di­vis­ib­il­ity of \( h \) in \( H_1(M) \). Moreover, \( f(\xi) \) is de­term­ined by the spin\( ^c \) struc­ture in­duced by \( \xi \) and there are ex­pli­cit for­mu­las for dis­tin­guish­ing ele­ments of \( f^{-1}(h)=\mathbb{Z}/(2d(h)) \); see [e19]. So we see, among oth­er things, that every spin\( ^c \) struc­ture ad­mits sev­er­al over­twisted con­tact struc­tures but also that any ori­ented 3-man­i­fold ad­mits in­fin­itely many such struc­tures (be­cause \( d(0)=0 \)). Just for some con­text, we note that for a lens space \( L(p,q) \) the ho­mo­topy classes of plane fields are in one-to-one cor­res­pond­ence with \[ H_1(L(p,q)\oplus \mathbb{Z}\cong \mathbb{Z}/p\mathbb{Z}\oplus \mathbb{Z}, \] and on \( S^1\times S^2 \) the ho­mo­topy classes of plane fields are in one-to-one cor­res­pond­ence with \[ \oplus_{n\in \mathbb{Z}} (\mathbb{Z}/(2n)\mathbb{Z})\cong \mathbb{Z}\oplus (\mathbb{Z}/2\mathbb{Z}\oplus \mathbb{Z}/2\mathbb{Z})\oplus (\mathbb{Z}/4\mathbb{Z}\oplus \mathbb{Z}/4\mathbb{Z})\oplus \cdots. \]

We note that this is a clas­sic­al ex­ample of an \( h \)-prin­ciple. Re­call that, roughly speak­ing, a weak form of an \( h \)-prin­ciple is that if there is no to­po­lo­gic­al ob­struc­tion for something be­ing true then it is true, and if two things look the same on the to­po­lo­gic­al level then they are the same. Yasha is re­spons­ible for many oth­er such \( h \)-prin­ciples, but this is cer­tainly a very in­flu­en­tial one, and he has an even stronger ver­sion.

Figure 3.  An almost horizontal characteristic foliation from [1].

To state the stronger ver­sion we de­note by \( \operatorname{Dist}_p(M) \) the space of plane fields on \( M \) that agree with a fixed plane at \( p \) and \( \operatorname{Cont}^D_{ot}(M) \) the space of con­tact struc­tures on \( M \) that have a fixed disk \( D\subset M \) as a stand­ard over­twisted disk that is tan­gent to \( \xi \) at \( p \) (by stand­ard over­twisted disk we just mean to fix one char­ac­ter­ist­ic fo­li­ation on \( D \) as de­scribed in the defin­i­tion of over­twisted disk). Yasha’s main the­or­em in [1] is that the in­clu­sion \[ \operatorname{Cont}^D_{ot}(M) \to \operatorname{Dist}_p(M) \] is a weak ho­mo­topy equi­val­ence. It is a simple ex­er­cise to check that this res­ult im­plies the res­ult above about \( \pi_0 \) fol­lows (note this is not auto­mat­ic since all the spaces in­volved are dif­fer­ent).

We briefly dis­cuss Yasha’s proof that there is a bijec­tion between the ho­mo­topy classes of plane fields on a 3-man­i­fold \( M \) and over­twisted con­tact struc­tures on the man­i­fold. The sur­jectiv­ity of \( i_* \) above fol­lows from the work of Lutz men­tioned above, so we con­sider two over­twisted con­tact struc­tures \( \xi_0 \) and \( \xi_1 \) on a man­i­fold \( M \) that are ho­mo­top­ic as plane fields. It is easy to iso­tope one of them so that they both share an over­twisted disk, say \( D \), and hence they agree near \( D \). Let \( \xi_t, t\in [0,1] \) be the ho­mo­topy between the two con­tact struc­tures. One now picks a tri­an­gu­la­tion of \( M \), then one may ho­mo­top all the \( \xi_t \), fix­ing \( \xi_0 \) and \( \xi_1 \), so that they agree in a neigh­bor­hood of \( D \) and near the ver­tices of the tri­an­gu­la­tion. One may then fur­ther ho­mo­top the \( \xi_t \), fix­ing \( \xi_0 \) and \( \xi_1 \), so that they are all con­tact struc­tures on the 2-skel­et­on of the tri­an­gu­la­tion. Now the \( \xi_t \) are con­tact struc­tures ex­cept pos­sibly on a fi­nite uni­on of balls \( B_i \). If the tri­an­gu­la­tion is chosen suf­fi­ciently small (with re­spect to some aux­il­i­ary met­ric) then one can ar­range that the char­ac­ter­ist­ic fo­li­ation on the bound­ar­ies of the \( B_i \) are al­most ho­ri­zont­al; see Fig­ure 3. One can now find trans­verse curves con­nect­ing the sin­gu­lar­it­ies of one of the \( B_i \) to an­oth­er (and also to the neigh­bor­hood of \( D \)). A neigh­bor­hood of the balls and the curves is a single ball and the \( \xi_t \) have been ho­mo­toped to be con­tact out­side this one ball. Now one can use the fact that we have an over­twisted disk to build a mod­el con­tact struc­ture to fill in these balls. This provides the iso­topy of con­tact struc­tures from \( \xi_0 \) to \( \xi_1 \).

