Bioflux System for Cellular Interactions Microfluidic Flow System for Live Cell Assays
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The Matrix Calculus You Need for Deep Learning
The Matrix Calculus You Need For Deep Learning Terence Parr and Jeremy Howard July 3, 2018 (We teach in University of San Francisco's MS in Data Science program and have other nefarious projects underway. You might know Terence as the creator of the ANTLR parser generator. For more material, see Jeremy's fast.ai courses and University of San Francisco's Data Institute in- person version of the deep learning course.) HTML version (The PDF and HTML were generated from markup using bookish) Abstract This paper is an attempt to explain all the matrix calculus you need in order to understand the training of deep neural networks. We assume no math knowledge beyond what you learned in calculus 1, and provide links to help you refresh the necessary math where needed. Note that you do not need to understand this material before you start learning to train and use deep learning in practice; rather, this material is for those who are already familiar with the basics of neural networks, and wish to deepen their understanding of the underlying math. Don't worry if you get stuck at some point along the way|just go back and reread the previous section, and try writing down and working through some examples. And if you're still stuck, we're happy to answer your questions in the Theory category at forums.fast.ai. Note: There is a reference section at the end of the paper summarizing all the key matrix calculus rules and terminology discussed here. arXiv:1802.01528v3 [cs.LG] 2 Jul 2018 1 Contents 1 Introduction 3 2 Review: Scalar derivative rules4 3 Introduction to vector calculus and partial derivatives5 4 Matrix calculus 6 4.1 Generalization of the Jacobian . -
A Brief Tour of Vector Calculus
A BRIEF TOUR OF VECTOR CALCULUS A. HAVENS Contents 0 Prelude ii 1 Directional Derivatives, the Gradient and the Del Operator 1 1.1 Conceptual Review: Directional Derivatives and the Gradient........... 1 1.2 The Gradient as a Vector Field............................ 5 1.3 The Gradient Flow and Critical Points ....................... 10 1.4 The Del Operator and the Gradient in Other Coordinates*............ 17 1.5 Problems........................................ 21 2 Vector Fields in Low Dimensions 26 2 3 2.1 General Vector Fields in Domains of R and R . 26 2.2 Flows and Integral Curves .............................. 31 2.3 Conservative Vector Fields and Potentials...................... 32 2.4 Vector Fields from Frames*.............................. 37 2.5 Divergence, Curl, Jacobians, and the Laplacian................... 41 2.6 Parametrized Surfaces and Coordinate Vector Fields*............... 48 2.7 Tangent Vectors, Normal Vectors, and Orientations*................ 52 2.8 Problems........................................ 58 3 Line Integrals 66 3.1 Defining Scalar Line Integrals............................. 66 3.2 Line Integrals in Vector Fields ............................ 75 3.3 Work in a Force Field................................. 78 3.4 The Fundamental Theorem of Line Integrals .................... 79 3.5 Motion in Conservative Force Fields Conserves Energy .............. 81 3.6 Path Independence and Corollaries of the Fundamental Theorem......... 82 3.7 Green's Theorem.................................... 84 3.8 Problems........................................ 89 4 Surface Integrals, Flux, and Fundamental Theorems 93 4.1 Surface Integrals of Scalar Fields........................... 93 4.2 Flux........................................... 96 4.3 The Gradient, Divergence, and Curl Operators Via Limits* . 103 4.4 The Stokes-Kelvin Theorem..............................108 4.5 The Divergence Theorem ...............................112 4.6 Problems........................................114 List of Figures 117 i 11/14/19 Multivariate Calculus: Vector Calculus Havens 0. -
Policy Gradient
