Finite Element Implementation of Orbital-Free Density Functional Theory for Electronic Structure Calculations

Total Page:16

File Type:pdf, Size:1020Kb

Finite Element Implementation of Orbital-Free Density Functional Theory for Electronic Structure Calculations Finite Element Implementation of Orbital-Free Density Functional Theory for Electronic Structure Calculations Soumya Swayamjyoti Report/Preprint No. 12–I–02 Institute of Applied Mechanics (CE) · Micromechanics of Materials Group University of Stuttgart, 70550 Stuttgart, Pfaffenwaldring 7, Germany ⋄ ⋄ ⋄ ⋄ ⋄ ⋄ ⋄ ⋄·⋄·⋄·⋄ ⋄⋄ ⋄·⋄ ⋄ ⋄ ⋄ ⋄·⋄ ⋄⋄··⋄·⋄·⋄·⋄⋄·⋄··⋄⋄ ⋄⋄··⋄·⋄·⋄⋄·⋄··⋄⋄ ⋄··⋄⋄··⋄·⋄·⋄⋄··⋄⋄··⋄ ·⋄··⋄⋄··⋄·⋄·⋄·⋄·⋄·⋄·⋄·⋄·⋄··⋄ ·⋄⋄·⋄⋄·⋄⋄·⋄⋄·⋄⋄·⋄⋄·⋄⋄·⋄⋄·⋄ ·⋄··⋄··⋄··⋄··⋄··⋄··⋄··⋄··⋄ ·⋄ ·⋄⋄·⋄·⋄·⋄·⋄⋄·⋄ ·⋄ ·⋄ ·⋄⋄· ⋄··⋄·⋄·⋄·⋄ ·⋄ ·⋄⋄· ⋄··⋄·⋄·⋄·⋄⋄· · ⋄··⋄·⋄··⋄·⋄·⋄··⋄ · ··⋄·⋄···⋄··⋄··⋄·⋄·· ···⋄··⋄··⋄··⋄··⋄·· Contents 1. Acknowledgements. 2. Introduction. 3. Orbital-Free Density Functional Theory. 3.1. The Orbital-Free Density Functional Theory Framework. 3.2. The Variational Problem. 3.3. Finite Element Formulation. 4. Multi-dimensional Optimization Methods for Orbital-Free DFT. 4.1. Steepest Descent Method. 4.2. Conjugate Gradient Method. 4.3. Root-Finding Newton Method. 5. Numerical Implementation. 5.1. Mesh Generation. 5.2. Implementation with DUNE Numerics. 6. Numerical Examples. 6.1. Atoms. 6.2. Molecules. 6.3. Aluminium Clusters. 6.4. Computational Time. 7. Conclusion and Future Directions. A. Required Derivatives. A.1. Derivatives with respect to {ui}. A.2. Derivatives with respect to {φi}. Master Thesis supervised by Dipl.-Phys. V. Schauer & Jun.-Prof. Dr. C. Linder Stuttgart, April 2012 (modified Dec 2013) Acknowledgements 1 1. Acknowledgements First of all, I would like to thank Jun.-Prof. Christian Linder for giving me the opportunity to do my master thesis in his group. I thank him for his encouragement and support during this interesting study. Additionally, I would like to express my gratitute to him for his help and advice during a period of personal difficulties. I want to thank Dipl.-Phys Volker Schauer for his guidance and supervision of this thesis. I am thankful to him for his constant support and help. It was a great learning experience to work with him. I am grateful to him for his valuable suggestions. The discussions we had pertaining to this thesis and about physics in general motivated my interest in computational physics to a great extent. I would also like to thank him for his friendship during my studies in Stuttgart. I seize this opportunity to wish him the best in his future endeavors. Many thanks to Prof. Christian Miehe for his timely advice and institutional support. I would like to thank my PhD supervisors Dr. Peter M. Derlet and Prof. J¨org L¨offler for the confidence they reposed in my profile following my seminar at Paul Scherrer Institut and subsequent discussions. Thanks to our collaborators Prof. Vikram Gavini and his group (in particular, Mr. Phani Sudheer Motamarri) for useful inputs. Thanks to all my colleagues in the Micromechanics of Materials Group and the In- stitute of Applied Mechanics (Chair I) of University of Stuttgart for the cordial work atmosphere. I thank Prof. Christian Linder, Prof. Eugenio Onate and Prof. Pedro Diez for their help during my PhD applications. A strong reference by Prof. Christian Linder as my Master Thesis Supervisor, a reference letter of Outstanding Performance in the first semester in Barcelona by Prof. Eugenio Onate and support of my abilities by Prof. Pedro Diez as the coordinator of my master program helped me find a very good PhD position at Paul Scherrer Institut and ETH Zurich. It is also relevant to point out that I enjoyed Prof. Christian Linder’s interactive lectures on Atomistic Modeling of Materials very much during my Masters. I look upto Prof. Eugenio Onate for the pioneering research he has done in the field of computational