Blog

  • Cut points in Bowditch Boundary of Relatively hyperbolic groups 2

    Understanding Swenson (large excerpt.. some diagrams .. some remarks). Please be cautious. Potentially wrong remarks lie ahead.

    Continuum

    A continuum is a compact connected Hausdorff space.

    continuum

    Cut Point

    In a continuum Z, \( c \in Z \) is a cut point if \( Z = A \cup B \) where A and B are non-singleton continua and \( A \cap B = \{c\} \). If in addition \( D \subset A – \{c\} \) and \( E \subset B – \{ c \} \), we say that c separates D from E.

    cut point

    For the remainder of this section, Z will be a metric continuum, G will be a group (possibly trivial) of homeomorphisms of Z, and \( C \subset Z \) will be a G-equivariant (GC = C) set of cut points of Z.

    Is a member of (interval)

    For \( a, b \in Z \) and \( c \in C \), we define \( c \in (a, b) \) if there exist non-singleton continua A containing a and B containing b with \( A \cup B = Z \) and \( A \cap B = \{ c \} \).

    Any point in an interval is a cut point by definition of interval.

    not an interval

    We define the closed and half open intervals in the obvious way i.e., \( [a, b] = \{a, b \} \cup (a, b) \), and \( [a, b) = \{a\} \cup (a, b) \) for \( a \neq b \) ( \([a, a) = \phi \) )

    Notice that if \( c \in (a, b) \) then for any subcontinuum \( Y \subset Z \) from a to b (\(a, b \in Y\) ), \( c \in Y \). Why? Suppose Y is a subcontinuum containing a and b. \( c \in (a, b) \) implies there are continua A and B such that \( a \in A, b \in B, A \cup B = Z, A \cap B = \{ c \} \).

    \( A \cap Y \) and \(B \cap Y \) compact and Hausdorff (hence are subcontinua) containing a and b respectively. Their union is Y (as all y in Y are either in A or B as A union B is Z and Y is contained in Z). Their intersection is either \( \phi \) or {c}.

    confusion

    Equivalence of points

    For \( a, b \in Z – C \) we say that a is equivalent to b, a ~ b, if \( (a, b) = \phi \). That is there is no cut point between a and b.For \( c \in C \), c is equivalent only to itself. This is clearly an equivalence relation, so let P bet the set of equivalence classes of Z. We will abuse notation and say \( C \subset P \) since each element of C is its own equivalence class.

    Observe that for \( a, b, d\in Z \) if a ~ b, then (a, d) = (b, d). We can therefore translate the interval relation on Z to P and we also enlarge it as follows.

    Membership in P (interval in P)

    For \( x, y, z \in P \), we say \( y \in (x, z) \) if either

    1. \( y \in C\) where \( y \in (a, b) \) for some \( a, b \in Z \) with \( a \in x \) and \( b \in z \) (note that x, and z are equivalence classes ) or
    2. \( y \notin C and if \( a, b, d \in Z \) with \( a\in x , b \in Y \) and \( d \in z \), then \( [a, b) \cup (b, d] = \phi \)
    interval in P - first kind
    interval in P – first kind
    interval in P – second kind

    Since C was chosen to be G invariant, the action of G on Z gives an action of G on P which preserves the interval structure ( we have not given P a topology so it doesn’t make sense to ask if the action is by homeomorphism).

  • Dunwoody’s Accessibility Theorem – Day 2

    Suppose G is a finitely presented group. Let us fix \( \mathcal{A} \) – a favorite class of subgroups of G (closed under taking subgroups and conjugation).

    If G acts on an \(\mathcal{A} \) – tree T, we have a graph of groups decomposition for G.

    If H < G then H acts on T and we have graph of groups decomposition for H.

    Definitions

    1. H acts elliptically on T means the splitting of G does not split H (or H is contained in a vertex stabilizer).
    2. H is universally elliptic if it acts elliptically on all \( \mathcal{A} \) – trees. Example: Groups with property FA (Finite Groups).
    3. An \( \mathcal {A} \) – tree is universally elliptic, if its edges stabilizers are elliptic in every \(\mathcal {A} \) – tree
    4. T dominates T’ means there exists a G-equivariant map from T to T’. This further implies that if some subgroup H is not split by T then H is not split by T’.
    5. A JSJ decomposition (or JSJ tree) of G over  is an  – tree such that:
      1. T is universally elliptic (its edge stabilizers are elliptic in every  \(\mathcal {A} \) – tree or fixes a point in every  \(\mathcal {A} \) – tree \)
      2. T dominates any other universally elliptic tree T’ (the vertex stabilizers are as small as possible; they are elliptic in every universally elliptic tree).
      3. Example: If  \(\mathcal {A} \) only contains the trivial group, JSJ trees are same as Grushko trees.

    Motivation from JSJ Decomposition of compact 3 manifold

    William Jaco, Peter Shalen, and Klaus Johannson (1979) proved the following:

    Irreducible orientable closed (i.e., compact and without boundary) 3-manifolds have a unique (up to isotopy) minimal collection of disjointly embedded incompressible tori such that each component of the 3-manifold obtained by cutting along the tori is either atoroidal or Seifert-fibered.

    Comparing JSJ decomposition of groups and manifold

    Graph of groups decomposition of G over \( \mathcal{A} \).

    Graph of groups for H < G

    H acts elliptically on T

    H is universally elliptic

    JSJ decomposition of a 3 manifold by cutting along embedded family of tori

    H ‘cut’ by the family of tori.

    Tori can be pushed off of H

    H is not cut by any embedded torus

    Goal

    We wish to show that for every sequence of graph of groups decomposition of a finitely presented group G, over a favored class of subgroups \( \mathcal {A} \), there exists a JSJ decomposition that dominates all decompositions eventually.

  • Cut points in Bowditch Boundary of Relatively hyperbolic groups 1

    This document is a personal musing. It has many excerpts without credit, potentially false claims, and misquotes. If some cosmic accident has lead you to this page, then take a deep breath and assume caution. If you are worried about copyright infringement, kindly let me know. I will modify the document.

    B.H. Bowditch thought about cut points in the boundary of relatively hyperbolic groups. His comments in the page 64 of the following monologue is particularly interesting.

    Bowditch says that if the boundary of a relatively hyperbolic group is connected then each of its global cut points is a parabolic fixed point.

    “For this one need to place certain mild restrictions on the class of groups that can occur as maximal parabolic groups. (It is sufficient to assume that they are one or two-ended, finitely presented, and not infinite torsion groups. Probably only the last of these assumptions is really important.)”

    Do we really need all three of these conditions? That is, do the maximal parabolic subgroups need to be

    • one or two ended
    • finitely presented
    • not infinite torsion group (Bowditch thinks only this one is really important)

    In the same monologue he refers to Swenson’s paper which has an ‘alternative route’.

