Framed Knotoids and Their Quantum Invariants

We modify the definition of spherical knotoids to include a framing, in analogy to framed knots, and define a further modification that includes a secondary ‘coframing’ to obtain ‘biframed’ knotoids. We exhibit topological spaces whose ambient isotopy classes are in one-to-one correspondence with framed and biframed knotoids respectively. We then show how framed and biframed knotoids allow us to generalize quantum knot invariants to a knotoid setting, leading to the construction of general Reshetikhin-Turaev type biframed knotoid invariants.


Introduction and Motivation
Knotoids were introduced by V. Turaev in [15] as a generalization of knots.Intuitively, knotoids are knot diagrams that have open ends; see Figure 2.1 below.Unlike long knots [4, Ch. 1], these end-points are allowed to lie in the interior of the diagram.To prevent all knotoid diagrams from being trivial, the diagrammatic moves in Figure 1.1 are explicitly forbidden.Turaev showed that such diagrams are in correspondence with so-called 'simple theta-curves', in the same way that knot diagrams correspond to knots.In this sense we say that simple theta-curves are the 'geometric realization' of knotoid diagrams.
Knotoids are a natural object to use when studying the knottedness of open-knotted protein chains.This is done in e.g.[7] where the knottedness of a protein is analysed by projecting it onto planes in many possible directions and identifying the resulting knotoids.The result is a map from a discretization of S 2 to the set of all knotoids, which encodes much information about the shape of the protein.
To make this application of knotoids viable for more complex proteins, it is helpful to have a classification of knotoids.The classification of knotoids on the sphere with up to 6 crossings is complete [6], and makes use of strong knotoid invariants such as the arrow polynomial from [8] and the double branched cover from [2].For further progress a larger selection of knotoid invariants is needed.Extending this selection is the primary goal of of this paper.
In this paper the notion of a knotoid diagram is generalized to include a framing, in analogy to framed knots.It is generally easier to construct invariants of framed knots since framed knot diagrams have fewer allowed Reidemeister moves than knot diagrams.This same principle motivates the introduction of framed knotoids to facilitate the production of knotoid invariants.Along with definitions of several notions of framed knotoid diagrams we will also give geometric realizations of these types of diagrams.This helps to keep the theory grounded in topology, before allowing algebraic and diagrammatic manipulations to take over when we move on to constructing framed knotoid invariants.
This construction of framed knotoid invariants leads to the construction of general Reshetikhin-Turaev type quantum invariants of knotoids.This is related to the very recent work by Gügümcü and Kauffman [9] on quantum knotoid invariants.Our work in this paper is independent from theirs, but there are similarities between our approach and theirs: e.g.what we shall call our 'coframing' is analogous to their 'rotation number'.Our approach will add some topological motivation to the ideas developed there, and as a result has a focus on spherical knotoids rather than planar ones.

Definitions and Geometric Realizations
In this section we briefly recall the basic results on knotoids and simple theta-curves, both due to Turaev [15].Afterwards we introduce framed and biframed versions of both knotoids and simple theta-curves.

Knotoids and Simple Theta-curves
Definition 2.1.[15] Let Σ be a surface.A knotoid diagram in Σ is a smooth immersion φ : [0, 1] → Σ • into the interior of Σ, whose only singularities are transversal double points endowed with over/undercrossing data.Knotoid diagrams have a natural orientation, namely from the leg φ(0) to the head φ(1).We will not always label the leg and head or depict knotoids as oriented, but this orientation is always implicit.Two knotoid diagrams are equivalent if they can be related by a sequence of isotopies of Σ and applications of the Reidemeister moves R1, R2, R3 familiar for knot diagrams.Knotoids are the equivalence classes of knotoid diagrams.
Applications of the Reidemeister moves are not allowed to involve the end-points, and indeed the diagrammatic moves in Figure 1.1 are expressly forbidden.The following is immediate from noting that S 2 is isomorphic to the one-point compactification of R 2 .Remark 2.2.Knotoids in Σ = S 2 are equivalent to knotoids in Σ = R 2 modulo the spherical move R4 depicted in Figure 2.2.Note that while this move needs to be imposed on knotoid diagrams in R 2 and may change the equivalence class of a knotoid diagram in R 2 , it is a surface isotopy for knotoids in S 2 given by sweeping a strand external to the diagram along the back of S 2 .Nevertheless, it will be helpful to distinguish this move from other isotopies, so that we are free to think of knotoids in S 2 as lying in R 2 .
We call a knotoid in S 2 spherical.In this paper all knotoids are assumed to be spherical unless stated otherwise.
Remark 2.3.In the remainder of this section we will consider several kinds of embeddings of topological spaces in S 3 , related to 'theta-curves' defined below.All of these topological spaces will be locally homeomorphic to R, R 2 , or R × [0, ∞) except at two points or arcs.All the embeddings that we will consider in what follows will be implicitly assumed to be smooth everywhere except for these points or arcs, where smoothness is not defined.Definition 2.4.[15] A theta-curve θ is an embedding into S 3 of the graph Θ, which consists of two vertices v 0 , v 1 and three edges e − , e 0 , e + joining them.We consider such embeddings up to ambient isotopies of S 3 that preserve the labels of the vertices and edges.If θ is a theta-curve, then omitting any edge from Θ results in an embedding S 1 → S 3 , i.e. a knot.A theta-curve θ is said to be simple if the image of e − ∪ e + is the unknot.
The reason for introducing simple theta-curves is the following geometric realization result, also due to Turaev [15]: Theorem 2.5.There is a bijection between spherical knotoids and label-preserving ambient isotopy classes of simple theta-curves.We say that Θ is therefore the geometric realization of knotoids.
For a detailed proof, see [15,Sec. 6].For us the important parts of the proof are the explicit correspondence, and the notion of a standard theta-curve.Intuitively a thetacurve is standard if e + ∪ e − is manifestly the unknot: lie in the upper-and lower half-plane of R 2 ×{0} respectively, and θ(e + ), θ(e − ) project bijectively to the same arc a ⊆ R 2 ×{0} that connects the vertices of θ.
Turaev shows that any simple theta-curve is ambient isotopic to a standard one, and that if θ, θ are ambient isotopic standard simple theta-curves then they are ambient isotopic within the class of standard simple theta-curves [15].For standard simple thetacurves the bijection of Theorem 2.5 is depicted in Figure 2.3.
Figure 2.3: The bijection of Theorem 2.5.A standard theta-curve produces a knotoid by moving θ(e 0 ) onto a neighborhood of R 2 × {0} and taking a vertical planar projection.A knotoid conversely produces a theta-curve by considering a knotoid diagram as a knotted arc lying in a neighbourhood of R 2 × {0} and tying arcs e ± to its end-points.