4.  Legacy and applications of overtwisted contact structures

It was com­mon after Yasha’s clas­si­fic­a­tion of over­twisted con­tact struc­tures for people (in­clud­ing my­self) to say that over­twisted con­tact struc­tures were not in­ter­est­ing since they were de­term­ined by their ho­mo­topy class of plane field where­as tight con­tact struc­tures were seen to be tightly con­nec­ted to the to­po­logy of 3- and 4-man­i­folds. But just be­cause something is clas­si­fied, and fairly easy to un­der­stand, does not make it un­in­ter­est­ing! For ex­ample, sur­faces have been clas­si­fied for a long time now, but the study of sur­faces is still a ro­bust field of math­em­at­ics. One just needs to ask more re­fined ques­tions, such as what do we know about dif­feo­morph­isms of sur­faces or how can we ap­ply them to un­der­stand 3-man­i­folds, among many oth­er ques­tions. The last few dec­ades have shown that over­twisted con­tact struc­tures are sim­il­arly in­ter­est­ing. There are many in­ter­est­ing and subtle fea­tures of over­twisted con­tact struc­tures as well as sev­er­al ex­cit­ing ap­plic­a­tions. We will dis­cuss these now.
4.1.  Results about overtwisted contact structures
Figure 4.  On the left, each dot represents a nonloose Legendrian unknot and the arrows indicate what happens after stabilization. On the right we see the same for Legendrian unknots in the standard tight contact structure on \( S^3 \).
We be­gin with Le­gendri­an knots in an over­twisted con­tact struc­ture. A Le­gendri­an knot \( L \) in an over­twisted con­tact struc­ture is called loose if the con­tact struc­ture re­stric­ted to its com­ple­ment is also over­twisted; oth­er­wise, the knot is called non­loose (the term ex­cep­tion­al is also used). It is a folk­lore res­ult, see [e53], that any two loose knots with the same clas­sic­al in­vari­ants (that is, they are in the same knot type, have the same Thur­ston–Ben­nequin in­vari­ant, and have the same ro­ta­tion num­ber) are coarsely equi­val­ent, which means that there is a con­tacto­morph­ism of the am­bi­ent man­i­fold that is smoothly iso­top­ic to the iden­tity and takes one of the knots to the oth­er. We will see, be­low, that un­der­stand­ing loose knots up to iso­topy through Le­gendri­an knots is much more subtle. But first, we turn to non­loose knots. In [10] Yasha and Fraser clas­si­fied non­loose Le­gendri­an un­knots in \( S^3 \). We re­call that over­twisted con­tact struc­tures on \( S^3 \) can be in­dexed by the in­tegers. So we let \( \xi_n \) be the over­twisted con­tact struc­ture on \( S^3 \) with Hopf in­vari­ant \( n \). Yasha and Fraser’s clas­si­fic­a­tion says that non­loose un­knots ex­ist only in \( \xi_{-1} \) and in \( \xi_{-1} \) the com­plete list, up to coarse equi­val­ence, is \( L_1 \) and \( L^\pm_n \) for \( n\geq 2 \), where \[ \operatorname{tb}(L_1)=1, \operatorname{tb}(L_n^\pm)=n, \operatorname{rot}(L_1)=0, \text{ and } \operatorname{rot}(L_n^\pm)=\pm n-1, \] and the \( \mp \)-sta­bil­iz­a­tion of \( L_n^\pm \) is \( L_{n-1}^\pm \) for \( n > 2 \) and the \( \mp \)-sta­bil­iz­a­tion of \( L_2^\pm \) is \( L_1 \). It is easi­est to visu­al­ize this clas­si­fic­a­tion by plot­ting the ro­ta­tion num­ber and Thur­ston–Ben­nequin in­vari­ants of these non­loose knots; such a plot is called the moun­tain range of the non­loose Le­gendri­an un­knots. See Fig­ure 4. It is in­ter­est­ing to con­trast this with the clas­si­fic­a­tion of Le­gendri­an un­knots in the tight con­tact struc­ture on \( S^3 \). This was giv­en in [10] too and the moun­tain range for these knots is shown in Fig­ure 4. We note that in a tight con­tact man­i­fold, there is a Le­gendri­an ver­sion of the Ben­nequin in­equal­ity which says that for a Le­gendri­an knot \( L \) that bounds a sur­face \( \Sigma \) we have \[ \operatorname{tb}(L)+\operatorname{rot}(L)\leq -\chi(\Sigma). \] This in­equal­ity shows that in a tight con­tact man­i­fold, the moun­tain range for any knot is bounded above, but we see in the clas­si­fic­a­tion of non­loose un­knots that they can have Thur­ston–Ben­nequin in­vari­ant ar­bit­rar­ily large! This seems quite sur­pris­ing, but it also seems to be a gen­er­al phe­nomen­on. For ex­ample, in work of Min, Mukher­jee and the present au­thor [e61], we clas­si­fy all non­loose Le­gendri­an tor­us knots in over­twisted con­tact struc­tures on \( S^3 \) up to coarse equi­val­ence, and the moun­tain range for any tor­us knot is not bounded above! We also show that for any fixed tor­us knot there are only a fi­nite num­ber of over­twisted con­tact struc­tures that ad­mit non­loose rep­res­ent­at­ives of that knot. So, when study­ing non­loose knots we see that there are many subtle fea­tures and there are many open ques­tions about them. For ex­ample, giv­en a knot \( K \) in \( S^3 \), is it al­ways true that \( K \) ad­mits non­loose rep­res­ent­at­ives in only fi­nitely many over­twisted con­tact struc­tures on \( S^3 \)? And how does one de­term­ine which con­tact struc­tures those are? Are the moun­tain ranges for non­loose knots al­ways un­boun­ded from above? Why?

Now turn­ing to the clas­si­fic­a­tion of non­loose un­knots up to Le­gendri­an iso­topy we see the beau­ti­ful work of Vo­gel [e56]. He showed that giv­en a pair of in­tegers \( (r,t) \) with \( r+t \) odd, there is a unique, up to Le­gendri­an iso­topy, loose Le­gendri­an knot \( L \) in \( (S^3,\xi_{-1}) \) with \( \operatorname{tb}(L)=t \) and \( \operatorname{rot}(L)=r \) if \( t < 0 \), but if \( t > 0 \) then there are two dis­tinct loose Le­gendri­an un­knots in \( (S^3,\xi_{-1}) \) with these in­vari­ants (though of course from above, they will be coarsely equi­val­ent). This is quite sur­pris­ing! Moreover, he showed that in \( (S^3,\xi_n) \) with \( n\not=-1 \), loose Le­gendri­an un­knots are clas­si­fied, up to Le­gendri­an iso­topy, by their ro­ta­tion num­ber and Thur­ston–Ben­nequin in­vari­ant. Turn­ing to non­loose Le­gendri­an un­knots, Vo­gel showed that for each of the Le­gendri­an knots in Yasha and Fraser’s clas­si­fic­a­tion, there are two Le­gendri­an rep­res­ent­at­ives up to iso­topy. Again, this is very sur­pris­ing and points to a subtle dif­fer­ence between the clas­si­fic­a­tion of Le­gendri­an knots in over­twisted con­tact struc­ture up to Le­gendri­an iso­topy and coarse equi­val­ence.