    Bestvina’s paper hints at a route that may get rid of these extra conditions.

    There are three components of his thought:

    1. relatively hyperbolic group
    2. boundary of a group
    3. cut points

    We will try to explore each of these ideas.

  • A survey of relative Dunwoody’s accessibility theorem

    Motivation

    This is not (even remotely) an original work. For example it contains large excerpts from a variety of papers (often without reference).

    More importantly beware! What follows may contain outrageously false statements. This was created for an in-class presentation while the author was exploring these ideas for the first time..

    Consider a group G (finitely generated). We are interested to ‘split’ the group into simpler pieces. In this direction we have the following result:

    Grushko Decomposition Theorem

    Any non trivial finitely generated group G can be decomposed as a free product \( G = G_1 * G_2 * \cdots * G_r * F_s, r, s \geq 0 \) where each of the groups \( G_i \) is non trivial, freely indecomposable (that is it cannot be decomposed as a free product) and not infinite cyclic, and where \( F_s \) is a free group of rank s.

    For a given G, the groups G1, …, Gr are unique up to a permutation of their conjugacy classes in G (and, in particular, the sequence of isomorphism types of these groups is unique up to a permutation) and the numbers s and r are unique as well.

    More precisely, if G = B1∗…∗BkFt is another such decomposition then k = rs = t, and there exists a permutation σ∈Sr such that for each i=1,…,r the subgroups Gi and Bσ(iare conjugate in G.

    This gives a decomposition of the group G as the fundamental group of a graph of groups,  or equivalently actions of G on a simplicial  tree T (Grushko Tree) with trivial edge  stabilizers.

    Maximality of Grushko Trees

    Since the \(G_i\)’s are freely indecomposable, Grushko trees \(T_0 \) have the following maximality property: if T is any tree on which G acts with trivial edge stabilizers, \( G_i \) fixes a point in T, and therefore \(T_0 \) dominates T, in the sense that there is a G – equivariant map \( T_0 \to T \). In other words, among free decompositions of G, a Grushko tree \(T_0 \) is as far as possible from the trivial tree (a point): its vertex stabilizers are as small as possible (they are conjugates of the \(G_i\)’s ).

    This maximality property does not determine \(T_0 \) uniquely, as it is shared by all Grushko trees.

    Next level of generalization

    We want to consider more general decompositions. In Grushko decomposition, the edge stabilizers (of corresponding Grushko Trees) are trivial. What if we wanted the edge stabilizers to be cyclic? What if they were finite?

    Toward this end, we first choose our favorite class of edge stabilizers and call it \( \mathcal{A} \). For example \( \mathcal{A} \) could be the class of cyclic subgroups or the class of virtually cyclic subgroups or the class of finite subgroups and so on.

    Suppose \( \mathcal{A} \) is closed under taking subgroups and conjugation. We investigate the action of G on all trees whose edge stabilizers are from \( \mathcal {A} \).

    These trees are known as \( \mathcal{A} \) – trees.

    Question

    Is it possible to find a tree with a maximality property as in the case of Grushko trees? That is, is it possible to find an \( \mathcal{A} \) tree on which G acts such that the vertex stabilizers are as small as possible? More explicitly speaking, is it possible to split the vertex groups finitely many times and terminate the process?

    Dunwoody’s inaccessible group

    The answer to the above question, for finitely generated groups, is negative. Even if we demand the edge stabilizers to be finite, there exists groups which do not yield to such maximal decompositions.

    Suppose G be a finitely generated group. \( \mathcal{A} \) = {finite subgroups of G}.

    A finitely generated group G is said to be accessible if it is the fundamental group of a graph of groups in which all edge groups are finite (from \( \mathcal{A} \) ) and every vertex group has at most one end.

    Stallings Theorem showed that a group G has more than one end if and only if G ≍ A*FB, where F is finite, A ≠ F ≠ B, or G is an HNN-extension with finite edge group F. Hence if we can find a graph of groups in which every vertex group has at most one end then, these vertex groups won’t split any more over finite groups.

    We say that G is inaccessible if it is not accessible.

    M.J. Dunwoody (1993) constructed a finitely generated group that is inaccessible

    .

    Next best hope: finitely presented groups

    Suppose G is a finitely presented group. \( \mathcal {A} \) be the class of cyclic groups (closed under taking subgroups and conjugation). We may hope that such a group has a maximal splitting over cyclic subgroups.

    Consider the following example: \( G = \mathbb{Z} * B \) where B is non-empty, indecomposable, finitely presented group. Then we have

    \( G = \mathbb{Z} * B = \mathbb{Z} *_{2\mathbb{Z}} <2\mathbb{Z}, B> \)

    But this can be split further. For example, we have

    \( G = \mathbb{Z} *_{2\mathbb{Z}} {2\mathbb{Z}}*_{4\mathbb{Z}} <4\mathbb{Z}, B> \)

    Hence we have found a finitely presented group, which has a graph of groups decomposition over cyclic groups that does not terminate.

    But all hope is not lost. In a sense \( G = \mathbb{Z} * B \) dominates all other decompositions that we have created. That is vertex stabilizers of \( G = \mathbb{Z} * B \) are stabilize vertices in the subsequent splittings

    In fact, what actually happens is this: for finitely presented groups, we will be able to find a universally elliptic \( \mathcal {A} \) -tree that will dominate all other universally elliptic \( \mathcal {A} \) -trees. That is, though we may get non-terminating splittings, there will exist one that will dominate all of them eventually.

    Motivation from manifold topology

    William Jaco, Peter Shalen, and Klaus Johannson (1979) proved the following:

    Irreducible orientable closed (i.e., compact and without boundary) 3-manifolds have a unique (up to isotopy) minimal collection of disjointly embedded incompressible tori such that each component of the 3-manifold obtained by cutting along the tori is either atoroidal or Seifert-fibered.

    “Differentiable manifolds can always be given the structure of PL manifolds, which can be triangulated into simplicial complexes. By shrinking a spanning tree of the 1-skeleton of this simplicial complex, we can obtain a CW complex ? with a single 0-cell. This complex is no longer a manifold, but has the same fundamental group as the original manifold, since quotienting out by a contractible subspace is a homotopy equivalence.

    If the manifold is compact, it has a simplicial decomposition with a finite number of cells. This carries over to ?. But the fundamental group of a ?? complex with a single 0-cell has a presentation with a generator for each 1-cell and a relation for each 2-cell. Thus ?, and therefore the original manifold, has a finitely presented fundamental group.”

    This idea motivates search for ‘a’ maximal splitting of the (finitely) group over favorite subgroups.