Framed and Biframed Knotoids
The aim of this section is to give reasonable definitions of what it means for a knotoid to be framed.First recall the main results on framed knots from [5]: A framed knot K is a knot with a transversal, smooth, everywhere nonzero vector field.The framing of K is then defined to be the associated element in π 1 (SO(2)) ∼ = Z.There is an equivalence between framed knots and tangled ribbons in S 3 , so framed knots can equivalently be characterized as embeddings of the annulus into S 3 .
Any knot diagram induces a blackboard framing on the corresponding knot, with framing integer given by the writhe of the diagram.Letting R1 denote the weakened first Reidemeister move (see Figure 2.4), framed knots up to equivalence are in bijection with knot diagrams up to R1 , R2, R3.Such knot diagrams are referred to as framed knot diagrams.Details can be found in [5].

Framed Knotoids
Given that framed knot diagrams are simply knot diagrams up to the moves R1 , R2, R3, the definition of framed knotoids is natural: Definition 2.7.A framed knotoid is an equivalence class of knotoid diagrams under the equivalence generated by ambient isotopies and R1 , R2, R3.A diagram representing a framed knotoid is also called a framed knotoid diagram.
As the terminology suggests, framed knotoid diagrams are just knotoid diagrams with a 'framing integer' attached.Our immediate goal is to prove this.To extract an integer from a given diagram K in a canonical way we proceed in analogy with framed knots: Definition 2.8.Let K be a framed knotoid diagram.We define the blackboard framing of K to be the writhe of K, i.e. the sum of the signs of all crossings of K.Here the sign of a crossing is defined analogously as for knot diagrams, see [5].
The blackboard framing is an integer that is also well-defined for the framed knotoid that K represents.This last statement follows from invariance of the writhe under R1 , R2, R3.To justify the use of the term 'blackboard framing' for the writhe of a knotoid in analogy with framed knots, we need to interpret the framed knotoid as an object in S 3 with an associated canonical transversal vector field.We do so after introducing framed theta-curves in the next subsection.For now it suffices to work with the combinatorially defined writhe, without reference to a geometric realization.Using the writhe, we conclude the following lemma: Lemma 2.9.There is a bijection Proof.First note that surjectivity is clear.Indeed, given a knotoid diagram K we can add R1 loops to adjust the framing of K at will without altering the underlying knotoid.
(By an R1 loop we mean a loop like those pictured in Figure 2.4.)For injectivity, suppose that K, K are equivalent knotoid diagrams with equal writhe.Then we must show that K, K are equivalent as framed knotoid diagrams.To see this, first note that positive and negative R1 loops can be cancelled against each other via a combination of R2 and R3 moves.See  Since K, K are equivalent as knotoids there is a sequence of isotopies of S 2 and Reidemeister moves that turns K into K.By the above, we can modify this sequence of moves into a sequence of framed knotoid diagram moves.Namely we replace every deletion of an R1 loop by the sequence of isotopies of S 2 and R2, R3 moves that brings this R1 loop to a neighbourhood of the head of K , and every creation of an R1 loop by the creation of that loop and its opposite, followed by moving this opposite to the head of K .The result is the diagram K, but with a finite number of R1 loops concentrated in a neighbourhood of the head.Since K and K have equal writhe, the sum of the signs of these loops is 0. Thus we can apply the moves in Figure 2.5 finitely many times to remove all these loops, ending up with a diagram of K.