We now turn to the con­tacto­morph­isms of over­twisted con­tact struc­tures. We will de­note by \( \operatorname{Diff}_+(M,\xi) \) the space of con­tacto­morph­isms of \( \xi \) that pre­serve the ori­ent­a­tion on \( \xi \). In [e56] Vo­gel showed that \[ \pi_0(\operatorname{Diff}_+(S^3,\xi_n))=\begin{cases} \mathbb{Z}/2\mathbb{Z}\oplus \mathbb{Z}/2\mathbb{Z} & \text{ if } n={}-1,\\ \mathbb{Z}/2\mathbb{Z}& \text{ otherwise.} \end{cases} \] This res­ult was ori­gin­ally an­nounced by Chekan­ov [10], but was first proven in [e56]. We note that the \( \mathbb{Z}/2\mathbb{Z} \) factor in all of the dif­feo­morph­ism groups is de­tec­ted by in­vari­ant due to Dy­mara [e24] while the oth­er \( \mathbb{Z}/2\mathbb{Z} \) factor for \( \xi_{-1} \) is de­tec­ted by the ac­tion of a con­tacto­morph­ism on the non­loose un­knots. We con­trast the res­ult above with Yasha’s proof [5] that \[ \pi_0(\operatorname{Diff}_+(S^3,\xi_{\mathrm{tight}}))=\{1\}, \] which shows that con­tacto­morph­isms of over­twisted con­tact struc­tures on \( S^3 \) are “more in­ter­est­ing” than the con­tacto­morph­isms of the tight con­tact struc­ture!

4.2.  Applications of overtwisted contact structures
Figure 5.  Surgery diagrams for two overtwisted contact structures on \( S^3 \).
We will fo­cus on three ap­plic­a­tions of over­twisted con­tact struc­tures: the sur­gery de­scrip­tion of all con­tact 3-man­i­folds, the ex­ist­ence of near sym­plect­ic forms on 4-man­i­folds with pos­it­ive \( b_2^+ \), and the ex­ist­ence of En­gel struc­tures on par­al­lel­iz­able 4-man­i­folds.

One of the first ap­plic­a­tions of over­twisted con­tact struc­tures is to con­tact geo­metry in gen­er­al. In [e36] Ding and Geiges showed that any con­tact 3-man­i­fold \( (M,\xi) \) could be ob­tained from \( S^3 \) with its stand­ard tight con­tact struc­ture by con­tact sur­gery on a Le­gendri­an link. For ex­ample, Fig­ure 5 shows sur­gery dia­grams for two dif­fer­ent over­twisted con­tact struc­tures on \( S^3 \). It is a beau­ti­ful res­ult that does not men­tion over­twisted con­tact struc­tures but es­sen­tially uses them in its proof. Moreover, it should be noted that this res­ult is now ubi­quit­ous in con­tact geo­metry; it gives us one of the key ways to present gen­er­al con­tact man­i­folds! The proof of this res­ult goes as fol­lows. It is easy to show that there are Le­gendri­an knots in any con­tact man­i­fold such that \( +1 \) con­tact sur­gery on the knot yields an over­twisted man­i­fold. So, giv­en \( (M,\xi) \) we can find a Le­gendri­an knot \( L \) on which we can do \( +1 \) con­tact sur­gery to get a man­i­fold \( (M^{\prime},\xi^{\prime}) \) with an over­twisted con­tact struc­ture. We note that in \( (M^{\prime},\xi^{\prime}) \) there is “dual” Le­gendri­an \( L^{\prime} \) on which we can per­form \( -1 \) con­tact sur­gery to ob­tain \( (M,\xi) \) back again. Now there is also a Le­gendri­an \( K \) in \( (S^3,\xi_{\mathrm{tight}}) \) on which we can per­form \( +1 \) con­tact sur­gery to ob­tain \( (M^{\prime\prime},\xi^{\prime\prime}) \) where \( \xi^{\prime\prime} \) is over­twisted. It is now fairly easy to see that one can get from any over­twisted con­tact man­i­fold to any oth­er over­twisted con­tact man­i­fold by a se­quence of \( -1 \) con­tact sur­ger­ies; see for ex­ample [e26]. This com­pletes the proof.

There are also sev­er­al ap­plic­a­tions to the geo­metry of 4-man­i­folds. We first men­tion a res­ult of Gay and Kirby [e32] that says a 4-man­i­fold hav­ing \( b_2^+ > 0 \) ad­mits a near sym­plect­ic struc­ture. A near sym­plect­ic struc­ture on a 4-man­i­fold is a closed 4-form that is a sym­plect­ic form away from some em­bed­ded circles, and along those circles it has a spe­cial form. The key to Gay and Kirby’s con­struc­tion is to real­ize that near the sin­gu­lar circles, one could build a mod­el for the near sym­plect­ic struc­ture whose bound­ary is over­twisted. They then use some clev­er handle ma­nip­u­la­tions to ex­tend this struc­ture over the rest of the man­i­fold, and to do this, it is es­sen­tial to know that over­twisted con­tact struc­tures are de­term­ined by their ho­mo­topy class of plane field. The read­er can refer to Gay’s art­icle, “From near-sym­plect­ic con­struc­tions to tri­sec­tions of 4-man­i­folds”, in the Cel­eb­ra­tio Math­em­at­ica volume on Rob Kirby, for a dis­cus­sion of how this near sym­plect­ic con­struc­tion led to their dis­cov­ery of tri­sec­tion of 4-man­i­folds, which is cur­rently a very act­ive area of re­search.