    JSJ Decomposition

    A JSJ decomposition (or JSJ tree) of G over \( \mathcal {A} \) is an \( \mathcal{A} \) – tree such that:

    1. T is universally elliptic (its edge stabilizers are elliptic in every \( \mathcal{A} \) – tree or fixes a point in every \( \mathcal {A} \) – tree \)
    2. T dominates any other universally elliptic tree T’ (the vertex stabilizers are as small as possible; they are elliptic in every universally elliptic tree).

    If \( \mathcal {A} \) only contains the trivial group, JSJ trees are same as Grushko trees.

    What if \( \mathcal {A} \) is something else? Cyclic, Abelian, Slender etc. Dunwoody’s accessibility theorem concludes that a finitely presented group has JSJ decompositions over any class \( \mathcal{A} \) of subgroups.

    Theorem: Let \( \mathcal {A} \) be an arbitrary family of subgroups of G, stable under taking subgroups and under conjugation. If G is finitely presented, it has a JSJ decomposition over \( \mathcal {A} \). In fact there exists a JSJ tree whose edge and vertex stabilizers are finitely generated.

    Dunwoody’s accessibility theorem is a consequence of this (general) existence theorem.

    Dunwoody’s Accessibility Theorem

    G is finitely presented. There exist a graph of groups decomposition of G such that all edge groups are finite and all vertex groups are finite or one-ended.

    Lemma

    Let G be finitely presented relative to \( \mathcal{H} = \{ H_1, H_2 , \cdots , H_p \} \). Assume that \( T_1 \leftarrow \cdots \leftarrow T_k \leftarrow T_{k+1} \leftarrow \cdots \) is a sequence of refinements of \( (\mathcal {A, H} ) \) trees. There exists an \( (\mathcal {A, H} ) \) – tree S such that:

    1. for k large enough, there is a morphism \( S \to T_k \);
    2. each edge stabilizer of S is finitely generated.

    Morsels of the statement

    • Relatively finitely presented: G is relatively finitely presented relative to its subgroups \( H_1 , \cdots , H_p \) if there exists a finite subset \( \Omega \subset G \) such that the natural morphism \( F ( \Omega ) * H_1 * \cdots * H_p \to G \) is onto and its kernel is normally generated by a finite subset \( \mathcal{R} \)
    • \( (\mathcal {A, H} ) \) trees
    • Equivariant Maps: A map \( f: T \to T’ \) is said to be G-equivariant if \( f (g \cdot x ) = g \cdot f(x) \).
    • Maps between trees will always be G – equivariant, send vertices to vertices, and edges to edge-paths (may be a point)
    • Morphism: A map \( f : T \to T’ \) between two trees is a morphism if an only if one can subdivide T so that f maps each edge onto an edge; equivalently, no edge of T is collapsed to a point. Folds are examples of morphism. (Fig. 1)
    Examples of morphism
    Fig 1: Example of Morphism
    • Collapse Map: A collapse map \( f : T \to T’ \) between two trees is a map obtained by collapsing certain edges to points followed by an isomorphism (by equivariance, the set of collapsed edges is G-invariant). Equivalently f preserves alignment: the image of any arc [a, b] is a point or the arc [f(a), f(b)]. (Fig. 2)
    • Refinements (of trees): A tree T’ is a collapse of T if there is a collapse map \( T \to T’ \); conversely, we say that T refines T’.
    Collapse Map, Refinement
    Fig 2: Example of Collapse map, refinement

    And the big picture

    Why do we care about refinements?

    Action of a group on a tree is a description of the group in simpler terms or a splitting of the group. In figure 2, \( G_1, L_1, H_1, I_1 \) and edges connecting them maps to the vertex \( N_1 \) in tree T’.

    Since the collapse map is G-equivariant this implies if g stabilizes \(G_1 \) then \( N_1 = f(G_1) = f( g \cdot G_1 ) = g \cdot f(G_1) = g \cdot N_1 \) or g stabilizes \(N_1 \). In other words, stabilizers of \( G_1, L_1, H_1, I_1 \) and the edges connecting them are contained in stabilizer of \(N_1 \).

    The vertex group \( G_{N_1} \) is the fundamental group of the graph of groups \( \Gamma_{N_1} \) in red, occurring as the preimage of \(N_1\).

    Why do we want the edge stabilizers of S to be finitely generated?

    Proof

    Make the 2-complex, universal cover, and fix the lifts of elliptic portions, and vertices of remaining parts.

    1. Construct a connected simplicial 2-complex X such that \( \pi_1 (X) = G \)
      1. \( (Y_i, u_i) \) be a pointed 2-complex with \( \pi_1 (Y_i, u_i) = H_i \)
      2. Starting from the disjoint union of the \( Y_i’s \), add p edges joining the \( u_i \) ‘s to an additional vertex u.
      3. Add # \( \Omega \) additional edges joining u to itself.
      4. Represent each element of \( \mathcal {R} \) by a loop in this space, and glue a disc along this loop to obtain the desired space X.
      5. I wonder if it helps to build the Eilenberg Maclane complex
    2. X has a universal cover \(\pi : X \to \tilde {X} \)
    3. G acts on \( \tilde {X} \) by deck transformation.
    4. For \( i \in \{1, \cdots , p \} \) consider a connected component \( \tilde {Y}_i \) of \( \pi^{-1} (Y_i) \), whose stabilizer is \( H_i \).
    5. Fix lifts \( v_1 , \cdots , v_q \in \tilde {X} \) of all the vertices in X \ \( Y_1 \cup \cdots \cup Y_p \) . (It is a finite simplicial complex. Hence it has finitely many vertices)

    Construct equivariant maps \( f_k : \tilde {X} \to T_k \) inductively.

    1. \( p_k : T_{k+1} \to T_k \) be the collapse map. By definition of collapse map the pre-image of the midpoint of an edge of \( T_k \) is a single point, namely the midpoint of the edge of \(T_{k+1} \) mapping onto \( e_k \)
    2. We demand \( f_k : \tilde {X} \to T_k \) to be G – equivariant, mapping \( \tilde {Y}_i \) to a vertex fixed by \( H_i \), sends each \(v_j \) to a vertex and sends each edge of \( \tilde {X} \) either to a point or injectively onto a segment in \(T_k \). We further require that \( p_k (f_{k+1} (x) ) = f_k (x) \) if x is a vertex of \( \tilde {X} \) or if \( f_k (x) \) is a midpoint of an edge in \( T_k \)
    f_k
    Fig 3: Construction of \(f_k \)

    Construction

    We start with \(T_0 \) a point, and \(f_0, p_0 \) the constant maps. We then assume that \( f_k : \tilde{X} \to T_k \) has been constructed and we construct \( f_{k+1} \).