Framed Simple Theta-curves
Our next goal is to find a geometric realization of framed knotoids, and to interpret their writhe in terms of the framing of this geometric realization.
This means that we want topological spaces whose ambient isotopy classes in S 3 are in bijection with framed knotoids.Recall that framed knots are equivalent to tangled ribbons in S 3 , and hence the geometric realization of framed knot diagrams is the annulus.Also recall the sketch proof of Theorem 2.5, which implies that knotoids correspond to the edge e 0 of a simple theta-curve.From these two facts it is reasonable to expect that framed knotoids correspond to simple theta-curves in S 3 , with e 0 thickened into a ribbon.The associated geometric realization is pictured in Figure 2.6.Definition 2.10.Let Θ denote the space Θ with the middle edge e 0 thickened into a 2-dimensional ribbon e 0 attached along neighbourhoods of v 0 , v 1 as depicted in Figure 2.6.A framed theta-curve is an embedding Θ → S 3 .We consider such embeddings up to label-preserving ambient isotopies of S 3 .
We say that a framed theta-curve is simple if it has integer framing and the image of e + ∪ e − is the unknot, the former meaning that if we put θ in a form such that e + ∪ e − is manifestly unknotted then the same side of e 0 must face 'outwards' at v 0 and v 1 .In other words, it means that we want θ(e 0 ) to make an integer number of turns through S 3 , in some sense; see Figure 2.6.
To make this notion of 'turns' more precise we define standard framed simple thetacurves and their framing integers: 3 .In analogy to the proof of Theorem 2.5 we say that a framed simple theta-curve θ is standard if the same assumptions on θ(e + ), θ(e − ) as for standard theta-curves hold, and the neighbourhoods of θ(e + ∪ e − ) where θ(e 0 ) is attached are parallel straight lines in R 2 .In particular the example in Figure 2.6 is standard.
Let e 0 be one of the lengths of the boundary of θ(e 0 ).The direction into the interior of e 0 that is transversal to e 0 defines a path in SO(2) when considered along all of θ(e 0 ).In the case of a standard simple framed theta-curve this path is a loop by assumption.The corresponding element of π 1 (SO(2)) ∼ = Z is defined to be the framing integer fr(θ) of θ.
Remark 2.12.Note that any framed simple theta-curve can be brought into standard form.Indeed, it suffices to extend the same moves that bring a simple theta-curve into standard form to a framed simple theta-curve, and then to adjust regular neighbourhoods of the end-points to be vertical.(For the definition of a regular neighbourhood of an endpoint, see [15].Here we assumed without loss of generality that the attachments of e 0 lie inside such a neighbourhood.)This works because any move on theta-curves can easily be extended to a move of framed theta-curves, up to deformations that shrink a portion of the ribbon e 0 .We will see in subsection 2.2.3 that for biframed theta-curves this is not quite the case.
It is clear that the framing integer is independent of the standard form produced in this way.Indeed, the relative twisting between the transversal vectors to e 0 into e 0 at v 0 , v 1 when transforming a theta-curve into standard form is clearly independent of the standard form chosen. Remark 2.12 allows us to define the framing integer of any simple theta-curve θ, namely as the framing integer of any standard theta-curve equivalent to θ.Using this we can conclude the following: Lemma 2.13.There is a bijection where θ • is the simple theta-curve obtained from the projection e 0 e 0 of a ribbon onto one of its 1-dimensional boundary lengths (which is a smooth arc).
Proof.This proof is analogous to that of Lemma 2.9: surjectivity is clear.For injectivity suppose that θ 1 , θ 2 have equal framing and that θ Then an ambient isotopy relating θ • 1 to θ • 2 can be extended to an ambient isotopy relating θ 1 to a theta-curve This extension may end up adding extra twists (both clockwise and counter-clockwise) to θ 3 that are not present in θ 2 .But since fr(θ 3 ) = fr(θ 1 ) = fr(θ 2 ) these extra twists must cancel to give θ 1 θ 3 θ 2 , proving injectivity.
Combining bijection (2.2) with bijection (2.1) and Theorem 2.5 gives a sequence of bijections ( Thus we obtain the following corollary to Theorem 2.5: Corollary 2.14.The geometric realization of framed knotoids is Θ, i.e. the equivalence classes of embeddings of Θ are in bijective correspondence with framed knotoids. Remark 2.15.A priori the bijection of Corollary 2.14 is not topological in nature: it simply says that both framed knotoids and framed simple theta-curves correspond to knotoids with an integer attached.As with framed knots, the topological interpretation of Corollary 2.14 passes through the blackboard framing.Given a knotoid diagram K, let K be given by a small shift transversal to K; see Figure 2.7.Under the inverse of the projection assignment from Theorem 2.5, this K specifies a transversal vector field on e 0 of the standard theta-curve corresponding to K. (As a convention, we take this vector field to be upwards in R 2 × {0} at v 0 , v 1 .)In turn this specifies a ribbon extension e 0 to e 0 .The corresponding framing is defined to be the blackboard framing of K.This is a number equal to the writhe of K.The proof of this is analogous to that for framed knots; see [5].
In this way, the notions of framing for knotoids and theta-curves coincide under the map {Knotoids} → {Simple theta-curves} from Theorem 2.5.
Framed simple theta-curves, and hence framed knotoids, could be useful in their own right for modelling DNA structures.Namely the framing can be used to model the double helix structure of a DNA strand more accurately.A consequence is that framed knotoid models of DNA can detect features such as supercoiling [3], which is undetectable by knotoid models due to the R1 relation.For such modelling purposes, it is natural to ask whether knotoids can be generalized to encode non-integer framing.Clearly this can be done for framed simple theta-curves, but there is no simple way to translate this to knotoid diagrams.
Defining a notion of half-integer framing that is easy to recognize in diagrams is one of the motivations for introducing 'biframed ' knotoids and theta-curves in the next subsections.