mechanics and his active management of CIMNE Barcelona as its director and founder. I acknowledge Prof. Pedro Diez’s, Prof. Sergio Zlotnik’s and Mr. Gautam Ethiraj’s excellent coordination of the Erasmus Mundus Master Program in Computational Mechanics from Barcelona and Stuttgart. Thanks to Prof. Sergio Zlotnik for organizational support for hosting the next EMA General Assembly in Barcelona in June 2013. I gratefully acknowledge the contributions to the formative years of my scientific career of Prof. K. Swaminathan as my Bachelor Thesis Advisor and Prof. Lakshman Nandagiri as a mentor at my home university National Institute of Technology Karnataka, Surathkal. I thank Dr. Brijesh Eshpuniyani as one of the first persons to introduce me to research while interning with him at IIT Delhi and IIT Kanpur during two consecutive summers. Special mention to Mr. Gautam Ethiraj (Stuttgart) and Ms. Lelia Zielonka (Barcelona) for their help with administrative affairs during my studies in the Erasmus Mundus Master of Science in Computational Mechanics. I thank my teachers at University of Stuttgart and UPC Barcelona for helping me build up my knowledge base in computational me- Acknowledgements 2 chanics. Thanks to my colleague and my best friend in Europe Mr. Anuj Sharma for a very generous friendship in Stuttgart. I thank Mr. Rodolfo Fleury (Swansea) and Mr. Fabien Poulhaon (Nantes) for the good times in Barcelona. I wish Anuj, Rodolfo and Fabien (who are also my classmates in the Erasmus Mundus Master of Science in Computational Mechanics) the very best in their doctoral studies at TU Darmstadt, Oxford University and Ecole Centrale Nantes respectively. I thank my family in India for their unconditional love and support. I gratefully acknowledge the financial support of the European Commission. My stud- ies in Europe were funded by the prestigious Erasmus Mundus Scholarship (A grant of 42k EUR by the European Commission for two years of master studies). I thank the selection consortium comprising of CIMNE (International Center for Numerical Methods in Engineering, Barcelona), University of Stuttgart, Ecole Centrale Nantes and Swansea University. Introduction 3 2. Introduction At the fundamental level, ground state properties of materials depend only on elec- tron density and hence are obtainable from first principles. However, a complete ab-initio calculation by solving the Schrodinger equation is computationally ambitious for a wide range of length scales involved in material modeling and thus separation of scales become necessary. At the microscopic scale, one can aim at ab-initio electronic structure calcula- tions in the framework of approximate theories developed over the last decades, the most prominent being the density functional theory which was pioneered by [24] and [25]. In the Kohn-Sham Density Functional Theory (KSDFT) the kinetic energy is computed by solv- ing an eigenvalue problem involving the wave-functions or orbitals of a material system. The computational complexity associated with this calculation is high and thus limits the potential system size to a few hundred atoms. This has inspired interest in orbital-free ki- netic energy functionals. This form of density functional theory where the kinetic energy is modeled by orbital-free kinetic energy functionals is referred to as Orbital-Free Density Functional Theory (OFDFT). This theory has its roots in the Thomas-Fermi model which finds mention in the early papers of [39], [27], [26]. In the context of material science, the electronic structure of a material determines the behavior of the material at the macroscopic level, which is the length scale of interest for engineering applications. Processes that occur at a certain length scale govern the behaviour of the material at larger length scales. Hence, it becomes necessary to success- fully bridge scales that can couple quantum mechanical, molecular