    To define \( f_{k+1} \) in \( \tilde {Y}_i \) we note that \( f_k (\tilde {Y}_i) \) is a vertex of \(T_k \) fixed by \(H_i \). Since \(p_k \) preserves alignment, \( p_k^{-1} (f_k (\tilde {Y}_i )) \) is an \( H_i \) invariant subtree. Since \( H_i \) is elliptic in \( T_{k+1} \), it fixes some vertex 0f this subtree, and we map \( \tilde {Y}_i \) to such a vertex.

    (confusion: why should that vertex be contained in that subtree) 

    We then define \( f_{k+1} (v_j ) \) as any vertex in \( p_k^{-1} (f_k (v_j) ) \), and we extend by equivariance.

    (Recall that \( v_j \) were the chosen lifts of vertices of X. For example a vertex u in X may be lifted to \( v_{u_1} , v_{u_2}, \cdots \). If we chose \( v_{u_1} \) as the favorite lift then \( v_{u_i} = g_i \cdot v_{u_1} \). Since we fixed \( f_{k+1} (v_{u_1} ) \) then we define \( f_{k+1} (v_{u_i} ) = g_i \cdot f_{k+1} (v_{u_1} ) \) )

    Notice that we finished defining \( f_{k+1} \) on all vertices of \( \tilde {X} \) . 

    Now consider an edge e of X not contained in any \( Y_i \), and a lift \( \tilde {e} \subset \tilde{X} \). The map \( f_{k+1} \) is already defined on the endpoints of \( \tilde {e} \).

    The restriction of \( p_k \) to the segment of \( T_{k+1} \) joining the images of the endpoints of \( \tilde {e} \) is a collapse map. In particular, the preimage of the midpoint of an edge \( e_k \) of \( T_k \) is the midpoint of the edge of \( T_{k+1} \) mapping onto \( e_k \)

    \(f_k \) is constant or injective on \( \tilde {e} \), this allows us to define \( f_{k+1} \) on \( \tilde {e} \) as a map which is either constant or injective and satisfies \( p_k ( f_{k+1} (x) = f_k (x) \) if \( f_k(x) \) is the midpoint of an edge of \( T_k \)

    Doing this equivariantly we have now defined \( f_{k+1} \) on the 1- skeleton of \( \tilde {X} \)

    We then extend \( f_{k+1} \) in a standard way to every triangle abc not contained in \( \pi ^{-1} (Y_i ) \); in particular, if \( f_{k+1} \) is not constant on abc, preimages of the midpoints of the edges in \(T_{k+1} \) are straight arcs joining two distinct sides.

    Tracks of Dunwoody
    Fig 4: Extension to 2-skeleton

    Pattern of Dunwoody, its dual tree

    1. Define \( \tilde {\tau}_k \subset \tilde{X} \) as the preimage (under \( f_k \) of the midpoints of all edges of \( T_k \). This is a pattern in the sense of Dunwoody
    2. \( \tilde {\tau}_k \) does not intersect any \( \tilde {Y}_i \)
    3. \( \tilde{\tau}_k \subset \tilde {\tau}_{k+1} \)
    4. \( \tau_k = \pi ( \tilde{\tau}_k ) \) be the projection of in X. It is a finite graph as it is contained in the complement of \( Y_1 \cup \cdots \cup Y_p \).
    5. \( S_k \) be the tree dual to the pattern \( \tilde{\tau}_k \)

    Claim 1: \(S_k \) is an \( (\mathcal {A, H} ) \) tree.

    Proof: Each edge in \( S_k \) is ‘cut’ by a unique track which corresponds to a midpoint of an edge in \( T_k \). This defines a map from \( S_k \to T_k \). Hence edge stabilizers of \( S_k \) are in edge stabilizers of \( T_k \) implying \(S_k \) is \( \mathcal {A} \) tree.

    Every \( H_i \) is elliptic in \( S_k \) because \( \tilde {Y}_i \) does not intersect \( \tilde{\tau}_k \).

    Fig 5: Tree dual to the pattern

    Claim 2: \( S_k \) has finitely generated edge stabilizers.

    Proof: (Forwarded by Professor Hruska, explained by Arka Banerjee)

    Let A be a subcomplex of B. Consider the universal cover \( \tilde{B} \). Each component of the preimage of A in the universal cover is a cover of A corresponding to the subgroup \( N = ker (\pi_1(A) \to \pi_1(B) ) \)

    Why? Some loops in A may shrink to the basepoint in B but not in A. These loops are precisely the members of N (apart from the trivial loop that shrinks both in A and in B). Pre-images of the homotopy classes of these loops (under the covering projection in the cover) are distinct homotopy classes of loops in a connected component of the pre-image of A. Hence N is the fundamental group of each connected component.

    Such a component is called an “elevation” of A to the cover. (It’s not the same thing as a “lift” of A.)

    Why? After all, a lift will include A in the universal cover of its super space. These components are covers of A and is possibly larger than A

    The deck transformations that stabilize the elevation of A would be
    \( im ( \pi_1(A) \to \pi_1(B) ) = \pi_1(A) / N \)

    Why? The elements in \( im ( \pi_1(A) \to \pi_1(B) ) \) are the homotopy classes of loops in A which do  not shrink to basepoint in A and in B (except the trivial one). These are precisely all those group elements that keep members of elevations of A in elevations of A.

    (The fundamental group of the base space acts on the universal cover by deck transformations. The action is determined as follows. Take a base point \(x_0 \in X \) and a pre-image \( \tilde{x}_0 \) of \(x_0 \) in the universal cover \( \tilde {X} \). Then each element of \( \pi_1 (X, x_0) \) is represented by a loop f : I → X based at \( x_0 \). There is a unique lift \( \tilde{f} : I → \tilde{X} \) starting at \( \tilde{x}_0 \). Then we define the action of the homotopy class [f] on \(\tilde{x}_0 \) by \( [f] (\tilde{x}_0 = \tilde {f}(1) \). The quotient under this group action is the base space.)

    If A is a finite graph, it is clear that any quotient of \( \pi_1(A) \) is finitely generated.

    Why? Fundamental group of a finite graph is generated by the finite number of edges (of that graph sans the maximal tree in it). Hence it is finitely generated. Finally quotient of finitely generated group is finitely generated. The quotient group is generated by the images of the generators of G under the canonical projection.

    Number of non-parallel tracks are bounded

    Let \( X’ \subset X \) be the closure of the complement of \( Y_1 \cup \cdots \cup Y_p \). By construction this is a finite complex.

    Theorem [Dun85, Theorem 2.2]

    There is a bound on the number of non-parallel tracks in X’.