Biframed Simple Theta-curves
To define biframed knotoids we will work backwards; we start by defining the geometric realization and its embeddings, and consider the associated diagrams in the next subsection.The idea of a biframed theta-curve is to take a framed theta-curve, and add a secondary coframing by allowing the outer ring e + ∪ e − to carry framing information.The associated geometric realization is depicted in Figure 2.8.Definition 2.16.Let |Θ| denote the space depicted on the left in Figure 2.8, i.e. the space Θ with {e − , e 0 , e + } thickened into ribbons {e − , e 0 , e + } and with e 0 attached at attaching arcs a 0 , a 1 along the width of e − ∪e + .This means that if we note that e + ∪e − ∼ = S 1 ×[0, 1] then the arcs a i are equal to p i × [0, 1] for some p i ∈ S 1 and i ∈ {0, 1}.A biframed theta-curve is an embedding θ : |Θ| → S 3 .We consider such embeddings up to labelpreserving ambient isotopies of S 3 .
To justify the terminology 'biframed', we give a way of assigning two numbers to (a certain class of) biframed theta-curves.One of these is analogous to the framing of a framed theta-curve.The other is derived from the fact that for a biframed theta-curve e − ∪ e + is also a ribbon, and shall be referred to as the 'coframing' of a biframed thetacurve.As for framed theta-curves, to facilitate the definition of these numbers we first define a class of 'standard' theta-curves.Definition 2.17.A biframed theta-curve θ is said to be standard if the following conditions hold: • The annulus θ(e − ∪ e + ) is the unframed (i.e.framing 0) unknot, and θ(a i ) lies in the horizontal plane R 2 × {0} ⊆ S 3 for i ∈ {0, 1}.
• The annulus θ(e − ∪ e + ) is in manifestly unframed form, i.e. of the form • Let e 0 denote one of the lengths of the boundary of θ(e 0 ).Some neighbourhoods of the attaching arcs of θ(e 0 ) to θ(e − ∪ e + ) lie in a single plane P , and the tangent of e 0 is perpendicular to θ(e − ∪ e + ) at both attaching points.
• Away from the attaching arcs, θ(e 0 ) does not intersect the vertical bars perpendicular to P that are depicted in Figure 2.9.
Figure 2.9: A standard embedding of |Θ|, along with the vertical bars from Definition 2.17 that θ(e 0 ) is not allowed to intersect.
Definition 2.18.Let θ, e 0 be as in Definition 2.17.As with framed theta-curves, the direction of the interior of θ(e 0 ) perpendicular to e 0 determines a framing integer in π 1 (SO( 2)) ∼ = Z.To define the coframing, parametrize e 0 by t ∈ [0, 1] such that e 0 (0) ∈ a 0 and e 0 (1) ∈ a 1 .Note that e 0 is a smooth arc by assumption on θ : |Θ| → S 3 .For t ∈ (0, 1) and i ∈ {0, 1}, consider the vectors in S 3 from e 0 (i) to e 0 (t).Project these vectors onto P and normalize them.This is possible by the fourth assumption of standard-ness: note that without this assumption some of these projections onto P could yield the zero vector.This results in paths p i in SO (2), which are loops by the first and third assumption of standard-ness.Let n i denote the associated elements of π 1 (SO(2)) ∼ = Z.Then we define the coframing of θ to be given by It is easy to see that any biframed theta-curve θ for which θ(e − ∪ e + ) is the unframed unknot can be put into standard form: moves of a theta-curve away from the attaching points extend readily to moves of biframed theta-curves.Moves at the attaching points can be extended by replacing swivels around the end-points by twists that drag e 0 along, as in the right-hand side of Figure 2.11.After such an extension, θ can be put into standard form by applying moves such as that depicted in the right-hand side of Figure 2.11 to put θ(e − ∪ e + ) into standard unframed form, followed by deformations in regular neighbourhoods of a 0 , a 1 and deformations moving θ(e 0 ) away from the bars of Figure 2.9.
Remark 2.19.As before it is clear that fr(θ) is independent of how θ is put into standard form, but this is not immediate for cofr(θ): the ambiguity arises because we can undo a twist in θ(e − ∪ e + ) either at a 0 or at a 1 , dragging e 0 around one end of θ(e − ∪ e + ) or the other.This is illustrated in Figure 2.10.
As can be read off immediately from Figure 2.10, the difference between undoing a twist in θ(e − ∪ e + ) at one end or the other is a difference n i → n i − 1 for i ∈ {0, 1}.The minus sign in Equation (2.4) cancels this difference, so that the coframing is independent of the chosen standard form.Analogous reasoning holds for oppositely directed twist in θ(e − ∪ e + ).Thus Definition 2.18 gives a well-defined coframing for any biframed theta-curve θ such that θ(e − ∪ e + ) is the unframed unknot.Definition 2.18 and Remark 2.19 allow us to define the framing and coframing of any biframed theta-curve θ for which θ(e − ∪ e + ) is the unframed unknot.Using this we can define the objects that are of interest to us, namely 'simple' biframed theta-curves: Definition 2.20.A biframed theta-curve θ is simple if the annulus θ(e − ∪ e + ) is the unframed unknot and θ has integer framing and coframing numbers.
In particular the example shown in Figure 2.8 is simple.
Remark 2.21.For both standard and simple biframed theta-curves, note that we have restricted to embeddings of |Θ| such that e − ∪ e + has framing 0. One may think that the complexity added by making e − ∪ e + a ribbon is negated by this restriction.To see that this is not the case, consider  Figure 2.11 depicts two simple biframed theta-curves.Indeed, for the second thetacurve e − ∪ e + can clearly be deformed into the standard unframed form (as depicted).However, the deformation that accomplishes this drags e 0 around e − ∪ e + , as pictured, resulting in a biframed theta-curve that differs from the first.The coframing is defined to record exactly such differences.
The upshot of the biframing is the following lemma: Lemma 2.22.There is a bijection: Here θ • is the theta-curve given by any one component of the 1-dimensional boundary of θ(|Θ|).

Biframed Knotoids
Next we define biframed knotoids.As the terminology suggests, this will turn out to be the class of diagrams whose geometric realization is |Θ|.In light of Remark 2.15 and the proof of Theorem 2.5, it is no surprise that these are the knotoid diagrams obtained from projecting the smooth arc e 0 of a standard biframed theta-curve onto its plane P .Definition 2.23.Pick two points v 0 , v 1 ∈ S 2 .Denote the directed straight arc in R 2 ∪ {∞} ∼ = S 2 from v 0 to v 1 by L. A biframed knotoid diagram is a knotoid diagram K in S 2 with leg and head equal to v 0 and v 1 respectively, such that the tangents of K coincide with L in neighbourhoods of v 0 , v 1 .Two biframed knotoid diagrams are said to be equivalent if they can be related by applications of R1 , R2, R3, R4, ambient isotopies of S 2 away from v 0 , v 1 , and the coframing identities depicted in Figure 2.12 which encode the move in Figure 2.10.
Figure 2.12: The coframing identities.Here K denotes the rest of the knotoid diagram, which is fixed under the identities.
Fixing v 0 , v 1 uniformly for all biframed knotoid diagrams prevents the case of biframed knotoid diagrams that are in-equivalent only because their end-points disagree and cannot be moved.An example of a biframed knotoid diagram is given in Figure 2.13.To give meaning to the above terminology, we define the framing and coframing of a biframed knotoid diagram.After Definitions 2.8 and 2.18, there are no surprises here.Definition 2.24.Let K be a biframed knotoid diagram.We define its framing to be its writhe.To define its coframing, let n i be the winding number of K around v i for i ∈ {0, 1}.By assumption on the tangents of K, n i ∈ Z.In analogy with Equation (2.4) we define the coframing of K by cofr(K) = n 0 − n 1 .
To see that the coframing is well-defined we must verify that it is invariant under the moves on biframed knotoid diagrams.This is the content of the following lemma.
Proof.The only moves for which invariance is not immediate are the non-local moves, i.e.R4 and the coframing identities.The coframing is defined to be invariant under the coframing identities, namely these identities respectively change both n 0 and n 1 by ±1, and so these changes cancel in the definition of cofr(K).Next say that R4 is applied to an arc that traverses α i radians around v i .Then the new arc traverses −(2π − α i ) radians around v i .Noting that we see that these differences again cancel in the definition of cofr(K).
Lemma 2.26.There is a bijection Proof.Clearly n 0 , n 1 , and hence the coframing of a biframed knotoid, can be adjusted at will by adding loops around v 0 as needed.Combined with bijection (2.1), this gives surjectivity of assignment (2.6).Injectivity follows from bijection (2.1), and reasoning analogous to the proof of bijection (2.1) for the coframing: in short, an equivalence K K as knotoids can be extended to an equivalence of biframed knotoids, up to loops around v 0 , v 1 which must cancel via Figures 2.12 and 2.14 if we assume cofr(K) = cofr(K ).Thus assignment (2.6) is a bijection.As an extension to Remark 2.15, bijection (2.7) also has a topological realization analogous to the 'projection' θ → e 0 from Figure 2.3.The respective definitions of framing for diagrams and theta-curves translate to each other under this projection via the blackboard framing as before, and the respective definitions of coframing are set up so that they translate to each other immediately under this projection.