mechanical or classical atomistic and continuum mechanics simulations in a unified theory. A feature of these multiscale simulations is to use accurate and computationally complex techniques to treat regions of small length scale and “coarse-grain” the rest of the system, that is, use less accurate and computationally faster methods for the rest of the system. In the atomistic framework, each atom is tracked during a deformation process and this information is used for predicting the macroscopic properties. While such resolution gives the exact description of a material, the computational demand associated with large system sizes makes most problems intractable in a completely atomistic framework. This is where the quasi-continuum (QC) methods come into play. Extensively discussed in [38], [42] and [16], QC methods aims at the right balance between fully atomistic and fully continuum techniques. They involve an adaptive use of both methodologies, that is, retaining the atomistic resolution in spatial regions of the problem only where required and use of continuum appoximations elsewhere to reduce the computational expense. Initially, the QC method was limited to atomistic interactions at the highest resolution. But it turns out that, a complete material description depends on the electronic structure, in particular, to predict material phenomenon such as bond breaking at the crack tip during failure in solids. To put the present work in context, we have implemented numerical methods to compute electronic structure of materials. The mathematical frameworks used in the current study can be programmed into a QC formalism. A natural question that arises here is our choice of OFDFT as the quantum mechanical sub-framework in the larger framework of multiscale method development. Arguably, Kohn-Sham-DFT will suit better for it’s accuracy and theoretical robustness, refer [52] and [41] for recent developments in finite-element implementation of KSDFT. However, a direct implementation of Kohn-
Recommended publications
  • God and Design: the Teleological Argument and Modern Science
    GOD AND DESIGN Is there reason to think a supernatural designer made our world? Recent discoveries in physics, cosmology, and biochemistry have captured the public imagination and made the design argument—the theory that God created the world according to a specific plan—the object of renewed scientific and philosophical interest. Terms such as “cosmic fine-tuning,” the “anthropic principle,” and “irreducible complexity” have seeped into public consciousness, increasingly appearing within discussion about the existence and nature of God. This accessible and serious introduction to the design problem brings together both sympathetic and critical new perspectives from prominent scientists and philosophers including Paul Davies, Richard Swinburne, Sir Martin Rees, Michael Behe, Elliott Sober, and Peter van Inwagen. Questions raised include: • What is the logical structure of the design argument? • How can intelligent design be detected in the Universe? • What evidence is there for the claim that the Universe is divinely fine-tuned for life? • Does the possible existence of other universes refute the design argument? • Is evolutionary theory compatible with the belief that God designed the world? God and Design probes the relationship between modern science and religious belief, considering their points of conflict and their many points of similarity. Is God the “master clockmaker” who sets the world’s mechanism on a perfectly enduring course, or a miraculous presence continually intervening in and altering the world we know? Are science and faith, or evolution and creation, really in conflict at all? Expanding the parameters of a lively and urgent contemporary debate, God and Design considers the ways in which perennial questions of origin continue to fascinate and disturb us.
