Recent Progress in Coalescent Theory
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Applied Probability
ISSN 1050-5164 (print) ISSN 2168-8737 (online) THE ANNALS of APPLIED PROBABILITY AN OFFICIAL JOURNAL OF THE INSTITUTE OF MATHEMATICAL STATISTICS Articles Optimal control of branching diffusion processes: A finite horizon problem JULIEN CLAISSE 1 Change point detection in network models: Preferential attachment and long range dependence . SHANKAR BHAMIDI,JIMMY JIN AND ANDREW NOBEL 35 Ergodic theory for controlled Markov chains with stationary inputs YUE CHEN,ANA BUŠIC´ AND SEAN MEYN 79 Nash equilibria of threshold type for two-player nonzero-sum games of stopping TIZIANO DE ANGELIS,GIORGIO FERRARI AND JOHN MORIARTY 112 Local inhomogeneous circular law JOHANNES ALT,LÁSZLÓ ERDOS˝ AND TORBEN KRÜGER 148 Diffusion approximations for controlled weakly interacting large finite state systems withsimultaneousjumps.........AMARJIT BUDHIRAJA AND ERIC FRIEDLANDER 204 Duality and fixation in -Wright–Fisher processes with frequency-dependent selection ADRIÁN GONZÁLEZ CASANOVA AND DARIO SPANÒ 250 CombinatorialLévyprocesses.......................................HARRY CRANE 285 Eigenvalue versus perimeter in a shape theorem for self-interacting random walks MAREK BISKUP AND EVIATAR B. PROCACCIA 340 Volatility and arbitrage E. ROBERT FERNHOLZ,IOANNIS KARATZAS AND JOHANNES RUF 378 A Skorokhod map on measure-valued paths with applications to priority queues RAMI ATAR,ANUP BISWAS,HAYA KASPI AND KAV I TA RAMANAN 418 BSDEs with mean reflection . PHILIPPE BRIAND,ROMUALD ELIE AND YING HU 482 Limit theorems for integrated local empirical characteristic exponents from noisy high-frequency data with application to volatility and jump activity estimation JEAN JACOD AND VIKTOR TODOROV 511 Disorder and wetting transition: The pinned harmonic crystal indimensionthreeorlarger.....GIAMBATTISTA GIACOMIN AND HUBERT LACOIN 577 Law of large numbers for the largest component in a hyperbolic model ofcomplexnetworks..........NIKOLAOS FOUNTOULAKIS AND TOBIAS MÜLLER 607 Vol. -
Superprocesses and Mckean-Vlasov Equations with Creation of Mass
Sup erpro cesses and McKean-Vlasov equations with creation of mass L. Overb eck Department of Statistics, University of California, Berkeley, 367, Evans Hall Berkeley, CA 94720, y U.S.A. Abstract Weak solutions of McKean-Vlasov equations with creation of mass are given in terms of sup erpro cesses. The solutions can b e approxi- mated by a sequence of non-interacting sup erpro cesses or by the mean- eld of multityp e sup erpro cesses with mean- eld interaction. The lat- ter approximation is asso ciated with a propagation of chaos statement for weakly interacting multityp e sup erpro cesses. Running title: Sup erpro cesses and McKean-Vlasov equations . 1 Intro duction Sup erpro cesses are useful in solving nonlinear partial di erential equation of 1+ the typ e f = f , 2 0; 1], cf. [Dy]. Wenowchange the p oint of view and showhowtheyprovide sto chastic solutions of nonlinear partial di erential Supp orted byanFellowship of the Deutsche Forschungsgemeinschaft. y On leave from the Universitat Bonn, Institut fur Angewandte Mathematik, Wegelerstr. 6, 53115 Bonn, Germany. 1 equation of McKean-Vlasovtyp e, i.e. wewant to nd weak solutions of d d 2 X X @ @ @ + d x; + bx; : 1.1 = a x; t i t t t t t ij t @t @x @x @x i j i i=1 i;j =1 d Aweak solution = 2 C [0;T];MIR satis es s Z 2 t X X @ @ a f = f + f + d f + b f ds: s ij s t 0 i s s @x @x @x 0 i j i Equation 1.1 generalizes McKean-Vlasov equations of twodi erenttyp es. -
Collision Times of Random Walks and Applications to the Brownian
Collision times of random walks and applications to the Brownian web David Coupier1, Kumarjit Saha2, Anish Sarkar3, and Viet Chi Tran4 1Univ. de Valenciennes, CNRS 2Ashoka University 3Indian Statistical Institute, Delhi 4Univ. Lille, CNRS February 12, 2019 Abstract Convergence of directed forests, spanning on random subsets of lattices or on point processes, towards the Brownian web has made the subject of an abundant literature, a large part of which relies on a criterion proposed by Fontes, Isopi, Newman and Ravishankar (2004). One of their conver- gence condition, called (B2), states that the probability of the event that there exists three distinct paths for a time interval of length t(> 0), all starting within a segment of length ε, is of small order of ε. This condition is often verified by applying an FKG type correlation inequality together with a coalescing time tail estimate for two paths. For many models where paths have complex interactions, it is hard to establish FKG type inequalities. In this article, we show that for a non-crossing path model, with certain assumptions, a suitable upper bound on expected first col- lision time among three paths can be obtained directly using Lyapunov functions. This, in turn, provides an alternate verification of Condition (B2). We further show that in case of independent simple symmetric one dimensional random walks or in case of independent Brownian motions, the expected value can be computed explicitly. We apply this alternate method of verification of (B2) to several models in the basin of attraction of the Brownian web studied earlier in the literature ([22], [14], [11]). -