Half-integer Coframing
Our original motivation for introducing biframed theta-curves was finding a way of adding a 'half-twist' to a framed knotoid in such a way that can be seen easily in the corresponding knotoid diagrams.Here we discuss how biframed knotoids provide this feature by extending the discussion to non-integer coframing.
Biframed knotoids with half-integer coframing are obtained simply by weakening the condition of simplicity of a biframed theta-curves by removing the requirement that the coframing be integer.This adds the possibility of theta-curves with θ(e 0 ) attached to θ(e − ∪ e + ) at the back.See  Such an attachment at the back can occur at either end of θ(e 0 ), and we can translate between these two cases via the isotopies shown in Figure 2.16.These same isotopies show that a biframed theta-curve with two half-integer coframing attachments is nothing but an integer-coframing theta-curve, as the terminology 'half-integer' suggests.The coframing of a half-integer coframing theta-curve is defined analogously as for the integer-coframing case, i.e. by putting the theta-curve in standard form and subtracting the turning numbers of θ(e 0 ) around its attachments to θ(e − ∪ e + ).
Half-integer coframing manifests in biframed knotoid diagrams as the possibility of the tangent vectors at the end-points to be opposite to L. See Figure 2.17.(Again, the coframing in this case is defined as a difference of turning numbers, exactly as for integer-coframing knotoid diagrams.) To properly define half-integer coframing knotoids, then, we need to add coframing identities encoding the moves in Figure 2.16 and similar such moves.
There are a total of 6 coframing identities that need to be added; the three identities involving a positive half-integer coframing attachment at the leg are depicted in Figure 2.18.

Quantum Knotoid Invariants
In this section we begin by recalling the construction of quantum knot invariants, specifically Reshetikhin-Turaev invariants, and then give several generalizations of such invariants to the setting of knotoids using framed and biframed knotoid diagrams.One such generalization relies a slight modification to the setup of quantum invariants, moving to the setting of 'braided groups'.Hence we first recall this setup very briefly.

Reshetikhin-Turaev Invariants
We follow standard notation from [13], where C is a category, ⊗ provides a monoidal structure on C with unit k, (Ψ, ν) further provide a ribbon braided structure on C, and (•) * is a dualization operation on C that turns it into a rigid category via (ev, coev).Recall that quantum knot invariants are constructed by fixing a rigid ribbon category (C, ⊗, k, Ψ, (•) * , ev, coev, ν), picking an object V of C, and mapping a knot diagram to an element of Hom C (k, k) via the assignment specified on elementary tangles by Figure 3.1.This assignment, call it ϕ, is extended to arbitrary tangle diagrams via the rules , where the tensor product and composition of tangles denote their horizontal and vertical juxtapositions respectively.For a more detailed discussion see [10].
Here ev V and coev V are defined using the ribbon element ν −1 V , as is detailed for coev V .Our convention is that knot diagrams are read top to bottom, with downward strands represented by V and upward strands by V * .More generally for crossings that involve V * , Ψ is assigned to positively oriented crossings and Ψ −1 to negative ones.
The assignment ϕ is well-defined on framed tangles, and therefore provides an invariant of oriented framed knots for any choice (C, V ) when applied to a knot diagram viewed as a tangle with no in-or out-going strands.Such an invariant is computed by selecting a 'Morse decomposition' of the knot; dividing it into a composition of tangles, each of which is a finite tensor product of elementary tangles.
For our purposes here, we will wish to extend ϕ to the setting of tangle diagrams decorated with splittings and mergings of strands.To this end, consider a Hopf algebra (H, •, ∆, η, , S), following standard notation from [12].Then in analogy with ϕ we can represent morphisms H ⊗n → H ⊗m as tangles decorated with splittings, mergings, and end-points as in Figure 3.2.Notice that the second-to-last axiom in Figure 3.3 contains a crossing.For Hopf algebras this represents the vector space isomorphism τ : V ⊗ W ∼ = W ⊗ V , i.e. the trivial braiding on the category Vect k .The diagrammatic notation developed so far now suggests we define the following: If B is a braided group in C, then the inverse of Figure 3.2 provides an extension of ϕ to tangle diagrams decorated with splittings, mergings, and end-points.This extension is well-defined on decorated framed tangles because ϕ is, and because we can pull the decorations under and over crossings by naturality of Ψ, Ψ −1 .
Finally recall that to produce explicit Reshetikhin-Turaev invariants one usually picks a ribbon Hopf algebra H and picks C = H M F , the category of finite-dimensional Hmodules.By the representation theory of Hopf algebras this is a rigid ribbon category [12,Ch. 9].A closely related choice is C = H H M F , the category of finite-dimensional crossed H-modules, which is equivalent to D(H) M F for H finite-dimensional where D(H) is the Drinfeld double of H [13, Ch. 10].