Lecture 7: Policy Gradient Lecture 7: Policy Gradient David Silver Lecture 7: Policy Gradient Outline 1 Introduction 2 Finite Difference Policy Gradient 3 Monte-Carlo Policy Gradient 4 Actor-Critic Policy Gradient Lecture 7: Policy Gradient Introduction Policy-Based Reinforcement Learning In the last lecture we approximated the value or action-value function using parameters θ, V (s) V π(s) θ ≈ Q (s; a) Qπ(s; a) θ ≈ A policy was generated directly from the value function e.g. using -greedy In this lecture we will directly parametrise the policy πθ(s; a) = P [a s; θ] j We will focus again on model-free reinforcement learning Lecture 7: Policy Gradient Introduction Value-Based and Policy-Based RL Value Based Learnt Value Function Implicit policy Value Function Policy (e.g. -greedy) Policy Based Value-Based Actor Policy-Based No Value Function Critic Learnt Policy Actor-Critic Learnt Value Function Learnt Policy Lecture 7: Policy Gradient Introduction Advantages of Policy-Based RL Advantages: Better convergence properties Effective in high-dimensional or continuous action spaces Can learn stochastic policies Disadvantages: Typically converge to a local rather than global optimum Evaluating a policy is typically inefficient and high variance Lecture 7: Policy Gradient Introduction Rock-Paper-Scissors Example Example: Rock-Paper-Scissors Two-player game of rock-paper-scissors Scissors beats paper Rock beats scissors Paper beats rock Consider policies for iterated rock-paper-scissors A deterministic policy is easily exploited A uniform random policy -
The Infinite and Contradiction: a History of Mathematical Physics By
The infinite and contradiction: A history of mathematical physics by dialectical approach Ichiro Ueki January 18, 2021 Abstract The following hypothesis is proposed: \In mathematics, the contradiction involved in the de- velopment of human knowledge is included in the form of the infinite.” To prove this hypothesis, the author tries to find what sorts of the infinite in mathematics were used to represent the con- tradictions involved in some revolutions in mathematical physics, and concludes \the contradiction involved in mathematical description of motion was represented with the infinite within recursive (computable) set level by early Newtonian mechanics; and then the contradiction to describe discon- tinuous phenomena with continuous functions and contradictions about \ether" were represented with the infinite higher than the recursive set level, namely of arithmetical set level in second or- der arithmetic (ordinary mathematics), by mechanics of continuous bodies and field theory; and subsequently the contradiction appeared in macroscopic physics applied to microscopic phenomena were represented with the further higher infinite in third or higher order arithmetic (set-theoretic mathematics), by quantum mechanics". 1 Introduction Contradictions found in set theory from the end of the 19th century to the beginning of the 20th, gave a shock called \a crisis of mathematics" to the world of mathematicians. One of the contradictions was reported by B. Russel: \Let w be the class [set]1 of all classes which are not members of themselves. Then whatever class x may be, 'x is a w' is equivalent to 'x is not an x'. Hence, giving to x the value w, 'w is a w' is equivalent to 'w is not a w'."[52] Russel described the crisis in 1959: I was led to this contradiction by Cantor's proof that there is no greatest cardinal number. -
High Order Gradient, Curl and Divergence Conforming Spaces, with an Application to NURBS-Based Isogeometric Analysis