Science Fiction and Astronomy
Sci Fi Science Fiction and Astronomy Many science fiction books include subjects of astronomical interest. Here is a list of some that have been recommended to me or I’ve read. I expect that most are not in the University library but many are available in Kindle and other e-formats. At the top of my list is a URL to a much longer list by Andrew Fraknoi of the Astronomical Society of the Pacific. Each title in his list has a very brief summary indicating the kind of story it is. Andrew Fraknoi’s list (http://www.astrosociety.org/education/resources/scifi.html). Gregory Benford is a plasma physicist who has been rated by some as one of the finest observes and interpreters of science in modern fiction. Note: Timescape [Vista, ISBN 0575600500] In the Ocean of Night [Vista, ISBN 0575600357] Across the Sea of Suns [Vista, ISBN 0575600551] Great Sky River [Gallancy, ISBN 0575058315] Eater and over 2 dozen more available as e-books. Stephen Baxter Titan [Voyager, 1997, ISBN 0002254247] has been strongly recommended by New Scientist as a tense, near future, thriller you shouldn’t miss. David Brin has a PhD in astrophysics with which he brings real understanding of the Universe to his stories. The Crystal Spheres won an award. Fred Hoyle is probably the most famous astronomer to have written science fiction. The Back Cloud [Macmillan, ISBN 0333556011] is his classic, followed by A for Andromeda. Try also October the First is too late. Larry Niven’s stories include plenty of ideas inspired by modern astronomy. -
Semimartingale Properties of a Generalized Fractional Brownian Motion and Its Mixtures with Applications in finance
Semimartingale properties of a generalized fractional Brownian motion and its mixtures with applications in finance TOMOYUKI ICHIBA, GUODONG PANG, AND MURAD S. TAQQU ABSTRACT. We study the semimartingale properties for the generalized fractional Brownian motion (GFBM) introduced by Pang and Taqqu (2019) and discuss the applications of the GFBM and its mixtures to financial models, including stock price and rough volatility. The GFBM is self-similar and has non-stationary increments, whose Hurst index H 2 (0; 1) is determined by two parameters. We identify the region of these two parameter values where the GFBM is a semimartingale. Specifically, in one region resulting in H 2 (1=2; 1), it is in fact a process of finite variation and differentiable, and in another region also resulting in H 2 (1=2; 1) it is not a semimartingale. For regions resulting in H 2 (0; 1=2] except the Brownian motion case, the GFBM is also not a semimartingale. We also establish p-variation results of the GFBM, which are used to provide an alternative proof of the non-semimartingale property when H < 1=2. We then study the semimartingale properties of the mixed process made up of an independent Brownian motion and a GFBM with a Hurst parameter H 2 (1=2; 1), and derive the associated equivalent Brownian measure. We use the GFBM and its mixture with a BM to study financial asset models. The first application involves stock price models with long range dependence that generalize those using shot noise processes and FBMs. When the GFBM is a process of finite variation (resulting in H 2 (1=2; 1)), the mixed GFBM process as a stock price model is a Brownian motion with a random drift of finite variation. -
Lecture 19 Semimartingales
Lecture 19:Semimartingales 1 of 10 Course: Theory of Probability II Term: Spring 2015 Instructor: Gordan Zitkovic Lecture 19 Semimartingales Continuous local martingales While tailor-made for the L2-theory of stochastic integration, martin- 2,c gales in M0 do not constitute a large enough class to be ultimately useful in stochastic analysis. It turns out that even the class of all mar- tingales is too small. When we restrict ourselves to processes with continuous paths, a naturally stable family turns out to be the class of so-called local martingales. Definition 19.1 (Continuous local martingales). A continuous adapted stochastic process fMtgt2[0,¥) is called a continuous local martingale if there exists a sequence ftngn2N of stopping times such that 1. t1 ≤ t2 ≤ . and tn ! ¥, a.s., and tn 2. fMt gt2[0,¥) is a uniformly integrable martingale for each n 2 N. In that case, the sequence ftngn2N is called the localizing sequence for (or is said to reduce) fMtgt2[0,¥). The set of all continuous local loc,c martingales M with M0 = 0 is denoted by M0 . Remark 19.2. 1. There is a nice theory of local martingales which are not neces- sarily continuous (RCLL), but, in these notes, we will focus solely on the continuous case. In particular, a “martingale” or a “local martingale” will always be assumed to be continuous. 2. While we will only consider local martingales with M0 = 0 in these notes, this is assumption is not standard, so we don’t put it into the definition of a local martingale. tn 3. -