Group-Based Invariants
In this subsection we generalize quantum invariants resulting from seeing a finite-dimensional Hopf algebra H as a crossed module in H H M F = D(H) M F .We restrict to H = kG for k a field and G a finite group because it will give us an additional knotoid invariant for free, but the contents of this subsection generalize readily to arbitrary (finite-dimensional) H as in [16].
where g, h, a, b ∈ G, and δ a is the Kronecker delta function taking value 1 on a. Moreover D(kG) has quasitriangular structure R given by Here e ∈ G is the group unit.For more details see [12,Ch. 7].Note that each term of R ∈ D(H) ⊗ D(H) consists of a 'left part' (δ g ⊗ e) and a 'right part' (1 ⊗ g); similarly for R −1 .Now let K be a framed knot.Present K as an oriented long knot diagram.Then V G (K) is an element of Hom(kG, kG) ∼ = (kG) * ⊗ kG = D(kG).To compute this element we place at every crossing of K a copy of R if the crossing is positive, or a copy of R −1 if it is negative.We then trace through the long knot diagram of K following its orientation.Beginning with the unit 1 ⊗ e ∈ D(kG), every time we encounter a crossing we multiply (from the left) with the left part of R or R −1 if we are going under the crossing, or with the right part if we are going over.After the final crossing we sum over all indices of all crossings, and the result is equal to V G (K) [16].To obtain the knot invariant associated to this long knot invariant one takes the trace of V G (K) ∈ Hom(kG, kG).The result is the cardinality of Hom(π 1 (S 3 − K), G) [13,Ch. 13], for reasons we shall soon discuss.
As we shall see in the next subsection, the general Reshetikhin-Turaev invariant construction is tricky to generalize to knotoids.However, the above algorithm for computing V G generalizes effortlessly to give a framed knotoid invariant: Definition 3.2.Let K be a diagram for a framed knotoid.Recall that all knotoids are implicitly oriented from leg to head.Define V G (K) ∈ D(H) by the same process as above, tracing through K from leg to head.
Proof.Invariance under ambient isotopy and the spherical move R4 is immediate since these moves do not alter the crossing data of K. Thus it suffices to check invariance of V G (K) under R1 , R2, R3.This follows from V G being an invariant when defined on framed (long) knots.For completeness, we also prove by hand that V G is a framed knotoid invariant below: Since the oriented versions of R1 do not change the signs of crossings, invariance of The move R2 has four oriented versions.The move R3 has eight.For brevity we consider only one of each; see Figure 3 orientation of R2, one is positive and the other negative.To find invariance we must show that the contributions from these crossings cancel.Indeed, the bottom arc gives a contribution The top arc gives a contribution (1 ⊗ g)(1 ⊗ h) which is thus (1 ⊗ e) for nonzero contributions.Noting that h (δ h ⊗ e) = 1 ⊗ e we see that the contribution of the bottom arc is also trivial, as required.
To verify invariance under the R3 move in Figure 3.4, we calculate the contributions of both sides and show they are equal.When running through K, suppose we pass through the vertical line first, then through the line going diagonally up, and finally through the strand going diagonally down (other orders are proven analogously).Then we compute V G (K) on the left-hand side to be Here the (. . . ) are generic placeholder for contributions due to the rest of K. Now we drag the term (δ k −1 ⊗ e) towards the middle contribution.Every time an element of the form (1 ⊗ x) is encountered, the argument of δ k −1 is conjugated by x −1 .Thus we find for some word w on G.This implies that g −1 = kwk −1 w −1 k −1 .Thus we conclude Following the same procedure on the right-hand side (with the labels g, h, k attached to the same crossings as before) we find (Note that w here is the same word as in the left-hand side computation!)We thus conclude that V G is indeed invariant under R3, completing the proof.
Here the last two equalities use that δ a δ b = 0 ⇐⇒ a = b.This also means that a choice of (g, k) only gives a nonzero contribution to V G (K) if gkg = kgk.In other words, we only obtain a contribution to V G (K) if B 3 → G : (x, y) → (g, k) constitutes a group homomorphism, where is the braid group on 3 strands.
At the beginning of this subsection we stated that taking H = kG gives us an extra knotoid invariant for free.Indeed, this follows from the relation between V G and the Wirtinger presentation of the knot group π 1 (S 3 − K).See [14,Ch. 3] for more on the Wirtinger presentation.Namely, if K is a knot presented as a long knot diagram then after some simplification V G (K) is of the form Here the subscripts of the δ's are words in (g, h, . . .).We only get a non-zero contribution to V G for g, h, . . .such that all these words coincide.The multiplication in D(H) is set up precisely so that the relations corresponding to coincidence of these words are exactly the relations of the Wirtinger presentation.Indeed: if we encounter a term in V G such as then to arrive at the reduced form for V G we must pull the δ h term to the left.The multiplication in D(H) prescribes that this term equals This conjugation by g reflects exactly the action of going under the over-lying g-strand and back again in order to relate h to k, which is precisely the setup of the Wirtinger presentation.
In conclusion, the invariant V G gives us an alternative way of computing the Wirtinger presentation.This implies that nonzero contributions to V G (K) correspond to homomorphisms π 1 (S 3 − K) → G.Both of these results are well-known [1].The novelty is that we have extended V G to framed knotoids, and so this interpretation of V G allows us to associate a group to knotoids.
where each w i is a word in g 1 , . . .g n .We define the knotoid group W (K) of K by the presentation: Remark 3.6.One might expect the knotoid group W (K) to be isomorphic to the fundamental group of S 3 with an arc that projects to give K removed, in which case it is isomorphic to S 3 with an arc removed and hence trivial.Instead W (K) is a group defined by the combinatorial information of K and hence not necessarily related to any fundamental group.We shall see below that it is nontrivial in general.A knotoid group was also defined by Turaev directly via the Wirtinger presentation [15].Turaev's knotoid Figure 3.6: The knotoids K 1 and K 2 , corresponding respectively to orientations of the knotoids 5 5 and 5 24 in the knotoid table from [6]. and Taking G = S 3 , we find that both V S 3 (K 1 ) and V S 3 (K 2 ) have 12 nonzero contributions.More specifically, we find where the omitted terms in both expressions each consist of ten terms only involving the 2-cycles (1, 2), (1, 3), (2, 3) ∈ S 3 .From these computations we note that #Hom(W (K 1 ), S 3 ) = 12 = #Hom(W (K 2 ), S 3 ), meaning that #Hom(W (•), S 3 ) cannot distinguish K 1 and K 2 .However, the expressions of V S 3 (K 1 ) and V S 3 (K 2 ) given above clearly show that V S 3 (K 1 ) = V S 3 (K 2 ), which implies that V S 3 (•) can distinguish K 1 and K 2 .We therefore conclude that V G (•) can be a strictly stronger invariant than #Hom(W (•), S 3 ), as claimed.