    This implies that there exists \( k_0 \) such that for all \( k \geq k_0 \), for every connected component \( \sigma \) of \( \tau_k \) \ \( \tau_{k_0} \), there exists a connected component \( \sigma’\) of \( \tau_{k_0} \) such that \( \sigma \cup \sigma’\) bounds a product region containing no vertex of X’.

    It follows that, for \( k \geq k_0 \), one can obtain \( S_k \) from \( S_{k_0} \) by subdividing edges. We then take \( S = S_{k_0} \)

    Proof of Dunwoody bounded track theorem:

    Morsels of the Statement

    Tracks: Let L be a connected 2-dimensional complex. A track is a subset S of |L| with the following properties.

    • S is connected
    • For each two simplex \(\sigma \) of |L|, \( S \cap | \sigma | \) is a union of finitely many disjoint straight lines
    Fig 6: Finitely many (2) tracks in MOP
    • If \( \gamma \) is a 1-complex of L and \( \gamma \) is not a face of a 2-complex, then either \( S \cap | \gamma | = \phi \) or S consists of a single point in the interior of \( | \gamma | \) . This implies S is 1 point set.

    If |L| is a 2-manifold then S is a connected 1 dimensional submanifold.

    Band: A band is a subset of B of |L| with the following properties.

    • B is connected
    • For each 2-complex \( \sigma \) 0f L, \( B \cap | \sigma | \) is a union of finitely many components each of which is bounded by two closed intervals in distinct faces of \( \sigma \) and the disjoint lines joining the endpoints of these intervals.
    • If \( \gamma \) is a 1-complex of L, which is not a face of 2-complex, then either \( B \cap | \gamma | = \phi \) or B consists of a subset of \( | \gamma | \) bounded by two points in the interior of \( | \gamma | \)

    If B is a band then we get a track \( t(B) \) by choosing the midpoint of each component of \( | \gamma | \cap B \) for every 1-simplex \( \gamma \) of L and joining these points in the appropriate components of \( | \sigma | \cap B \) where \( \sigma \) is a 2-complex of L.

    Untwisted Band: B is untwisted if B is homeomorphic to \( t(B) \times [0, 1] \) in which case \( \partial B \) has two components each homeomorphic to t(B).

    Twisted Band: If B is not untwisted then it is twisted. In this case \( \partial B \) is a track which double covers t(B).

    Twisted and Untwisted tracks: If S is a track then S is called twisted (untwisted) if there is a twisted (untwisted) band B such that t(B) = S.

    Fig 7: Twisted tracks and bands

    Parallel Tracks: Two tracks \( S_1 \) and \( S_2 \) are parallel if there is an untwisted band B such that \( \partial B = S_1 \cup S_2 \)

    1-cochains with \( \mathbb{Z}_2 \) coefficients: Let S be a track in the connected 2-dimensional complex L. If \( \gamma \) is a 1-simplex of L, 1-cochain \( z(S) (\gamma\) = k \mod 2 \) where k = # \( (|\gamma| \cap S) \). That is the number of times S intersects \(\gamma \)  modulo 2. (Is it hitting \(\gamma \)  even or odd times ?)

    If \( \sigma \) is a 2-simplex then \( \partial \sigma \cap \S \) has an even number of points.

    If AB, BC and CA are the sides of a triangle and S hits AB and BC, then every time it hits AB, it will also hit BC. In this particular case z(S) (AB) – z(S) (BC) + z(CA) is even or 0 mod 2. Hence it z(S) is a map which goes to 0 under \( \delta \) or difference function.

    Hence z(S) is a 1-cocycle.

    Claim 1: z(S) is a coboundary (an image of the differential) if and only if S separates |L|, i.e. |L| – S has two components.

    Notice that z(S) is a 1-cochain. Can it be regarded as a map obtained by taking difference of the value assigned to the vertices? That is, if \( \phi : \Delta^0 \to \mathbb{Z}_2 \), then is \( \delta \phi = z(S) \) ?

    This is possible if and only if S splits L into two components.

    Fig 8: Track leading to co-boundary.

    Claim 2: A twisted track cannot separate L.

    Proof: Follow the track along from side of the track long enough to reach the other side as there is only one side per se.

    Hence if S is twisted, z(S) is not a coboundary. Hence it is a non-trivial element of \( H^1 (L; \mathbb{Z}_2 ) \). Why? Notice that z(S) is a cocycle (as shown earlier). Hence it is in kernel. \( H^1 (L; \mathbb{Z}_2 ) \) is formed by quotienting out the coboundaries from the kernel. Is S is twisted, z(S) is not coboundary (but nevertheless a cocycle). Hence it is not quotiented out. Hence it represents a non trivial element of \( H^1 (L; \mathbb{Z}_2 ) \) .

    In fact no non empty union of disjoint twisted tracks separates |L|. Hence the corresponding elements of \( H^1 (L; \mathbb{Z}_2 ) \) are linearly independent.

    Theorem

    Suppose \( \beta = \textrm{rank} H^1 (L; \mathbb{Z}_2 ) \) is finite. Let \( T = \{ t_1, \cdots , t_n \} \) be a set of disjoint tracks. Then \( |L| – \cup t_i \) has at least \( n – \beta \) components, The set T contains at most \( \beta \) twisted tracks.

    Proof: Let M be the subgroup of \( H^1 (L; \mathbb{Z}_2 ) \) generated by the elements corresponding to \( z(t_1), z(t_2), \cdots , z(t_n) \). Consider the epimorphism $$ \theta : \underbrace{ \mathbb{Z}_2 \oplus \mathbb{Z}_2 \oplus \cdots \oplus \mathbb{Z}_2}_\text{n copies } \to M $$. We can think of this epimorphism as a ‘string picker’. For example (1, 0, 0 , … 0) is mapped to \(z(t_1) \) etc.

    Kernel of this epimorphism are elements mapping to the identity element of \( H^1 (L; \mathbb{Z}_2 ) \); that is the coboundary maps. Basis elements of this kernel corresponds to the number of untwisted tracks. Since untwisted (disjoint) tracks splits \( |L| – \cup t_i \) into components, hence the basis elements of the kernel corresponds to the components of \( |L| – \cup t_i \)

    The proposition follows. There are atmost \( \beta \) twisted, disjoint, tracks. In T, therefore there are at least n – \( \beta \) untwisted disjoint tracks. Which leads to \( n – \beta \) components of \( L – \cup t_i \)

    Suppose now that L is finite. Let

    \( v_L \) = number of vertices of L

    \(f_L \) = number of 2 simplexes of L

    and n(L) = \( 2 \beta + v_L + f_L \)

    Theorem

    Suppose \( t_1 , t_2 , \cdots , t_k \) are disjoint tracks in |L|. If \( k > n(L) \), then there exists \( i \neq j \) such that \( t_i \) and \( t_j \) are parallel.