High order gradient, curl and divergence conforming spaces, with an application to compatible NURBS-based IsoGeometric Analysis R.R. Hiemstraa, R.H.M. Huijsmansa, M.I.Gerritsmab aDepartment of Marine Technology, Mekelweg 2, 2628CD Delft bDepartment of Aerospace Technology, Kluyverweg 2, 2629HT Delft Abstract Conservation laws, in for example, electromagnetism, solid and fluid mechanics, allow an exact discrete representation in terms of line, surface and volume integrals. We develop high order interpolants, from any basis that is a partition of unity, that satisfy these integral relations exactly, at cell level. The resulting gradient, curl and divergence conforming spaces have the propertythat the conservationlaws become completely independent of the basis functions. This means that the conservation laws are exactly satisfied even on curved meshes. As an example, we develop high ordergradient, curl and divergence conforming spaces from NURBS - non uniform rational B-splines - and thereby generalize the compatible spaces of B-splines developed in [1]. We give several examples of 2D Stokes flow calculations which result, amongst others, in a point wise divergence free velocity field. Keywords: Compatible numerical methods, Mixed methods, NURBS, IsoGeometric Analyis Be careful of the naive view that a physical law is a mathematical relation between previously defined quantities. The situation is, rather, that a certain mathematical structure represents a given physical structure. Burke [2] 1. Introduction In deriving mathematical models for physical theories, we frequently start with analysis on finite dimensional geometric objects, like a control volume and its bounding surfaces. We assign global, ’measurable’, quantities to these different geometric objects and set up balance statements. -
1 Space Curves and Tangent Lines 2 Gradients and Tangent Planes
CLASS NOTES for CHAPTER 4, Nonlinear Programming 1 Space Curves and Tangent Lines Recall that space curves are de¯ned by a set of parametric equations, x1(t) 2 x2(t) 3 r(t) = . 6 . 7 6 7 6 xn(t) 7 4 5 In Calc III, we might have written this a little di®erently, ~r(t) =< x(t); y(t); z(t) > but here we want to use n dimensions rather than two or three dimensions. The derivative and antiderivative of r with respect to t is done component- wise, x10 (t) x1(t) dt 2 x20 (t) 3 2 R x2(t) dt 3 r(t) = . ; R(t) = . 6 . 7 6 R . 7 6 7 6 7 6 xn0 (t) 7 6 xn(t) dt 7 4 5 4 5 And the local linear approximation to r(t) is alsoRdone componentwise. The tangent line (in n dimensions) can be written easily- the derivative at t = a is the direction of the curve, so the tangent line is given by: x1(a) x10 (a) 2 x2(a) 3 2 x20 (a) 3 L(t) = . + t . 6 . 7 6 . 7 6 7 6 7 6 xn(a) 7 6 xn0 (a) 7 4 5 4 5 In Class Exercise: Use Maple to plot the curve r(t) = [cos(t); sin(t); t]T ¼ and its tangent line at t = 2 . 2 Gradients and Tangent Planes Let f : Rn R. In this case, we can write: ! y = f(x1; x2; x3; : : : ; xn) 1 Note that any function that we wish to optimize must be of this form- It would not make sense to ¯nd the maximum of a function like a space curve; n dimensional coordinates are not well-ordered like the real line- so the fol- lowing statement would be meaningless: (3; 5) > (1; 2). -
Or, If the Sine Functions Be Eliminated by Means of (11)
52 BINOMIAL THEOREM AND NEWTONS MONUMENT. [Nov., or, if the sine functions be eliminated by means of (11), e <*i : <** : <xz = X^ptptf : K(P*ptf : A3(Pi#*) . (53) While (52) does not enable us to construct the point of least attraction, it furnishes a solution of the converse problem : to determine the ratios of the masses of three points so as to make the sum of their attractions on a point P within their triangle a minimum. If, in (50), we put n = 2 and ax + a% = 1, and hence pt + p% = 1, this equation can be regarded as that of a curve whose ordinate s represents the sum of the attractions exerted by the points et and e2 on the foot of the ordinate. This curve approaches asymptotically the perpendiculars erected on the vector {ex — e2) at ex and e% ; and the point of minimum attraction corresponds to its lowest point. Similarly, in the case n = 3, the sum of the attractions exerted by the vertices of the triangle on any point within this triangle can be rep resented by the ordinate of a surface, erected at this point at right angles to the plane of the triangle. This suggestion may here suffice. 22. Concluding remark.—Further results concerning gen eralizations of the problem of the minimum sum of distances are reserved for a future communication. WAS THE BINOMIAL THEOEEM ENGKAVEN ON NEWTON'S MONUMENT? BY PKOFESSOR FLORIAN CAJORI. Moritz Cantor, in a recently published part of his admir able work, Vorlesungen über Gescliichte der Mathematik, speaks of the " Binomialreihe, welcher man 1727 bei Newtons Tode . -