An­oth­er ap­plic­a­tion of over­twisted con­tact struc­tures is the ex­ist­ence of En­gel struc­tures on par­al­lel­iz­able 4-man­i­folds. An En­gel struc­ture on a 4-man­i­fold \( X \) is a 2-plane field \( \mathcal{D} \) on \( X \) such that \( [\mathcal{D},\mathcal{D}] \) has rank 3 every­where and \( [\mathcal{D},[\mathcal{D},\mathcal{D}]]=TX \). Here \( [\mathcal{D},\mathcal{D}] \) is the sub­bundle of \( TM \) formed by tak­ing all the com­mut­at­ors of loc­al sec­tions of \( \mathcal{D} \). En­gel struc­tures are in­ter­est­ing for many reas­ons, but one par­tic­u­larly in­ter­est­ing fea­ture is that they are stable in the sense that a \( C^2 \) small per­turb­a­tion of an En­gel struc­ture is an En­gel struc­ture. What makes this re­mark­able is that Mont­gomery [e14] clas­si­fied all stable dis­tri­bu­tions, and they come in three broad fam­il­ies (nonsin­gu­lar line fields, con­tact struc­tures, and “even” con­tact struc­tures) and En­gel struc­tures on 4-man­i­folds! It is not hard to check that if a 4-man­i­fold ad­mits an En­gel struc­ture then it must be par­al­lel­iz­able. There has been some work try­ing to prove that all par­al­lel­iz­able 4-man­i­folds ad­mit En­gel struc­tures. In 2009, Vo­gel [e49] fi­nally es­tab­lished this. His key idea was to take a “round handle” de­com­pos­i­tion of the 4-man­i­fold, build mod­el En­gel struc­tures on the handles and try to glue the En­gel struc­tures to­geth­er. To achieve the glu­ing, it is es­sen­tial that the bound­ar­ies of the round handles have over­twisted con­tact struc­tures in­duced on them. It is the flex­ib­il­ity that the over­twisted­ness al­lows for that makes the con­struc­tion work.

5.  Legacy and applications of tight contact structures

From the very be­gin­ning, tight con­tact struc­tures seemed more in­ter­est­ing than over­twisted ones since their ex­ist­ence is more subtle, and we know that the Ben­nequin in­equal­ity is true for tight con­tact struc­tures and thus there is a strong con­nec­tion between such con­tact geo­metry and the to­po­logy of the man­i­fold sup­port­ing the struc­ture. In this sec­tion, we will dis­cuss how our know­ledge of tight struc­tures has pro­gressed since its in­cep­tion, in­clud­ing an im­port­ant res­ult of Yasha and Bill Thur­ston, the cur­rent state of our un­der­stand­ing of tight con­tact struc­tures, and ap­plic­a­tions of tight con­tact struc­tures.
5.1.  The Eliashberg–Thurston theorem
We men­tioned above that Yasha showed sym­plect­ic­ally fil­lable con­tact struc­tures had to be tight. This al­lows us to con­struct many tight con­tact man­i­folds, but in 1996, Yasha and Thur­ston in­tro­duced a power­ful new con­struc­tion of tight con­tact man­i­folds that has been a key part of many ma­jor ad­vances in 3-man­i­fold to­po­logy.

A fo­li­ation on a 3-man­i­fold \( M \) is a “nice” de­com­pos­i­tion of \( M \) in­to a uni­on of sur­faces. If you look at the tan­gent planes to these sur­faces you get a dis­tri­bu­tion \( \mathcal{F} \) that de­term­ines the fo­li­ation. Yasha and Thur­ston’s re­mark­able the­or­em [7], [8] said that any ori­ented \( C^2 \) fo­li­ation of an ori­ented 3-man­i­fold \( M \), oth­er than the fo­li­ation of \( S^1\times S^2 \) by \( \{pt\}\times S^2 \), can be \( C^0 \) ap­prox­im­ated by a pos­it­ive \( \xi_+ \) and neg­at­ive \( \xi_- \) con­tact struc­ture.

While this is a very pleas­ing res­ult in its own right, fur­ther work of Yasha and Thur­ston made it a key tool in low-di­men­sion­al to­po­logy. Spe­cific­ally, if the fo­li­ation \( \mathcal{F} \) on \( M \) were taut, then they could build a sym­plect­ic struc­ture on \( M\times [-1,1] \) that gave a filling of \( (M\times\{1\}, \xi_+)\cup (-M\times\{-1\},\xi_-) \). By taut, we mean that on \( M \) there is a volume-pre­serving vec­tor field trans­verse to \( \mathcal{F} \). Of course this means that \( (M,\xi_+) \) and \( (-M,\xi_-) \) are sym­plect­ic­ally fil­lable and hence tight.

This last res­ult is par­tic­u­larly power­ful giv­en work of Gabai [e9]. Gabai showed that any closed, ori­ented, ir­re­du­cible 3-man­i­fold \( M \) with \( H_2(M) \) non­trivi­al ad­mits a taut fo­li­ation. Com­bined with Yasha and Thur­ston’s work, we know that such a man­i­fold al­ways ad­mits a tight con­tact struc­ture! We now know that, in some sense, most ori­ented, ir­re­du­cible 3-man­i­folds ad­mit tight con­tact struc­tures; in fact, the only way an ir­re­du­cible 3-man­i­fold might not ad­mit a tight con­tact struc­ture is if it is a ra­tion­al ho­mo­logy sphere.

To prove their res­ult, Yasha and Thur­ston in­tro­duced the no­tion of a con­foli­ation. This is a plane field \( \xi \) defined by a 1-form \( \alpha \) such that \( \alpha\wedge d\alpha\geq 0 \). So there are re­gions where \( \xi \) defines a fo­li­ation, and re­gions where it defines a con­tact struc­ture. The proof that a fo­li­ation (oth­er than the stand­ard fo­li­ation of \( S^1\times S^2 \)) can be per­turbed to a con­tact struc­ture has two steps. In Step 1, one shows that giv­en a fo­li­ation \( \xi \) on \( M \) one may \( C^0 \)-per­turb it to a con­foli­ation \( \xi^{\prime} \) such that every point in \( M \) can be con­nec­ted by a path tan­gent to \( \xi^{\prime} \) to a re­gion where \( \xi^{\prime} \) is a con­tact struc­ture. In Step 2, one shows that giv­en a con­foli­ation as in Step 1, one can \( C^{\infty} \) de­form it in­to a con­tact struc­ture \( \xi \).

Figure 6.  The induced foliation on an annulus transverse to a foliation along a curve with linear holonomy and the result of shifting it up. On the bottom, one sees the foliations superimposed, and that one is clockwise of the other at any given point in the annulus.