    [Show full text]
  • Fermi Estimates: from Harry Potter to ET
    Fermi Estimates: from Harry Potter to ET David Wakeham May 30, 2019 Abstract Some notes on Fermi estimates and methods for doing them, presented at the UBC Physics Circle in May, 2019. We’ll look at various applications, including global computer storage, the length of the Harry Potter novels, and the probability of intelligent aliens in the galaxy. Note: This is a rough draft only; I hope to polish these and add pictures and additional exercises at some point. For any comments, suggestions, or corrections, please get in touch at <[email protected]>. Contents 1 Introduction 1 1.1 Why Fermi problems? . 2 1.2 Powers of 10 . 2 2 Fermi problems 4 2.1 Comparison . 4 2.2 Factorisation . 6 2.3 Units . 7 2.4 Piano tuners . 10 3 Aliens 11 3.1 Counting aliens . 12 3.2 Cosmic numbers . 13 1 Introduction I’m going to be talking about Fermi problems: what they are, methods for solving them, and if there’s time, a fun application to the search for extraterrestrial intelligence, i.e. aliens we can talk to. Who knows what a Fermi problem is? Has anyone done one before? A Fermi problem is an order of magnitude estimate. Roughly speaking, it means to guess an answer to the nearest power of 10. 1 1.1 Why Fermi problems? Fermi problems are great because the nearest power of 10 is a very forgiving notion of correct- ness, and because they’re so forgiving, we can accurately estimate many things which seem impossible at first sight.
    [Show full text]
  • Engineering Notation Versus Scientific Notation
    ESTIMATION Chapter 5 Estimation Problems Number of hair on your head? Drops of water in a lake? HafiZ of Quran in the world? Estimation Problems •How many cubic yards of concrete are needed to pave one mile of interstate highway (two lanes each direction) ? •How many feet of wire are needed to connect the lighting systems in an automobile? Enrico Fermi Brilliant scientist and engineer Worked in Manhattan Project Development of Nuclear weapons Witnessed Trinity Test First atomic bomb explosion Enrico Fermi •Nobel laureate •Taught at University of Chicago • Gave students problems: • Much information missing • Solution seemed impossible •Such problems: Fermi problems Trinity Test • After the explosion •Brighter than in full daylight • After a few seconds • Rising flames lost their brightness • Huge pillar of smoke • Rose rapidly beyond the clouds • A height of the order of 30,000 feet Trinity Test •About 40 seconds after the explosion • Dropped small pieces of paper • From a height of 6 feet • Measured displacement of pieces of paper • Shift was about 2½ meters •Fermi estimated the intensity of explosion: • As from ten thousand tons of T.N.T. Trinity Test • calculated the explosion to be 19 kilotons. • By observing the behavior of falling bits of paper ten miles from the ground zero, Fermi's estimation of 10 kilotons was in error by less than a factor of 2. • After the war, Fermi taught at the university of Chicago where he became famous for his unsolvable problems FERMI PROBLEMS • Fermi's problems require the person considering them to determine the answer with far less information than would be necessary to calculate an accurate value.
    [Show full text]
  • Gamma Ray Bursts: Back to the Blackboard
    Gamma Ray Bursts: back to the blackboard Maxim Lyutikov Department of Physics, Purdue University, 525 Northwestern Avenue, West Lafayette, IN 47907-2036 Abstract Exceptional observational breakthroughs in the field of Gamma Ray Burst research are not paralleled by theoretical advances. In this re- view, based on the introductory talk given at the "The Shocking Uni- verse" meeting, I argue that any present day model of GRBs, especially of Short type, is grossly incomplete. I will highlight various contradic- tions with observations that many models face and briefly mention a number of ideas that might or might not work. In particular, I will discuss (i) a possibility that early X-ray afterglows are coming from internal dissipation, and not from the forwards shock; (ii) that prompt radiation is beamed in the outflow frame. It is impossible to obtain wages from a republic [...] without having duties attached. [...] so long as I am capable of lecturing and serving, no one in the republic can exempt me from duty arXiv:0911.0349v4 [astro-ph.HE] 3 Feb 2010 while I receive pay. I can hope to enjoy these benefits only from an absolute ruler. 1 Galilei, Opere x, 348 ff 1In modern words, Galilei did not want to teach and write grant applications in the Re- public of Venice, thinking that only monarchy in Florence can give him scientific freedom. As we know, years later he was proven wrong. 1 1 Instead of introduction The launch of Swift satellite (Gehrels, 2004) and ensuing discoveries, recent Fermi results (e.g. on GRB080916C Abdo, 2009), combined with maturing of the fast response GRB observations at other wave lengths, are shaking the foundation of the GRB science (for a recent review, see Gehrels et al., 2009).