Integrating Gradients
Integrating gradients 1 dimension The \gradient" of a function f(x) in one dimension (i.e., depending on only one variable) is just the derivative, f 0(x). We want to solve f 0(x) = k(x); (1) where k(x) is a known function. When we find a primitive function K(x) to k(x), the general form of f is K plus an arbitrary constant, f(x) = K(x) + C: (2) Example: With f 0(x) = 2=x we find f(x) = 2 ln x + C, where C is an undetermined constant. 2 dimensions We let the function depend on two variables, f(x; y). When the gradient rf is known, we have known functions k1 and k2 for the partial derivatives: @ f(x; y) = k (x; y); @x 1 @ f(x; y) = k (x; y): (3) @y 2 @f To solve this, we integrate one of them. To be specific, we here integrate @x over x. We find a primitive function with respect to x (thus keeping y constant) to k1 and call it k3. The general form of f will be k3 plus an arbitrary term whose x-derivative is zero. In other words, f(x; y) = k3(x; y) + B(y); (4) where B(y) is an unknown function of y. We have made some progress, because we have replaced an unknown function of two variables with another unknown function depending only on one variable. @f The best way to come further is not to integrate @y over y. That would give us a second unknown function, D(x). -
Mean Value Theorem on Manifolds
MEAN VALUE THEOREMS ON MANIFOLDS Lei Ni Abstract We derive several mean value formulae on manifolds, generalizing the clas- sical one for harmonic functions on Euclidean spaces as well as the results of Schoen-Yau, Michael-Simon, etc, on curved Riemannian manifolds. For the heat equation a mean value theorem with respect to `heat spheres' is proved for heat equation with respect to evolving Riemannian metrics via a space-time consideration. Some new monotonicity formulae are derived. As applications of the new local monotonicity formulae, some local regularity theorems concerning Ricci flow are proved. 1. Introduction The mean value theorem for harmonic functions plays an central role in the theory of harmonic functions. In this article we discuss its generalization on manifolds and show how such generalizations lead to various monotonicity formulae. The main focuses of this article are the corresponding results for the parabolic equations, on which there have been many works, including [Fu, Wa, FG, GL1, E1], and the application of the new monotonicity formula to the study of Ricci flow. Let us start with the Watson's mean value formula [Wa] for the heat equation. Let U be a open subset of Rn (or a Riemannian manifold). Assume that u(x; t) is 2 a C solution to the heat equation in a parabolic region UT = U £ (0;T ). For any (x; t) de¯ne the `heat ball' by 8 9 jx¡yj2 < ¡ 4(t¡s) = e ¡n E(x; t; r) := (y; s) js · t; n ¸ r : : (4¼(t ¡ s)) 2 ; Then Z 1 jx ¡ yj2 u(x; t) = n u(y; s) 2 dy ds r E(x;t;r) 4(t ¡ s) for each E(x; t; r) ½ UT . -
Gradient Sparsification for Communication-Efficient Distributed
Gradient Sparsification for Communication-Efficient Distributed Optimization Jianqiao Wangni Jialei Wang University of Pennsylvania Two Sigma Investments Tencent AI Lab [email protected] [email protected] Ji Liu Tong Zhang University of Rochester Tencent AI Lab Tencent AI Lab [email protected] [email protected] Abstract Modern large-scale machine learning applications require stochastic optimization algorithms to be implemented on distributed computational architectures. A key bottleneck is the communication overhead for exchanging information such as stochastic gradients among different workers. In this paper, to reduce the communi- cation cost, we propose a convex optimization formulation to minimize the coding length of stochastic gradients. The key idea is to randomly drop out coordinates of the stochastic gradient vectors and amplify the remaining coordinates appropriately to ensure the sparsified gradient to be unbiased. To solve the optimal sparsification efficiently, a simple and fast algorithm is proposed for an approximate solution, with a theoretical guarantee for sparseness. Experiments on `2-regularized logistic regression, support vector machines and convolutional neural networks validate our sparsification approaches. 