Reshetikhin-Turaev Invariants of Knotoids
There are two main obstructions to extending general Reshetikhin-Turaev invariants to framed knotoids.The first point is of course that of determining what to do with the endpoints.The second obstacle is that for a (framed) knotoid diagram, one is able to swivel the tangent vector at the end-points to go, say, either up or down.Such swiveling affects the number of 's and 's in a Morse decomposition of the diagram.Unfortunately there is no reason that a Reshetikhin-Turaev-type assignment of morphisms to knotoid diagrams should be invariant under this action.
Fortunately, in light of Section 2 we are equipped to solve this second problem.Namely, restricting our scope to producing invariants of biframed knotoids removes the obstruction entirely.A posteriori this is one of the main reasons for being interested in biframed knotoids in the first place!Naturally, the first obstruction admits several solutions.Intuitively one would think to extend ϕ to knotoid diagrams by assigning to and morphisms k → V and V → k respectively.However, by naturality of Ψ and Ψ −1 , ϕ would then be invariant under the forbidden moves in Figure 1.1 causing the associated invariant to be trivial.
Here we consider two options of how to handle and .

Option 1
The next best thing to representing and by morphisms k → V or V → k, is to represent them by linear maps that are not morphisms.Definition 3.10.Suppose C = H M F for some ribbon Hopf algebra 1 H.Let V be an n-dimensional object of C, and K a biframed knotoid diagram.For simplicity we assume K has integer coframing.View K as a tangle decorated with two endpoints representing maps η : k → V and : V → k.Extend ϕ to an assignment on K, by choosing a basis {e 1 , . . ., e n } of V and defining c i e i and : where {c i , d i } n i=1 consists of elements of k.The maps η and are chosen to be linear maps, but not H-module isomorphisms.The Reshetikhin-Turaev invariant associated to K is then ϕ(K).
This solution is closely related to the approach taken in [9].It has the advantage of being a simple and natural extension of ϕ.A distinct disadvantage is that this construction has no reason a priori to be invariant under the coframing identities, nor under the spherical move of Remark 2.2.Thus in general this approach yields invariants of planar 'triframed' knotoid diagrams, meaning that both endpoints have separate coframings which are not related by a coframing identity.
If we allow the end-points of these triframed knotoids to move around on R 2 , keeping the tangent vectors at the leg and head fixed, then we end up with the 'Morse knotoids' from [9].It turns out that the construction of quantum invariant given here also yields invariants of Morse knotoids, and that these Morse knotoids are essentially biframed planar knotoids in the sense that they can be described by knotoid type, framing integer, and 'rotation number'.The rotation number is equivalent to the coframing as defined for diagrams in Definition 2.24.See [9] for more details.To keep the discussion below self-contained, we will work with triframed knotoid diagrams.
Example 3.11.We consider the example of H = U q (sl 2 ), letting V be the standard 2dimensional representation.In this case the structures of Ψ, ev, coev, etc. are well-known (up to a choice of normalization); see e.g.[4, Ch. 2.6] or [10,Ch. 9.4].Let {e 1 , e 2 } be the standard basis on V , {e 1 , e 2 } the dual basis on V * , and {e 1 ⊗ e 1 , e 1 ⊗ e 2 , e 2 ⊗ e 1 , e 2 ⊗ e 2 } the standard ordered basis of V ⊗ V (and similarly for V * ⊗ V , V ⊗ V * ).Then the values of ϕ on knot diagram elements with respect to these bases are given in Figure 3.7.
From now on, assume for simplicity that we are working with a (triframed) knotoid diagram K with integer coframing, drawn so that the tangent vectors at the end-points of K are vertical.We can now carry out computations analogously as one does for knot diagrams, e.g.computing that q 1/4 R − q −1/4 R −1 = (q 1/2 − q −1/2 )I 4 , where I 4 is the identity matrix of dimension 4. We conclude the following: Proposition 3.12.Write Q sl 2 to denote the assignment ϕ for our choice of (C, V ).Then this assignment constitutes the existence of a class of triframed knotoid invariants, satisfying the properties of Figures 3.8 and 3.9.This class is indexed by the four free parameters c 1 , c 2 , d 1 , d 2 .
Our next question is whether we can pick c 1 , c 2 , d 1 , d 2 so that Q sl 2 is invariant under the coframing identities.To this end we calculate the value of Q sl 2 on coframing loops around either end-points.See Figure 3.10.
If we take c 1 = d 1 and c 2 = d 2 then adding a (+1)-coframing loop clearly has the same effect when added around either end-point, and similarly for (−1)-coframing loops.Thus in this case Q sl 2 is seen to be invariant under the coframing identities.
In particular taking c 1 = c 2 = d 1 = d 2 = 1/ √ 2 we conclude: Proposition 3.13.There exists an invariant of biframed planar knotoids, denoted Q sl 2 , possessing the properties from Figure 3.9 and satisfying One can adjust this invariant using the integer fr(K) to obtain an R1-invariant version of Q sl 2 exactly as one does for knots.For knots this results in the Jones polynomial [10,Ch. 9.4].Using the integer cofr(K) one can similarly adjust Q sl 2 to be coframing-invariant, resulting in an extension of the Jones polynomial to knotoids.Such an extension was already given in [8], and these extensions must agree up to normalization since a knotoid invariant is uniquely defined by its Skein relations and its values on unknotted components (given that an invariant with these Skein relation exists, which is the statement of Proposition 3.11).Also note that the Kauffman bracket was already extended to knotoids in [15].