The key idea for Step 1 is that if one has a leaf \( L \) of the fo­li­ation \( \xi \) that con­tains a closed curve \( \gamma \) with non­trivi­al lin­ear holonomy, then one may “shear” \( \xi \) in a neigh­bor­hood of \( \gamma \) to get a new plane field that is con­tact in a neigh­bor­hood of \( \gamma \) (and un­changed out­side of a slightly lar­ger neigh­bor­hood). To de­scribe this more fully, we re­call the defin­i­tion of holonomy. If \( A \) is an an­nu­lus con­tain­ing \( \gamma \) that is trans­verse to \( \xi \), then there is a nonsin­gu­lar one-di­men­sion­al fo­li­ation of \( A \) in­duced from \( \xi \), and \( \gamma \) is a leaf in this fo­li­ation. Tak­ing a trans­verse curve \( \eta \) to the fo­li­ation on \( A \), we can define a first re­turn map of the line field on \( A \) by start­ing with a point on \( \eta \) and push­ing it around the leaf of the fo­li­ation on \( A \) un­til we re­turn to \( \eta \). We can as­sume that \( \eta=[-1,1] \) and 0 is the in­ter­sec­tion of \( \gamma \) with \( \eta \). Thus 0 is a fixed point of the first re­turn map. We call the first re­turn map the holonomy of \( \gamma \). As­sum­ing the holonomy has de­riv­at­ive at 0 that is not 1, then we say it has non­trivi­al lin­ear holonomy. Con­sider a neigh­bor­hood \( [-\epsilon,\epsilon]\times A \) of \( A \). If we shift the fo­li­ation up slightly along \( A\times \{\epsilon\} \), then we can re­place \( \xi \) on the in­teri­or of \( [-\epsilon,\epsilon]\times A \) with a con­tact struc­ture. In Fig­ure 6, we see the \( A\times\{-\epsilon\} \) and \( A\times\{\epsilon\} \) (after sheer­ing) on the top, and on the bot­tom they are su­per­im­posed. From this, one can see a plane field that is tan­gent to the \( [-\epsilon,\epsilon] \) dir­ec­tion and ro­tates from the fo­li­ation on one an­nu­lus to the oth­er will be a con­tact struc­ture. Yasha and Thur­ston also show that giv­en oth­er non­trivi­al holo­nom­ies for \( \gamma \), one may still \( C^0 \) per­turb \( \xi \) in a sim­il­ar man­ner (though it is more com­plic­ated).

To com­plete Step 1, Yasha and Thur­ston show that one can find suf­fi­ciently many curves with non­trivi­al holonomy. To this end, we re­call that a sub­set of \( M \) is called min­im­al if it is a nonempty closed set that is a uni­on of leaves and does not con­tain a smal­ler such set. It is easy to see that every leaf in a fo­li­ation lim­its to a min­im­al set. So if we can find the ap­pro­pri­ate curves \( \gamma \) with good holonomy in the min­im­al sets, then we can eas­ily prove that per­turb­ing as above will pro­duce the de­sired \( \xi^{\prime} \). Luck­ily, we know that a min­im­al set in \( M \) must be either (i) all of \( M \), (ii) a closed leaf, or (iii) an “ex­cep­tion­al” min­im­al set. One can then ana­lyze these cases to find the de­sired \( \gamma \) (pos­sibly after al­ter­ing the fo­li­ation!).

There are two ap­proaches to Step 2. For the first ap­proach, Yasha and Thur­ston show how to take curves \( \nu \) tan­gent to \( \xi^{\prime} \) that starts in a con­tact re­gion of \( M \) and ends at a fo­li­ated re­gion of \( M \), and then per­turb \( \xi^{\prime} \) in a \( C^\infty \) way to make it con­tact in a neigh­bor­hood of \( \nu \). One may it­er­ate this pro­cess to turn \( \xi^{\prime} \) in­to a con­tact struc­ture. In the second ap­proach, one may ap­ply a res­ult of Altschuler [e16] to de­form \( \xi^{\prime} \) in­to a con­tact struc­ture. Altschuler defines a kind of “heat” flow on the space of dif­fer­en­tial 1-forms that can be used to “dis­trib­ute” the twist­ing of the plane field across the man­i­fold.

5.2.  The current state of tight contact structures
The most ba­sic ques­tion about tight con­tact struc­tures is when they ex­ist. As men­tioned in the last sub­sec­tion, the work of Yasha, Thur­ston, and Gabai shows that the only way an ir­re­du­cible 3-man­i­fold might not ad­mit a tight con­tact struc­ture is if it is an in­teg­ral ho­mo­logy sphere. It turns out that there are man­i­folds that do not ad­mit a tight con­tact struc­ture. The first such man­i­fold was found in 2001 in the work of Honda and the present au­thor [e25] where we show that the Poin­caré ho­mo­logy sphere with its “non­stand­ard” ori­ent­a­tion does not ad­mit a tight con­tact struc­ture, but with its stand­ard ori­ent­a­tion, it does ad­mit a tight con­tact struc­ture. It is cur­rently un­known if every ir­re­du­cible in­teger ho­mo­logy sphere ad­mits a tight con­tact struc­ture with at least one ori­ent­a­tion.

Gen­er­al­iz­ing the Poin­caré ho­mo­logy sphere ex­ample, Lis­ca and Stip­sicz [e43] showed that \( 2n-1 \) sur­gery on the \( (2,2n+1) \)-tor­us knot does not ad­mit any tight con­tact struc­tures (no­tice that the Poin­caré ho­mo­logy sphere with its non­stand­ard ori­ent­a­tion is the \( n=1 \) case). They later showed that a Seifert fibered space ad­mits a tight con­tact struc­ture if and only if it is not \( 2n-1 \) sur­gery on the \( (2,2n+1) \)-tor­us knot [e51]. Thus, un­der­stand­ing the ex­ist­ence of tight con­tact struc­tures on a giv­en ir­re­du­cible 3-man­i­fold re­duces un­der­stand­ing tight con­tact struc­tures on hy­per­bol­ic ra­tion­al ho­mo­logy spheres. Here vir­tu­ally noth­ing is known.