1 Introduction Scaling stochastic optimization algorithms [26, 24, 14, 11] to distributed computational architectures [10, 17, 33] or multicore systems [23, 9, 19, 22] is a crucial problem for large-scale machine learning. In the synchronous stochastic gradient method, each worker processes a random minibatch of its training data, and then the local updates are synchronized by making an All-Reduce step, which aggregates stochastic gradients from all workers, and taking a Broadcast step that transmits the updated parameter vector back to all workers. -
Divergence, Gradient and Curl Based on Lecture Notes by James
Divergence, gradient and curl Based on lecture notes by James McKernan One can formally define the gradient of a function 3 rf : R −! R; by the formal rule @f @f @f grad f = rf = ^{ +| ^ + k^ @x @y @z d Just like dx is an operator that can be applied to a function, the del operator is a vector operator given by @ @ @ @ @ @ r = ^{ +| ^ + k^ = ; ; @x @y @z @x @y @z Using the operator del we can define two other operations, this time on vector fields: Blackboard 1. Let A ⊂ R3 be an open subset and let F~ : A −! R3 be a vector field. The divergence of F~ is the scalar function, div F~ : A −! R; which is defined by the rule div F~ (x; y; z) = r · F~ (x; y; z) @f @f @f = ^{ +| ^ + k^ · (F (x; y; z);F (x; y; z);F (x; y; z)) @x @y @z 1 2 3 @F @F @F = 1 + 2 + 3 : @x @y @z The curl of F~ is the vector field 3 curl F~ : A −! R ; which is defined by the rule curl F~ (x; x; z) = r × F~ (x; y; z) ^{ |^ k^ = @ @ @ @x @y @z F1 F2 F3 @F @F @F @F @F @F = 3 − 2 ^{ − 3 − 1 |^+ 2 − 1 k:^ @y @z @x @z @x @y Note that the del operator makes sense for any n, not just n = 3. So we can define the gradient and the divergence in all dimensions. However curl only makes sense when n = 3. Blackboard 2. The vector field F~ : A −! R3 is called rotation free if the curl is zero, curl F~ = ~0, and it is called incompressible if the divergence is zero, div F~ = 0. -
3D Topological Quantum Computing
3D Topological Quantum Computing Torsten Asselmeyer-Maluga German Aerospace Center (DLR), Rosa-Luxemburg-Str. 2 10178 Berlin, Germany [email protected] July 20, 2021 Abstract In this paper we will present some ideas to use 3D topology for quan- tum computing extending ideas from a previous paper. Topological quan- tum computing used “knotted” quantum states of topological phases of matter, called anyons. But anyons are connected with surface topology. But surfaces have (usually) abelian fundamental groups and therefore one needs non-abelian anyons to use it for quantum computing. But usual materials are 3D objects which can admit more complicated topologies. Here, complements of knots do play a prominent role and are in principle the main parts to understand 3-manifold topology. For that purpose, we will construct a quantum system on the complements of a knot in the 3-sphere (see arXiv:2102.04452 for previous work). The whole system is designed as knotted superconductor where every crossing is a Josephson junction and the qubit is realized as flux qubit. We discuss the proper- ties of this systems in particular the fluxion quantization by using the A-polynomial of the knot. Furthermore we showed that 2-qubit opera- tions can be realized by linked (knotted) superconductors again coupled via a Josephson junction. 1 Introduction Quantum computing exploits quantum-mechanical phenomena such as super- position and entanglement to perform operations on data, which in many cases, arXiv:2107.08049v1 [quant-ph] 16 Jul 2021 are infeasible to do efficiently on classical computers. Topological quantum computing seeks to implement a more resilient qubit by utilizing non-Abelian forms of matter like non-abelian anyons to store quantum information.