    Proof: If \( \sigma \) is a 2-simplex of L and D is the closure of a component of \( |\sigma| – \cup t_i \) then D is a disc. We say that D is good if \( \partial D \cap \partial |\sigma| \) consists of two components in distinct faces of \( \sigma \)

    Fig 9: only one ‘not good’ disc D without a vertex

    For any \( \sigma \) there are at most three D’s which contain a vertex of \( \sigma \) and at most one other component which is not good.

    If \( k > n(L) \) then \( |L| – \cup t_i \) has more than \( 2 \beta + v_L + f_L – \beta \) = \( \beta + v_L + f_L \) components.

    Confusion: It follows that there are at least \( \beta + 1\) components whose closures are bands.

    Since |L| contains at mosts \( \beta \) disjoint twisted bands, there is at least one component whose closure is an untwisted band. The theorem follows immediately.

    Lemma (3.2 – Levitt)

    Assume that all groups in \( \mathcal {A} \) are universally elliptic. If T is a JSJ tree, then the vertex stabilizers are universally elliptic.

    Morsels of the proof

    As mentioned above, Grushko trees have a strong maximality property: their vertex stabilizers are elliptic in any free splitting of G. This does not hold any longer when one considers JSJ decompositions over infinite groups, in particular cyclic groups: a vertex stabilizer \(G_v \) of a JSJ tree may fail to be elliptic in some splitting (over the chosen family A).
    If this happens, we say that the vertex stabilizer \(G_v \) (or the corresponding vertex v, or the vertex group of the quotient graph of groups) is flexible. The other stabilizers (which are elliptic in every splitting over A) are called rigid. In particular, all vertices of Grushko trees are rigid (because their stabilizers are freely indecomposable). On the other hand, in the example of G = π1(Σ), the unique vertex stabilizer \(G_v = G \) is flexible.

    Proof:

    Suppose vertex stabilizer \( G_v \) is flexible (fails to be elliptic in some splitting). Consider T’ such that \( G_v \) is not elliptic in T.

    Since T is a JSJ decomposition, it is universally elliptic (its edges stabilizers fixes a point in every \( \mathcal{A} \) tree). So one can consider a standard refinement \( \hat{T} \) of T dominating T’.

    By our assumption on \( \mathcal{A} \), the tree \( \hat {T} \) is universally elliptic. So by definition of the JSJ deformation space T dominates \( \hat {T} \). This implies \( G_v \) is elliptic in \( \hat{T} \), hence in T’, a contradiction.

    Corollary (4.14 – Levitt)

    Let \( G_v \) be a vertex stabilizer of a JSJ tree \( T_J \).

    1. \( G_v \) does not split over a universally elliptic subgroup relative to \( Inc^{\mathcal{H}}_v \)
    2. \( G_v \) is flexible if it splits relative to \( Inc^{\mathcal{H}}_v \), rigid other wise.

    Morsels of Theorem

    Let T be a tree (minimal, relative to \( \mathcal {H} \) with edge stabilizers in \( \mathcal{A} \). Let \( v \) be a vertex with stabilizer \( G_v \).

    Incident edge groups \( Inc_v \)

    Given a vertex v of a tree T, there are finitely many \( G_v \) orbits of edges with origin v. We choose representatives \( e_i \) and we define \( Inc_v \) (or \( Inc_{G_v} \) as the family of stabilizers \( G_{e_i}\). We call \( Inc_v \), the set of incident edge groups. It is a family of subgroups of \( G_v \), each well defined up to conjugacy.

    Proof:

    If there is a splitting as in (1), we may use it to refine \(T_J \) to a universally elliptic tree. (see Lemma 4.12 Levitt). This tree must be in the same deformation space as \(T_J \), so the splitting of \(G_v \) must be trivial.

    (2) follows from Lemma 4.13 Levitt applied with \( H = G_v \)

    (Lemma 4.12 Levitt)

    Let \(G_v \) be a vertex stabilizer of an \( ( \mathcal {A, H} ) \) tree T. Any splitting of \(G_v\) relative to \( Inc^{\mathcal{H}}_v \) extends (non-uniquely) t0 a splitting of G relative to \( \mathcal {H} \).

    More precisely, given an \( (\mathcal{A}_v Inc^{\mathcal{H}}_v )\) tree \(S_v \), there exist an \( ( \mathcal {A, H} ) \) tree \( \hat {T} \) and a collapse map \( p: \hat{T} \to T \) such that \( p^{-1} (v) \) is \(G_v \) – equivariantly isomorphic to \(S_v\)

    We say that \( \hat{T} \) is obtainedby refining T at v using \( S_v \). More generally, one may choose a splitting for each orbit of vertices of T, and refine T using them. Any refinement of T may be obtained by this construction (possibly with non minimal trees \( S_v \) ).

    Proof:

  • Accessibility

    G is a finitely presented group.

    X is its presentation complex (a simplicial 2-complex). Since G is finitely presented, the number of vertices of X is finite. Suppose \( u_1 , \cdots , u_q \) be the vertices of X.

    \( \tilde {X} \) be its universal cover.

    Fix lifts of the vertices of X. Suppose they are \( v_1 , \cdots , v_q \).

    Choose \( \mathcal {A} \) : a preferred set of subgroups of G, stable under conjugation and taking subgroups. We will be working with trees, whose edge stabilizers come from\( \mathcal {A} \)

    Let \( T_1 \leftarrow \cdots  \leftarrow T_{k+1} \leftarrow T_{k} \leftarrow \cdots \) be refinements of \( \mathcal {A} \) -trees.

    This means there is a collapse map from \( T_{k+1} \to T_k \) for each k.

    Collapse Map

    A collapse map (is a G-equivariant map) that maps some edges to vertices. On the remaining tree, it is a graph isomorphism.

    Pre-image of midpoint of every edge \(e \) of \( T_k \) is the midpoint of an edge e’ in \( T_{k+1} \) that maps isomorphically onto e.

    We will construct equivariant maps \( f_k \) from \( \tilde {X} \) to \( T_k \) for all k inductively. 