Know­ing something about the ex­ist­ence of tight con­tact struc­tures on a giv­en man­i­fold, one might ask how many tight con­tact struc­tures can ex­ist on a giv­en 3-man­i­fold. The first res­ult along these lines was again due to Yasha. In [5], Yasha showed that if \( \xi \) was a tight con­tact struc­ture and \( \Sigma \) was any em­bed­ded sur­face, then we have an ad­junc­tion in­equal­ity \[ |\langle e(\xi),[\Sigma]\rangle| \leq 2g(\Sigma)-2, \] where \( \langle e(\xi),[\Sigma]\rangle \) is the pair­ing of the Euler class of \( \xi \) with the ho­mo­logy class of \( \Sigma \) and \( g(\Sigma) \) is the genus of \( \Sigma \). It is easy to see that this means on any com­pact man­i­fold there are only a fi­nite num­ber of co­homo­logy classes that can be real­ized as the Euler class of a tight con­tact struc­ture. This is in sharp con­trast to the case of over­twisted con­tact struc­tures that can real­ize any (even) co­homo­logy class as their Euler class. An­oth­er con­trast with over­twisted con­tact struc­tures can be seen in work of Lis­ca and Mati&cacute [e17], who showed that there are ho­mo­logy spheres that ad­mit an ar­bit­rar­ily large (but fi­nite) num­ber of tight con­tact struc­tures in a fixed ho­mo­topy class! A coarse un­der­stand­ing of tight con­tact man­i­folds was achieved in 2003 by Colin, Giroux, and Honda [e30], [e50], who showed that on any closed, ori­ented 3-man­i­fold there are only fi­nitely many ho­mo­topy classes of plane fields that con­tain a tight con­tact struc­ture and if in ad­di­tion the man­i­fold is at­or­oid­al, then the man­i­fold has a fi­nite num­ber of tight con­tact struc­tures! (We note that if the man­i­fold has in­com­press­ible tori, one can al­ways con­struct in­fin­itely many tight con­tact struc­tures us­ing “Giroux tor­sion”.)

We fi­nally turn to the clas­si­fic­a­tion of tight con­tact struc­tures. Here our know­ledge is sig­ni­fic­antly less than for over­twisted con­tact struc­tures, but it does point to the clas­si­fic­a­tion be­ing quite in­tric­ate and subtle. The first clas­si­fic­a­tion is, of course, due to Yasha. As noted above, in 1992 Yasha showed that \( S^3 \) ad­mits a unique tight con­tact struc­ture up to iso­topy [5]. In 2000, the present au­thor showed that any lens space ad­mit­ted a fi­nite num­ber of tight con­tact struc­tures and proved that for one co­homo­logy class on any lens space, there was a unique tight con­tact struc­ture real­iz­ing it. But the next big break­through was due to Giroux [e20] and Honda [e21], [e23], who clas­si­fied all tight con­tact struc­tures on lens spaces, circle bundles over sur­faces, and tor­us bundles. Their work comes down to study­ing “con­vex sur­faces”, which is now a key tool in the study of con­tact struc­tures. Con­vex sur­face the­ory grew out of Giroux’s [e12] ana­lys­is of the nota­tion of a con­vex con­tact man­i­fold in­tro­duced by Yasha and Gro­mov [4].

Over the last 20 years, there has been a steady stream of clas­si­fic­a­tion res­ults; for ex­ample, [e47], [e40], [e44], [e59], [e41] clas­si­fied tight con­tact struc­tures on many (but not all!) small Seifert fibered spaces and [e38] clas­si­fied such struc­tures on Seifert fibered spaces over \( T^2 \) with a single sin­gu­lar fiber. In ad­di­tion, there have been sev­er­al clas­si­fic­a­tions of tight con­tact struc­tures on some hy­per­bol­ic man­i­folds [e60], [e62]. We did not state the spe­cif­ic clas­si­fic­a­tion res­ults as they can be quite com­plic­ated, but the main point is that we only have clas­si­fic­a­tion res­ults for quite spe­cial man­i­folds, and we see a rich and beau­ti­ful the­ory but still do not have a real un­der­stand­ing of the sub­tleties. Such as, why do some man­i­folds have large num­bers of tight con­tact struc­tures in a fixed ho­mo­topy type of plane field, while oth­ers do not? Why do some con­tact struc­tures stay tight when pulled back to the uni­ver­sal cov­er and oth­ers do not? We clearly have a long way to go to ob­tain a good pic­ture of the num­ber and types of tight con­tact struc­tures a giv­en 3-man­i­fold sup­ports.

As dis­cussed above, one of the main ways to con­struct tight con­tact struc­tures is to con­struct con­tact struc­tures that have sym­plect­ic fillings, and at this point in the story, one might think that tight­ness of a con­tact struc­ture might be equi­val­ent to sym­plect­ic fil­lab­il­ity. It turns out this is not the case as was first ob­served in 2002 by Honda and the present au­thor in [e27]. Since then, there have been con­struc­tions of tight but not fil­lable con­tact struc­tures on some circle bundles [e31], [e37] (but these man­i­folds ad­mit oth­er con­tact struc­tures that are sym­plect­ic­ally fil­lable) and on hy­per­bol­ic man­i­folds [e55], [e57] (these man­i­fold ad­mit no fil­lable con­tact struc­tures at all), but over­all, con­struct­ing tight but non­fil­lable con­tact struc­tures seems dif­fi­cult.

5.3.  Applications of tight contact structures
We have already dis­cussed that the Ben­nequin in­equal­ity holds in any tight con­tact 3-man­i­fold. Thus we see that tight con­tact struc­tures can “see” subtle in­form­a­tion about to­po­logy, that is, they can give bounds on the min­im­al genus of a Seifert sur­face. But there are many oth­er ap­plic­a­tions of tight con­tact struc­tures!