    [Show full text]
  • Homework #1, AST 203, Spring 2012 Due in Class (I.E
    Homework #1, AST 203, Spring 2012 Due in class (i.e. by 4:20 pm), Thursday February 16 • To receive full credit, you must give the correct answer and show that you understand it. This requires writing your explanations in full, complete English sentences, clearly labeling all figures and graphs, showing us how you did the arithmetic, and being explicit about the units of all numbers given. All relevant mathematical variables should be explicitly defined. And please use your best handwriting; if we can't read it, we can't give you credit for it! Please staple together the sheets of paper you hand in. Please read http://www.astro.princeton.edu/ast203/writeup.pdf • Most of the calculations in this course involve numbers that are only approximately known. The result of such a calculation should reflect this imprecision. In particular, it is wrong to simply write down all the digits that your calculator spits out. Your final answer should have the same number of significant figures as the least precise number going into your calculation. In many (but not all!) cases, it's best to do the problems without a calculator. Please read http://www.astro.princeton.edu/ast203/mathtips.pdf • A number of useful formulas and quantities are summarized at http://www.astro.princeton.edu/ast203/formulas.pdf • Feel free to work with your classmates on this homework, but your write-up and wording should be your own. Answer all questions. 100 total points 1. Scientific notation review 10 total points Write the following in proper scientific notation, giving the proper number of significant figures.
    [Show full text]
  • Fermi Questions and Orders of Magnitude
    FERMI QUESTIONS AND ORDERS OF MAGNITUDE Patrick Liscio November 2019 Math CoOp ENRICO FERMI • Prominent physicist who worked on Manhattan Project during WWII • Known for making good, fast approximations • Estimated strength from first nuclear bomb test to within a factor of 2 FERMI QUESTIONS • Fermi questions are estimation problems where we have to guess some really large quantity using very little information. Things like: • How many fish are in the sea? • About 3 trillion • How long would it take to read all of Wikipedia? • About 20 years if it stopped updating • How many leaves are on an average, fully grown oak tree • About 200,000 How close to 200,000 leaves should our guess be? WHAT IS A GOOD GUESS? • 1 leaf is definitely too small • 100,000,000,000,000,000 (number of leaves in the world) definitely too big • Is “off by 5 leaves” good enough? • 199,995 or 200,005 both much more accurate than we could ever hope for • Is “off by 10%” good enough? • 180,000 or 220,000 probably still within error of approximation • What about 20,000? 2,000,000? MAIN MATH TOOL: POWERS OF 10 • Sometimes, we only care about “orders of magnitude” Decreasing by 1 order of magnitude: • Number of times you have to multiply or divide your answer by 10 to get 200000 to the right answer ↓ • 20,000 is 1 order of magnitude too low, 2,000,000 is 1 order of magnitude too high 200000 ↓ • What about 2,000? 20000 • 2 orders of magnitude too low, since you have to multiply by 10 twice to get to 200,000 Increasing by 1 order of magnitude: • What about 50,000? • Less
    [Show full text]
  • Basic Skills in Physics and Engineering Science
    Basic skills in physics and engineering science a guide to critical thinking about modelling Göran Grimvall KTH, Stockholm 2011 © Göran Grimvall Preface Information explosion, interdisciplinary work, lifelong learning and globalization are concepts, which mean that we must be prepared to take in and use new knowledge. In science and technology this knowledge often has a numerical aspect; in the form of data, as explicit mathematical relations, or disguised as computer models whose structure may even be unknown to the user. This challenge is made particularly acute through the Internet. Even if our internet source is reliable – how can we be sure that we are interpreting and using the information correctly? This text is meant to be a guide in this new world. Many of the presented ‘skills’ are what a practicing scientist or engineer acquires during a long life, often without being explicitly aware of it. It is like learning to speak your mother tongue, without attending a formal language course. A quicker way is offered here. Many of the ideas described in these notes are given a more popular presentation in the author's books Brainteaser Physics (2007) and Quantify! – A Crash Course in Smart Thinking (2011). Some aspects are treated in more depth than elsewhere, for instance estimation methods, while dimensional analysis and scaling have been extensively covered in many books. The main feature of the present work is a systematic approach, with examples from very many fields – not only science and engineering but also referring to, e.g., sports, economics, literature, historical aspects and daily life. The text is divided into two parts.