    Here is the recipe:

    • Map the (favorite) vertices \( v_i \) of \( \tilde {X} \) to vertices of \( T_1 \). 
    • Extend equivariantly to all vertices of \( \tilde {X} \). The map is now defined on 0- skeleton.
      That is if \( v_i \to f_1 (v_i) \) then \( gv_i \to f_1 (gv_i) = g f(v_i)  \) 
    • In order to extend the map to 1-skeleton, first note that we know where the endpoints of each edge are going. 
    • \( \tilde {e} \) be an edge of \( \tilde {X} \). Let v, w be its endpoints. Since \( T_1 \) is a tree, there is an unique edge path connecting \( f_1 (v) \) to \( f_1 (w) \) 
    • Map \( \tilde {e} \) to that path. 
    • For \( T_2 \), first send v to any vertex \( t_v \)  in the set \( p_1^{-1} ( f_1 (v) ) \). Similarly w is mapped to any vertex \(t_w \)  in \( p_1^{-1} (f_1 (w) ) \) 
    • Restrict \( p_1 \) to the segment \( t_v t_w \). It is a collapse map. 
    • In particular, the pre-image of the midpoint of an edge \( e_k \) of \( T_k \) is the midpoint of the edge of \(T_{k+1}\) mapping onto \( e_k \). 
    • Since \( f_1 \) is constant or injective on \( \tilde {e}\) this allows us to define \( f_{2} \) on \( \tilde {e}\) as a map which is either constant or injective.
    • Extend \( f_{2} \) equivariantly on the 1-skeleton.
    • Finally, we will extend \( f_2 \) to the two simplices. Whenever it is not constant, the image is tripod. Pre-images of midpoints of edges of  \(T_2\) are straight arcs joining two sides of the triangle. 

    Pattern of Dunwoody

    The pre-images of midpoints of \( T_k \) is \( \tilde {\tau_k } \subset \tilde {X} \)

     

    Dunwoody Pattern

    Also note that \( \tilde {\tau_k} \subset \tilde {\tau_{k+1}} \) 

    We will project the Dunwoody pattern to X (the presentation complex we started off with). This is a finite graph. 

    \( S_k \) be the tree dual to the pattern \( \tilde {\tau_k} \in \tilde {X} \). There is a natural induced map that sends \( S_k \to T_k \), sending edge to edge. Hence edge stabilizers of \( S_k \) are in \( \mathcal{A} \). 

    Edge Stabilizers of \( S_k \) are finitely generated

  • The Alexander Trick

    Here is the original paper:

    J. W. Alexander, On the deformation of an n-cell

    (A 2-page paper that influenced a remarkable amount of later work).

  • Ends

    Motivation


    Start with a locally finite simplicial complex X.

    Locally finite: Each vertex is attached to only finitely many simplices.

    Why locally finite: To make sure it is a CW complex. Notice that the closure-finite criteria require each cell of a CW complex to meet only finitely many other cells.

    Hence we do not have a situation like this:

    Screen Shot 2018-03-07 at 6.40.14 AM

    Suppose K is any finite subcomplex of X.

    We are interested in the number of infinite connected components of X – K. Call that number n(K).

    Example: 

    Screen Shot 2018-03-07 at 6.45.26 AM

    Consider the Real line (with usual triangulation). If we remove one vertex (shown in the picture), then n(I) = 2 (as there are two open rays or two infinite connected components).

    From \[\mathbb{R}^n, n \ge 2 \] onward, if you remove a finite subcomplex K, that can be enclosed within a (large enough) closed ball. Hence there can only one infinite connected component of \[\mathbb{R}^n – K , n \ge 2 \]

    This number n(K) can be different for different K.  Take for example the infinite binary tree.

    binary

    Removing the top vertex, the number of infinite connected components are 2. But removing up to level 2, we will have 4 infinite connected components. And as we go down the levels, n(K) will grow.

    So, we try with all possible such finite subcomplexes (possibly infinitely many of them) and check each time how many infinite connected components of X – K is there.

    This is precisely what leads us to ends of X.

    Ends of (X) =  E(X) = sup n(K)

    Example: \[E(\mathbb{R}) = 2, E(\mathbb{R^2}) = 1, E(T) = \infty, \textrm{T = infinite binary tree} \]

    Star of K: If K is a (finite) subcomplex of a simplicial complex X, then st(K) or star of K is defined to be the interior of all simplices which meet the vertices in K.

    Since K is locally finite st(K) is an open finite subset of K.

    If two point \[v_1, v_2 \] in X – st(K) can be connected by a path in X – st(K) then they can be connected via an edge path in X – st(K). Hence they are in a path component of X – K. Hence it is sufficient to look into the 1-skeleton of X – K to find out n(K).

    Cohomology 


    Recall that given a simplicial complex, one can create Chain complexes and Co-Chain Complexes.

    A chain complex, \[C_0 (X) \] of vertices is simply the set of formal sums of vertices in X. In other words, if \[v_1, v_2, v_3 \] are vertices in X then \[v_1 + v_2 – v_3 \] is an element of \[C_0 (X) \]. In fact it has all such finite formal sums.

    Once the chain complex is defined, one may quickly define co-chain complexes. They are formal sums of homomorphisms from \[C_0(X) \to G \] where G is a suitable group. Usually \[G = \mathbb{Z}_2, \textrm {or} G = \mathbb{Z} \]. It depends on what we are trying to achieve.

    One may think of each member of 0th cochain complex as an assignment of values to each vertex in X.

    Screen Shot 2018-03-07 at 7.14.56 AM

    In the above picture, we have assigned 0’s and 1’s to each vertex of the finite simplicial complex. This is one member of \[C^0(X) \]. Each such assignment is nothing but a function from \[C_0(X) \to \mathbb{Z}_2 \].

    We collect all such functions and their formal sum. They constitute \[C^0(X) \].

    In the present context, we may think of \[\mathbb{Z}_2 \] as {off, on}. Whenever we pick a finite subcomplex K in the simplicial complex X, we are indirectly assigning 1 to each vertex in K and 0 to all the vertices in X – K. That assignment is indeed a function from the set of vertices to {0, 1} hence a member of the cochain complex.

    Formally we say that the function has finite support; that is it is non-zero at only finitely many points and zero everywhere else.

    Thus the member of \[C^0(X) \] which have finite support, are our algebraic tools for ‘picking’ finite subcomplexes K from simplicial complex X. In fact, each such cochain corresponds to one such ‘pick’.

    Let \[C_f^0 (X) \] denote the subset of \[C^0 (X) \] with finite support.

    Notice that similarly we can define \[C_f^1 (X) \]. They are maps from (formal sums of) edges of X to \[\mathbb{Z}_2 \] which have 1 assigned to finitely many edges (and 0 elsewhere).

    \[C_f^0 (X) \] maps inside \[C_f^1 (X) \] under the coboundary map.

    Why? Suppose \[\phi \in C_f^0 (X) \] . Then \[\delta \phi (v_1, v_2) = \phi (v_2) – \phi (v_1) \] (Recall that the coboundary map assigns ‘difference’ of values at the vertices. This can be intuited as a change in height function: value at each edge is the difference of height at its vertices).