We start with an im­press­ive res­ult of Yasha’s. In [5], Yasha used his clas­si­fic­a­tion of tight con­tact struc­tures on \( S^3 \) to­geth­er with a clev­er use of pseudo­holo­morph­ic curves to re­prove Cerf’s the­or­em which states that any dif­feo­morph­ism of \( S^3 \) ex­tends over the 4-ball. Cerf’s proof [e3] of his the­or­em was im­press­ive and quite in­volved, while Yasha’s proof was one page! (Of course, this is not really quite true, it takes quite a few pages to clas­si­fy tight con­tact struc­tures on \( S^3 \) and then one needs Gro­mov’s the­ory of pseudo­holo­morph­ic curves [e11]. So the proof is not really short­er, but what I find im­press­ive is that the two big pieces of Yasha’s proof were de­veloped for their own reas­ons and when com­bined, one gets a beau­ti­ful proof of this beau­ti­ful res­ult! It really seems like con­tact geo­metry is try­ing to tell us deep things about to­po­logy.)

An­oth­er in­ter­est­ing ap­plic­a­tion of con­tact geo­metry to to­po­logy is Ghig­gini’s proof that knot Hee­gaard Flo­er ho­mo­logy de­tects genus one fibered knots [e48]. Spe­cific­ally, giv­en a non­fibered (genus one) knot \( K \), Ghig­gini con­structs two tight con­tact struc­tures on a man­i­fold ob­tained by 0 sur­gery on \( K \), whose Hee­gaard Flo­er con­tact classes are dif­fer­ent, but in the same grad­ing. The idea be­hind this proof was gen­er­al­ized by Ni to prove that all fibered knots are de­tec­ted by knot Hee­gaard Flo­er ho­mo­logy [e45].

We next ob­serve that Yasha and Thur­ston’s res­ult (dis­cussed above) has ma­jor im­plic­a­tions in the to­po­logy of 3-man­i­folds. For ex­ample, among oth­er res­ults, it was es­sen­tial in Kron­heimer and Mrowka’s proof of the Prop­erty P con­jec­ture [e34], that says non­trivi­al sur­gery on a non­trivi­al knot in \( S^3 \) is not simply con­nec­ted, and Oz­sváth and Szabó’s proof that the Hee­gaard–Flo­er ho­mo­logy de­tects the Thur­ston norm of a man­i­fold and the min­im­al Seifert genus of a knot [e33].

We briefly sketch the proof of one of these res­ults. Re­call know­ing the Thur­ston norm of a ho­mo­logy class is es­sen­tially the same as know­ing the min­im­al genus of a sur­face rep­res­ent­ing that ho­mo­logy class (the norm is ex­pressed in terms of the Euler char­ac­ter­ist­ic of the sur­face, and care must be taken when the sur­face is a sphere). Sup­pose \( \Sigma \) is a min­im­al genus sur­face in \( M \) rep­res­ent­ing a ho­mo­logy class \( h \). In [e9], Gabai tells us that there is a taut fo­li­ation \( \mathcal{F} \) on \( M \) that con­tains \( \Sigma \) as a leaf. Yasha and Thur­ston’s res­ults above then say there is a sym­plect­ic struc­ture on \( X=M\times[-1,1] \) that sym­plect­ic­ally fills \( (M\times\{1\}, \xi_+)\cup (-M\times\{-1\},\xi_-) \) where the \( \xi_\pm \) are pos­it­ive and neg­at­ive ap­prox­im­a­tions of \( \mathcal{F} \). Work of Yasha [9] and the present au­thor [e35] then con­struct a closed sym­plect­ic man­i­fold con­tain­ing \( X \). A non­van­ish­ing res­ult for the Hee­gaard–Flo­er in­vari­ant of a sym­plect­ic man­i­fold in the spin\( ^c \) struc­ture as­so­ci­ated to the sym­plect­ic struc­ture im­plies the non­van­ish­ing of the Hee­gaard–Flo­er group \( \operatorname{HF}^+(M,\mathfrak{s}_{\xi_+}) \), where \( \mathfrak{s}_{\xi_+} \) is the spin\( ^c \) struc­ture as­so­ci­ated to the con­tact struc­ture \( \xi_+ \). We now re­call that for any spin\( ^c \) struc­ture \( \mathfrak{s} \) with \( \operatorname{HF}^+(M,\mathfrak{s})\not= 0 \), we have an ad­junc­tion in­equal­ity \[ |\langle c_1(\mathfrak{s}),[\Sigma]\rangle| \leq 2g(\Sigma)-2, \] where \( \langle c_1(\mathfrak{s}),[\Sigma]\rangle \) is the pair­ing of the Chern class of \( \mathfrak{s} \) with the ho­mo­logy class of \( \Sigma \) and \( g(\Sigma) \) is the genus of \( \Sigma \). Since \( \Sigma \) was a leaf of \( \mathcal{F} \) and \( \xi_+ \) is \( C^0 \) close to \( \mathcal{F} \), it is easy to see that \( \langle c_1(\mathfrak{s}_{\xi_+}),[\Sigma]\rangle=2g(\Sigma)+2 \). Thus we see that we can de­tect the min­im­al genus of a non­trivi­al ho­mo­logy class in \( M \) by see­ing how \( c_1 \) of all the spin\( ^c \) struc­tures on \( M \) with nonzero Hee­gaard–Flo­er ho­mo­lo­gies eval­u­ate on the ho­mo­logy class!

6.  Higher dimensional overtwisted contact structures

As in di­men­sion 3, our dis­cus­sion of the tight versus over­twisted di­cho­tomy in high­er di­men­sions be­gins with the ques­tions of which man­i­folds ad­mit con­tact struc­tures. We saw in di­men­sion 3 that any ori­ented 3-man­i­fold ad­mits such a struc­ture, but in high­er di­men­sions, there are ob­struc­tions to ad­mit­ting a con­tact struc­ture. In­deed, con­sider a co­ori­ented con­tact struc­ture \( \xi \) on a \( (2n+1) \)-man­i­fold \( M \). By choos­ing a con­tact form \( \alpha \) for \( \xi \) we ob­tain a sym­plect­ic struc­ture \( d\alpha \) on \( \xi \). An al­most con­tact struc­ture on \( M \) is a pair \( (\alpha, \omega) \) where \( \alpha \) is a nonde­gen­er­ate 1-form on \( M \) and \( \omega \) is a 2-form that is sym­plect­ic when re­stric­ted to \( \ker \alpha \). Clearly, if \( M \) has a con­tact struc­ture it has an al­most con­tact struc­ture. We also note that wheth­er or not \( M \) ad­mits an al­most con­tact struc­ture is easy to de­term­ine; it is equi­val­ent to the struc­ture group of \( TM \) re­du­cing from \( SO(2n+1) \) to \( U(n)\oplus \mathbb{I} \) and this in turn can be de­term­ined by ob­struc­tion the­ory. So the real ex­ist­ence ques­tion in high­er di­men­sions is wheth­er or not any al­most con­tact struc­ture on a man­i­fold \( M \) is ho­mo­top­ic to a con­tact struc­ture.