Coalescent Likelihood Methods
Coalescent Likelihood Methods Mary K. Kuhner Genome Sciences University of Washington Seattle WA Outline 1. Introduction to coalescent theory 2. Practical example 3. Genealogy samplers 4. Break 5. Survey of samplers 6. Evolutionary forces 7. Practical considerations Population genetics can help us to find answers We are interested in questions like { How big is this population? { Are these populations isolated? How common is migration? { How fast have they been growing or shrinking? { What is the recombination rate across this region? { Is this locus under selection? All of these questions require comparison of many individuals. Coalescent-based studies How many gray whales were there prior to whaling? When was the common ancestor of HIV lines in a Libyan hospital? Is the highland/lowland distinction in Andean ducks recent or ancient? Did humans wipe out the Beringian bison population? What proportion of HIV virions in a patient actually contribute to the breeding pool? What is the direction of gene flow between European rabbit populations? Basics: Wright-Fisher population model All individuals release many gametes and new individuals for the next generation are formed randomly from these. Wright-Fisher population model Population size N is constant through time. Each individual gets replaced every generation. Next generation is drawn randomly from a large gamete pool. Only genetic drift affects the allele frequencies. Other population models Other population models can often be equated to Wright-Fisher The N parameter becomes the effective -
Natural Selection and Coalescent Theory
Natural Selection and Coalescent Theory John Wakeley Harvard University INTRODUCTION The story of population genetics begins with the publication of Darwin’s Origin of Species and the tension which followed concerning the nature of inheritance. Today, workers in this field aim to understand the forces that produce and maintain genetic variation within and between species. For this we use the most direct kind of genetic data: DNA sequences, even entire genomes. Our “Great Obsession” with explaining genetic variation (Gillespie, 2004a) can be traced back to Darwin’s recognition that natural selection can occur only if individuals of a species vary, and this variation is heritable. Darwin might have been surprised that the importance of natural selection in shaping variation at the molecular level would be de-emphasized, beginning in the late 1960s, by scientists who readily accepted the fact and importance of his theory (Kimura, 1983). The motivation behind this chapter is the possible demise of this Neutral Theory of Molecular Evolution, which a growing number of population geneticists feel must follow recent observations of genetic variation within and between species. One hundred fifty years after the publication of the Origin, we are struggling to fully incorporate natural selection into the modern, genealogical models of population genetics. The main goal of this chapter is to present the mathematical models that have been used to describe the effects of positive selective sweeps on genetic variation, as mediated by gene genealogies, or coalescent trees. Background material, comprised of population genetic theory and simulation results, is provided in order to facilitate an understanding of these models. -
Population Genetics: Wright Fisher Model and Coalescent Process
POPULATION GENETICS: WRIGHT FISHER MODEL AND COALESCENT PROCESS by Hailong Cui and Wangshu Zhang Superviser: Prof. Quentin Berger A Final Project Report Presented In Partial Fulfillment of the Requirements for Math 505b April 2014 Acknowledgments We want to thank Prof. Quentin Berger for introducing to us the Wright Fisher model in the lecture, which inspired us to choose Population Genetics for our project topic. The resources Prof. Berger provided us have been excellent learning mate- rials and his feedback has helped us greatly to create this report. We also like to acknowledge that the research papers (in the reference) are integral parts of this process. They have motivated us to learn more about models beyond the class, and granted us confidence that these probabilistic models can actually be used for real applications. ii Contents Acknowledgments ii Abstract iv 1 Introduction to Population Genetics 1 2 Wright Fisher Model 2 2.1 Random drift . 2 2.2 Genealogy of the Wright Fisher model . 4 3 Coalescent Process 8 3.1 Kingman’s Approximation . 8 4 Applications 11 Reference List 12 iii Abstract In this project on Population Genetics, we aim to introduce models that lay the foundation to study more complicated models further. Specifically we will discuss Wright Fisher model as well as Coalescent process. The reason these are of our inter- est is not just the mathematical elegance of these models. With the availability of massive amount of sequencing data, we actually can use these models (or advanced models incorporating variable population size, mutation effect etc, which are how- ever out of the scope of this project) to solve and answer real questions in molecular biology. -