Option 2
Our second suggestion for extending ϕ loses the advantage of being particularly simple, but in return has several pleasant features: it is guaranteed to be a biframed spherical knotoid invariant and requires no additional choices after (C, V ) are fixed.Moreover it has a strong topological motivation; namely we extend ϕ by not just considering a biframed knotoid, but a planar projection of the entire theta-curve associated to it: Definition 3.14.Let B be a braided group in a rigid ribbon category C. Let K be a biframed knotoid, assuming for simplicity that K has integer coframing.Take a diagram of K such that the tangent vectors of K at the endpoints are vertically downwards.Now replace the leg of K by a splitting ∆ representing the coproduct of B, attaching K on the left-hand side, and replace the head by a merging • representing the product of B, again attaching K on the left.See figure 3.11.Proof.Invariance under R1 , R2, R3 and isotopies away from the end-points follows from the invariance of ϕ under these moves, so for the first statement it suffices to prove invariance under the spherical move R4 and the coframing identities.
Invariance under R4 is clear, since strands can be moved over (•, ∆) and hence all of K, and oppositely oriented R1-loops cancel by Figure 2.5.
To show invariance under the first coframing identity from Figure 2.12 we do some preliminary computations, depicted in Figures 3. 13    In Figures 3.13 and 3.14 we turn (•, ∆) around to depict morphisms (∆ * , • * ) on B * .The morphisms defined as such diagrammatically extend to a canonical braided group structure on B * for which the diagrammatic moves we have used hold by definition; see [11,Prop. 4.11].
Using these preliminaries, as well as two applications of R1 , invariance of ϕ θ (K) follows from the sequence of moves depicted in Figure 3.15.Invariance under the other coframing identity is shown analogously.For the final statement of the theorem, let D 1 and D 2 denote the oriented tangle diagrams that ϕ θ assigns to both sides of one of the moves in Figure 1.1.Then clearly D 1 and D 2 differ by at least one crossing change, and so in general ϕ θ (K) cannot be invariant under either of these moves.
Remark 3.17.The proof of Theorem 3.16 shows in particular how ϕ θ (K) changes under adjustment of the coframing: namely by adding an R1-loop to the strand of K representing e + , and an oppositely oriented R1-loop to the strand representing e − .This remark also motivates why biframed knotoids are a natural object to consider if one wants to extend quantum knot invariants to knotoids or their associated thetacurves.Namely because quantum invariants are only R1 -invariant and not R1-invariant, one would expect the lines representing e ± to need to be framed as well.As the proof of Theorem 3.16 shows, it turns out biframed knotoids provide a proper framework for this in the case of spherical knotoids.
Although we have assumed K has integer coframing in Definition 3.14, the above generalizes readily to half-integer coframing.The only adjustment that needs to be made is that ∆ must be replaced by • * (or • by ∆ * ) at one endpoint.The construction is depicted (on its side) for an example half-integer coframing knotoid in Figure 3.16.
As a closing remark, we briefly discuss the existence of the objects required to construct an invariant of the type suggested in Definition 3.14.To see this existence we must exemplify braided groups in ribbon categories.Taking the ribbon category H M F for a Hopf algebra H and noting that braided groups in H M F are Hopf algebra objects, it is natural to hope H might be a braided group, or at least a bialgebra object in H M F , when acting on itself suitably.
In fact if we take the adjoint action Ad of H on itself, then • is automatically an intertwiner [13,Ch. 2].If moreover H is cocommutative then ∆ is also easily seen to be an intertwiner, giving an example of a nontrivial object suitable to apply Definition 3.14.

Figure 2 . 2 :
Figure 2.2: The spherical move on a knotoid diagram, where K denotes the rest of a fixed knotoid diagram.

Figure 2 . 16 :
Figure 2.16: Translating a half-integer coframing attachment from a 1 to a 0 .(A re-coloring occurs in the last equivalence.)

Figure 3 . 3 :
Figure 3.3: The axioms of a Hopf algebra in diagrammatic notation.

Definition 3 . 1 .
[11,12] Let C be a ribbon category.A braided group (or 'Hopf algebra object of a ribbon category') is an object B of C endowed with morphisms• : B ⊗ B → B, ∆ : B → B ⊗ B, η : k → B, : B → k, S : B → B. These morphisms must be such that the axioms depicted in Figure 3.3 are satisfied when considered as equations of morphisms via Figures 3.1 and 3.2.This means the crossing in Figure 3.3 is now taken to represent Ψ instead of τ , in accordance with Figure 3.1.

For
H = kG, we first describe an alternative way of computing the framed knot invariant associated to H ∈ H H M F .Call this invariant V G .Note that D(kG) = (kG) * ⊗ kG ∼ = k(G) ⊗ kG, where k(G) is the group of functions G → k, and multiplication in D(kG) is given by (

Example 3 . 4 .Figure 3 . 5 :
Figure 3.5: Construction of V G for an example framed knotoid.crossings of K are indicated in Figure 3.5, as are the nontrivial parts of R, R −1 that occur in the construction of V G .Using the definition of V G and Equation (3.1) we compute:

Figure 3 .
Figure 3.11: Attaching ∆ and • to the leg and head of K, respectively.The dotted lines depict 4 open ends.

Figure 3 . 13 :
Figure 3.13: Turning coframing into framing at the leg of K.

Figure 3 . 14 :
Figure 3.14: Turning coframing into framing at the head of K.