    [Show full text]
  • Fermi Paradox from Wikipedia, the Free Encyclopedia Jump To: Navigation, Search
    Fermi paradox From Wikipedia, the free encyclopedia Jump to: navigation, search This article is about the absence of evidence for extraterrestrial intelligence. For the type of estimation problem, see Fermi problem. For the music album, see Fermi Paradox (album). For the short story, see The Fermi Paradox Is Our Business Model. A graphical representation of the Arecibo message – Humanity's first attempt to use radio waves to actively communicate its existence to alien civilizations The Fermi paradox (or Fermi's paradox) is the apparent contradiction between high estimates of the probability of the existence of extraterrestrial civilization and humanity's lack of contact with, or evidence for, such civilizations.[1] The basic points of the argument, made by physicists Enrico Fermi and Michael H. Hart, are: • The Sun is a young star. There are billions of stars in the galaxy that are billions of years older; • Some of these stars likely have Earth-like planets[2] which, if the Earth is typical, may develop intelligent life; • Presumably some of these civilizations will develop interstellar travel, as Earth seems likely to do; • At any practical pace of interstellar travel, the galaxy can be completely colonized in just a few tens of millions of years. According to this line of thinking, the Earth should have already been colonized, or at least visited. But no convincing evidence of this exists. Furthermore, no confirmed signs of intelligence elsewhere have been spotted, either in our galaxy or the more than 80 billion other galaxies of the
    [Show full text]
  • THE GREAT SILENCE the Science and Philosophy of Fermi's
    The Great Silence THE GREAT SILENCE The Science and Philosophy of Fermi’s Paradox milan m. ćirković 1 1 Great Clarendon Street, Oxford, OX2 6DP, United Kingdom Oxford University Press is a department of the University of Oxford. It furthers the University’s objective of excellence in research, scholarship, and education by publishing worldwide. Oxford is a registered trade mark of Oxford University Press in the UK and in certain other countries © Milan M. Ćirković 2018 The moral rights of the author have been asserted First Edition published in 2018 Impression: 1 All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted, in any form or by any means, without the prior permission in writing of Oxford University Press, or as expressly permitted by law, by licence or under terms agreed with the appropriate reprographics rights organization. Enquiries concerning reproduction outside the scope of the above should be sent to the Rights Department, Oxford University Press, at the address above You must not circulate this work in any other form and you must impose this same condition on any acquirer Published in the United States of America by Oxford University Press 198 Madison Avenue, New York, NY 10016, United States of America British Library Cataloguing in Publication Data Data available Library of Congress Control Number: 2017954178 ISBN 978–0–19–964630–2 Printed and bound by CPI Group (UK) Ltd, Croydon, CR0 4YY Links to third party websites are provided by Oxford in good faith and for information only. Oxford disclaims any responsibility for the materials contained in any third party website referenced in this work.
    [Show full text]
  • Solutions to Problem Set #1, AST 203 Due on February 16, 2012 General Grading Rules: One Point Off Per Question (E.G., 2A Or
    Solutions to Problem Set #1, AST 203 Due on February 16, 2012 General grading rules: One point off per question (e.g., 2a or 2b) for egregiously ignoring the admonition to write in full sentences. One point off per question for inappropriately high precision (which usually means more than 2 significant figures in this homework). No more than 2 total points per problem off for not writing in full sentences, and two points per problem for overly high precision. Three points off for each arithmetic or algebra error. Further calculations correctly done based on this erroneous value should be given full credit. However, if the resulting answer is completely ludicrous (e.g., 10−30 seconds for the time to travel to the nearest star, 50 stars in the visible universe), and no mention is made that the value seems wrong, take three points off. One point off per question for not being explicit about the units, or for not expressing the final result in the units requested. Specific instructions for each problem take precedence over the above. In each question, one cannot get less than zero points, or more than the total number the question is worth. 1. Scientific notation review 10 total points (2-2-2-2-2) Write the following in proper scientific notation. Full sentences are not required here. a) Four hundred seventy million Answer: 4:7 × 108 The answer 4:70 × 108 gets full credit. Equivalent answers, such as 470 × 106, get full credit. More zeroes added on get one point off. Rounding to 5 × 108, or 4 × 108, gets no credit.