There is a long his­tory of study­ing this ex­ist­ence ques­tion and try­ing to define over­twisted con­tact struc­tures in high­er di­men­sions. In 1991, Geiges [e13] showed that every al­most con­tact struc­ture on a simply con­nec­ted 5-man­i­fold is ho­mo­top­ic to a con­tact struc­ture, and in 1993, the case of “highly con­nec­ted” man­i­folds in all di­men­sions was ad­dressed by Geiges [e15]. In 1998, Geiges and Thomas [e18] gave a par­tial an­swer for 5-man­i­folds with \( \pi_1=\mathbb{Z}/2\mathbb{Z} \). Des­pite this pro­gress, the ex­ist­ence ques­tion re­mained elu­sive. For ex­ample, up un­til 2002, it was not known if tori \( T^{2n+1} \) for \( n > 2 \) ad­mit­ted con­tact struc­tures! (In 1979, Lutz [e6] showed that \( T^5 \) ad­mit­ted a con­tact struc­ture, but for over 20 years noth­ing was known about \( T^7 \).) In 2002, Bour­geois [e28] showed that if \( M \) ad­mits a con­tact struc­ture then so does \( M\times T^2 \). The first gen­er­al res­ult was in 2015 when Cas­als, Pan­choli, and Pre­s­as [e54] showed that any al­most con­tact struc­ture on a 5-man­i­fold is ho­mo­top­ic to a con­tact struc­ture.

Shortly after [e54] Yasha, in col­lab­or­a­tion with Bor­man and Murphy, defined what it means for a con­tact struc­ture to be over­twisted in all di­men­sions [11]. The defin­i­tion is a bit more com­plic­ated than in di­men­sion 3, so we refer to the pa­per for the de­tails, but es­sen­tially a con­tact struc­ture \( \xi \) on \( M^{2n+1} \) is over­twisted if there is an em­bed­ding of a piece­wise smooth \( 2n \)-disk that defines the germ of a mod­el con­tact struc­ture. With this defin­i­tion in hand, they were able to show that any al­most con­tact struc­ture on a closed man­i­fold is ho­mo­top­ic to an over­twisted con­tact struc­ture that is unique up to iso­topy. Thus the dif­fi­cult ex­ist­ence prob­lem is now solved in all di­men­sions!

Just as in di­men­sion 3, con­sid­er­ably more is true: Yasha, Bor­man and Murphy ac­tu­ally show that the space of con­tact struc­tures con­tain­ing a fixed over­twisted \( D^{2n} \) and the space of al­most con­tact struc­tures also con­tinu­ing this \( D^{2n} \) are weakly ho­mo­topy equi­val­ent.

Pri­or to the above work on high­er di­men­sion­al over­twisted con­tact struc­tures, there was a pre­vi­ous at­tempt to gen­er­al­ize over­twisted­ness to high­er di­men­sions. In [e42] Neider­krúger defined the no­tion of a plastikstufe. This was something like a para­met­er­ized ver­sion of an over­twisted disk, and he was able to show that hav­ing such an ob­ject im­plied that the con­tact struc­ture could not be sym­plect­ic­ally filled, just like for 3-di­men­sion­al over­twisted con­tact struc­tures! It is not hard to see that an over­twisted man­i­fold con­tains plastikstufe, and in fact, if a con­tact man­i­fold has a spe­cial type of plastikstufe, it will be over­twisted [e58].

Now that we have a no­tion of over­twisted in high­er di­men­sions, we will define a tight con­tact struc­ture to be one that is not over­twisted. As noted above, if a con­tact man­i­fold is sym­plect­ic­ally fil­lable then it is not over­twisted, but one can won­der, as in di­men­sion 3, how tight­ness is re­lated to sym­plect­ic fil­lab­il­ity. The first pro­gress on this was due to Mas­sot, Nieder­krüger and Wendl [e52] who showed that there ex­ist tight man­i­folds that are not sym­plect­ic­ally fil­lable. There have been sev­er­al sim­il­ar res­ults, but very re­cently Bowden, Giron­ella, Moreno and Zhou [e63] showed that tight but not sym­plect­ic­ally fil­lable con­tact struc­tures are every­where. More ex­pli­citly, if \( M \) is a con­tact man­i­fold of di­men­sion at least 7 that ad­mits a Stein fil­lable con­tact struc­ture, then \( M \) ad­mits tight con­tact struc­tures in the same ho­mo­topy class of al­most con­tact struc­ture that is not strongly fil­lable. The same is true for a \( 5 \)-man­i­fold if the con­tact struc­ture has first Chern class equal to zero.

7.  Final thoughts

The tight versus over­twisted di­cho­tomy was born just over 30 years ago in sev­er­al sem­in­al pa­pers of Yasha. This di­cho­tomy crys­tal­lized sev­er­al in­sights of work from the past sev­er­al years and provided a frame­work for the fu­ture of con­tact geo­metry. This frame­work has been the driv­ing force for much of the work in the field and will cer­tainly be so mov­ing in­to the fu­ture.

Acknowledgement

The au­thor would like to thank Lori Le­jeune and Bülent Tosun for their help­ful com­ments on the manuscript.

John Et­nyre is a Pro­fess­or at the Geor­gia In­sti­tute of Tech­no­logy, whose fields of re­search in­clude con­tact geo­metry, sym­plect­ic geo­metry, and low-di­men­sion­al to­po­logy. He earned his Ph.D. in 1996 from the Uni­versity of Texas, Aus­tin and was a postdoc­tor­al schol­ar at Stan­ford Uni­versity from 1997–2001. Et­nyre was a fac­ulty mem­ber at the Uni­versity of Pennsylvania pri­or to join­ing the fac­ulty at the Geor­gia In­sti­tute of Tech­no­logy.

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