    Clearly \[\phi (v_2) – \phi (v_1) \] can be non zero if and only if one of them is 0 and the other one is 1. But as \[\phi \in C_f^0(X) \] has finite support, it gives nonzero output only at finitely many vertices hence \[\phi (v_2) – \phi (v_1) \] can be non zero only at finitely many edges.

    ‘Ends’ is the dimension of Cohomology


    Recall that cohomology groups of a space X are the homology groups of Cochain Complex.

    In more simpler terms, consider the following Cochain complex:

    \[… \overset{\delta_2} \Leftarrow C^1(X) \overset{\delta_1} \Leftarrow C^0(X) \overset{\delta_0} \Leftarrow 0 \]

    Then \[H^0 (X) = \frac{ker (\delta_1)}{im (\delta_0)} = ker (\delta_1) \]

    Intuition: Image of the lower level difference map contains lower level ‘difference’ data. By quotienting that out, we may focus only on higher level differences.

    We previously constructed \[C_f^0 (X) \] that singled out the finite subcomplexes. (K’s). Next, we wish to turn our attention toward X – K. Hence it makes sense to ‘quotient out’ \[C_f^0 (X) \] from \[C^0 (X) \]. Then we will be left out with those functions which assign 1 to infinitely many vertices.

    Define \[C_e^0 (X) = \frac{C^0 (X)}{C_f^0 (X)}  \]

    Similarly define \[C_e^1 (X) = \frac{C^1 (X)}{C_f^1 (X)}  \]

    Intuition: Imagine as ends. Functions in \[C_e^0 (X) \] flow 1’s upto ends (as 1’s appear infinitely many times at the vertices).

    Claim: \[dim_{\mathbb{Z}_2} H_e^0 (X) = E(X)  \]

    It is not hard to see why this could be true. Afterall what is $latex H_e^0 (X) $ ? It is the collection of all those \[\phi \in C_e^0 (X) \] that maps to 0 of $latex C_e^1 (X) $.

    More explicitly, these are 0-1assignments on vertices, which have 1 at infinitely many vertices, but non-zero differences at finitely many edges.

    Example: 

    Screen Shot 2018-03-07 at 8.27.28 AM

    Again consider the real line. Assign 1 at all vertices leftward from U. Assign 0 W onward (to the right).

    Note that this is a member of (an equivalence class of) \[C^0_e (X) \] as it has 1 at infinitely many vertices. Call it \[\phi \] .

    But after applying the coboundary map \[\delta \] to \[\phi \], we get 0 at all edges except on UV.  Clearly \[\delta \phi \] has finite support, hence is a member of \[C^1_f (X) \]. Therefore it is in the equivalence class of 0 in \[C^1_e (X) \] (as we have quotiented out all edge-functions with finite support).

    Note that U and V are the crossover points in the above example. When we talk about the \[ker \delta_1 \], we are seeking vertex-functions in \[C^0_e (X) \] we have finitely many crossover points (but infinitely many points with 1 assigned).

    Why? Because if we cut at the crossover, we have an infinite component at least at one side of it (after all the infinitely many 1’s need to accommodated somewhere).

    The recipe for finding the finite crossover but infinitely flowing vertex functions:

    • Look at all vertex-functions that map to edge-functions with finite support (\[\delta^{-1} {C^1_f(X) } \])
    • Quotient out those which are 1 (on) at finitely many vertices (they do not flow to the ends)
    • Final result \[\frac{\delta^{-1} {C^1_f(X) }}{C^0_f(X)} \]

    The rest is easy! 

    Each path component of X – K must bear the same value at each vertex. Hence we can create linearly independent vertex functions corresponding to each component of X – K.

    But we have taken care of all possible K as we considered all cochains.

    Hence the number of linearly independent finite crossover but infinitely flowing vertex maps provide the Ends of X.

    Good News: This data is cohomological. Hence it is independent of the triangulation of the space. (It is a deep theorem of algebraic topology that cohomology groups are independent of triangulation; infact can be achieved without triangulation).

  • Which manifold is this?

    This is the first exercise from Thurston’s Three Dimensional Geometry and Topology Vol. 1.

    Which manifold is this?

    It is like an old trick. Try following the lines. There are actually 6 loops (circles) in this maze.

    Here is a color coded picture of it.

  • Round robin tournament

    Round robin tournament

    Problem : Suppose there are \[ {k}\] teams playing a round robin tournament; that is, each team plays against all the other teams and no game ends in a draw.Suppose the \[ {i^{th}}\] team loses \[ {l_{i}}\] games and wins \[ {w_{i}}\] games.Show that

    \[ {{\displaystyle}{\sum_{i=1}^{k}{l_i^{2}}}}\] = \[ {{\displaystyle}{\sum_{i=1}^{k}{w_i^{2}}}}\]

    Solution : Each team plays exactly one match against each other team.

    Consider the expression \[ \displaystyle{\sum_{i=1}^{k} l_i^{2} – {w_i^2} = \sum_{i=1}^{k}(l_i + w_i)(l_i – w_i) } \]

    Since each team plays exactly k-1 matches and no match ends in a draw, hence number of wins plus numbers of loses of a particular team is k-1 (that is the number of matches it has played). In other words \[ l_i + w_i = k-1 \] for all i (from 1 to k).

    Hence

    \[ \displaystyle{\sum_{i=1}^{k} l_i^{2} – {w_i^2} } \]
    \[ \displaystyle{= \sum_{i=1}^{k}(l_i + w_i)(l_i – w_i) } \]
    \[ \displaystyle{= \sum_{i=1}^{k}(k-1)(l_i – w_i) } \]
    \[ \displaystyle{= (k-1)\left( \sum_{i=1}^{k} l_i – \sum_{i=1}^{k} w_i\right) } \]

    But \[ \displaystyle{ \sum_{i=1}^{k} l_i = \sum_{i=1}^{k} w_i } \] (as total number of loses = total number of matches = total number of wins; as each match results in a win or lose of some one)

    Hence \[ \displaystyle{= (k-1)\left( \sum_{i=1}^{k} l_i – \sum_{i=1}^{k} w_i\right) = (k-1) \times 0 = 0 } \]

    Therefore \[ \displaystyle{\sum_{i=1}^{k} l_i^{2} – {w_i^2} = 0 } \] implying \[ {{\displaystyle}{\sum_{i=1}^{k}{l_i^{2}}}}\] = \[ {{\displaystyle}{\sum_{i=1}^{k}{w_i^{2}}}}\]

    Proved.

  • Orthogonality

    Orthogonality

    Let ABC be a triangle and D be the midpoint of BC. Suppose the angle bisector of \[\angle ADC \] is tangent to the circumcircle of triangle ABD at D. Prove that \[\angle A = 90^o \] .

    (Regional Mathematics Olympiad, India, 2016)

    (more…)