    [Show full text]
  • Lecture Notes
    Astron 211, Fall 2017 Lecture I.0 Astronomy 211 ASTRON 211 FALL 2017 1 Astron 211, Fall 2017 Lecture I.3 Lecture I Preliminaries Course Description: quantitative astronomy. Emphasis on the “why” and the “how” rather than just the “what.” There will be some math(!) and physics. There will be no calculus. If you don’t want that, look at ASTRON 103. If you want a lab, take ASTRON 104. Here we will cover: • Celestial mechanics • The nature of light and its interaction with matter • Telescopes • The structure and evolution of single stars • The evolution of binary stars • The end-products of stellar evolution • The Solar System • Extra-solar planets • Galaxies & quasars • Expansion of the universe & dark matter • The big bang The textbook will be Kutner: Astronomy: A Physical Perspective Evaluation will be: • Weekly problem sets (50%), with the best 10 of 11 counting. • Weekly D2L quizzes (5%) • Weekly in-class problems (5%) • Midterm exam (20%) • Final exam (20%) I.2 Set the Stage Astrophysics mostly starts next lecture. ASTRON 211 FALL 2017 2 Astron 211, Fall 2017 Lecture I.4 I.3 Physics Synopsis The level of physics and math that you are expected to be familiar with (but not necessarily know in detail) is: Newton’s Laws : most importantly, F = ma 1 2 Kinetic Energy : K = 2 mv 2 Gravitation : F = GM1M2=r (on the surface of the Earth, F = gm) Potential Energy : U = −GM1M2=r (from gravity; on the surface of the Earth, U = gmh) Centripetal Acceleration : a = v2=r Ideal Gas Law : PV = NRT Circumference of a Circle : 2πr Area of Circle : πr2 Surface Area of a Sphere : 4πr2 4 3 Volume of a Sphere : 3 πr Radians : 180◦ = π radians, sin(π=2) = 1, sin π = 0, etc.
    [Show full text]
  • Sensitivity Analysis of Computational Models for Solving Paradox
    Sensitivity Analysis of Computational Models for solving Paradox Jurij Nastran, Beno Sircelj, Matjaz Gams “Jozef Stefan” Institute, Jamova cesta 39 Ljubljana, Slovenia [email protected] [email protected] [email protected] Drago Bokal University of Maribor, Koroska cesta 46 Maribor, Slovenia [email protected] ABSTRACT: Given the estimated number of stars and planets in our galaxy, the probability of existence of intelligent civilizations seems high. The first to indicate this was the Drake equation with the assumed default parameters. Yet, the actual observations have yet to reflect those expectations. This discrepancy corresponds to the so-called Fermi Paradox. Although many key factors about the likelihood of alien civilizations still remain largely unknown, new methods of estimating the probability are being proposed. Some of them use probability distributions and the Monte Carlo methods. In this paper we recalculate one of those - the Sandberg interpretation of the Drake equation, analyze the difference between the methods, their strengths and weaknesses. In the conclusion, we find that the probability distribution better reflects our ignorance about the properties of alien environments than the dot-product method. In our opinion, there are several ways to further improve the computational model based on the Drake equation using the AI methods, thus eliminating the problem with too small probabilities and introducing 3D views. What makes these analysis relevant, is not only the number of estimated civilizations in our galaxy and a probability that we encounter them in the near future. More important, these models enable estimation of the life-span of the human civilization.
    [Show full text]