Fclts for the Quadratic Variation of a CTRW and for Certain Stochastic Integrals
FCLTs for the Quadratic Variation of a CTRW and for certain stochastic integrals No`eliaViles Cuadros (joint work with Enrico Scalas) Universitat de Barcelona Sevilla, 17 de Septiembre 2013 Damped harmonic oscillator subject to a random force The equation of motion is informally given by x¨(t) + γx_(t) + kx(t) = ξ(t); (1) where x(t) is the position of the oscillating particle with unit mass at time t, γ > 0 is the damping coefficient, k > 0 is the spring constant and ξ(t) represents white L´evynoise. I. M. Sokolov, Harmonic oscillator under L´evynoise: Unexpected properties in the phase space. Phys. Rev. E. Stat. Nonlin Soft Matter Phys 83, 041118 (2011). 2 of 27 The formal solution is Z t x(t) = F (t) + G(t − t0)ξ(t0)dt0; (2) −∞ where G(t) is the Green function for the homogeneous equation. The solution for the velocity component can be written as Z t 0 0 0 v(t) = Fv (t) + Gv (t − t )ξ(t )dt ; (3) −∞ d d where Fv (t) = dt F (t) and Gv (t) = dt G(t). 3 of 27 • Replace the white noise with a sequence of instantaneous shots of random amplitude at random times. • They can be expressed in terms of the formal derivative of compound renewal process, a random walk subordinated to a counting process called continuous-time random walk. A continuous time random walk (CTRW) is a pure jump process given by a sum of i.i.d. random jumps fYi gi2N separated by i.i.d. random waiting times (positive random variables) fJi gi2N. -
Science Fiction Stories with Good Astronomy & Physics
Science Fiction Stories with Good Astronomy & Physics: A Topical Index Compiled by Andrew Fraknoi (U. of San Francisco, Fromm Institute) Version 7 (2019) © copyright 2019 by Andrew Fraknoi. All rights reserved. Permission to use for any non-profit educational purpose, such as distribution in a classroom, is hereby granted. For any other use, please contact the author. (e-mail: fraknoi {at} fhda {dot} edu) This is a selective list of some short stories and novels that use reasonably accurate science and can be used for teaching or reinforcing astronomy or physics concepts. The titles of short stories are given in quotation marks; only short stories that have been published in book form or are available free on the Web are included. While one book source is given for each short story, note that some of the stories can be found in other collections as well. (See the Internet Speculative Fiction Database, cited at the end, for an easy way to find all the places a particular story has been published.) The author welcomes suggestions for additions to this list, especially if your favorite story with good science is left out. Gregory Benford Octavia Butler Geoff Landis J. Craig Wheeler TOPICS COVERED: Anti-matter Light & Radiation Solar System Archaeoastronomy Mars Space Flight Asteroids Mercury Space Travel Astronomers Meteorites Star Clusters Black Holes Moon Stars Comets Neptune Sun Cosmology Neutrinos Supernovae Dark Matter Neutron Stars Telescopes Exoplanets Physics, Particle Thermodynamics Galaxies Pluto Time Galaxy, The Quantum Mechanics Uranus Gravitational Lenses Quasars Venus Impacts Relativity, Special Interstellar Matter Saturn (and its Moons) Story Collections Jupiter (and its Moons) Science (in general) Life Elsewhere SETI Useful Websites 1 Anti-matter Davies, Paul Fireball. -
The Brownian Web
The Annals of Probability 2008, Vol. 36, No. 3, 1153–1208 DOI: 10.1214/07-AOP357 c Institute of Mathematical Statistics, 2008 THE BROWNIAN NET By Rongfeng Sun and Jan M. Swart1 TU Berlin and UTIA´ Prague The (standard) Brownian web is a collection of coalescing one- dimensional Brownian motions, starting from each point in space and time. It arises as the diffusive scaling limit of a collection of coalescing random walks. We show that it is possible to obtain a nontrivial limiting object if the random walks in addition branch with a small probability. We call the limiting object the Brownian net, and study some of its elementary properties. Contents 1. Introduction and main results....................... .....................1154 1.1. Arrow configurations and branching-coalescing random walks.......1154 1.2. Topology and convergence......................... .................1155 1.3. The Brownian web................................. ................1158 1.4. Characterization of the Brownian net using hopping . .............1159 1.5. The left-right Brownian web....................... .................1160 1.6. Characterization of the Brownian net using meshes . .............1161 1.7. The dual Brownian web............................. ...............1162 1.8. Dual characterization of the Brownian net........... ...............1164 1.9. The branching-coalescing point set ................ ................. 1164 1.10. The backbone................................... ...................1166 1.11. Discussion, applications and open problems . .................1167