Generation of Magnetic Fields in Gravitationally Forming Structures in the Early Universe Russell M. Kulsrud Princeton Plasma Physics Laboratory.

Slides:



Advertisements
Similar presentations
9.2 Gravitational field, potential and energy
Advertisements

Dynamo Effects in Laboratory Plasmas S.C. Prager University of Wisconsin October, 2003.
Magnetic Relaxation in MST S. Prager University of Wisconsin and CMSO.
Ion Heating Induced by Waves Russell M. Kulsrud Princeton Plasma Physics Laboratory.
Galactic Dynamos and ISM Turbulence. Steve Cowley,UCLA/ Imperial College Alex Schekochihin, Imperial Jim McWilliams, UCLA Greg Hammett, Princeton Greg.
The Accretion of Poloidal Flux by Accretion Disks Princeton 2005.
Multiple reconnections and explosive events and in MST and solar flares Gennady Fiksel CMSO workshop, Princeton, NJ, Oct 5-8, 2005.
Some New Data From FRC Experiment on Relaxation For discussions at Hall-Dynamo and Related Physics meeting CMSO June 10-11, 2004 at PPPL Guo et al, PRL.
Magnetic Turbulence during Reconnection General Meeting of CMSO Madison, August 4-6, 2004 Hantao Ji Center for Magnetic Self-organization in Laboratory.
Outline Dynamo: theoretical General considerations and plans Progress report Dynamo action associated with astrophysical jets Progress report Dynamo: experiment.
arvard.edu/phot o/2007/m51/. Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies Q. Daniel Wang,
The Thick Disks of Spiral Galaxies as Relics from Gas-Rich, Turbulent, Clumpy Disks at High Redshifts Frédéric Bournaud, Bruce G. Elmegreen, and Marie.
Physics of fusion power
PHY306 1 Modern cosmology 3: The Growth of Structure Growth of structure in an expanding universe The Jeans length Dark matter Large scale structure simulations.
September 2005 Magnetic field excitation in galaxies.
THE ORIGIN OF COSMIC RAYS Implications from and for X and γ-Ray Astronomy Pasquale Blasi INAF/Osservatorio Astrofisico di Arcetri, Firenze.
“The interaction of a giant planet with a disc with MHD turbulence II: The interaction of the planet with the disc” Papaloizou & Nelson 2003, MNRAS 339.
The Movement of Charged Particles in a Magnetic Field
SELF-SIMILAR SOLUTIONS OF VISCOUS RESISTIVE ACCRETION FLOWS Jamshid Ghanbari Department of Physics, School of Sciences, Ferdowsi University of Mashhad,
Evidence from the Motions of Old Stars that the Galaxy Collapsed O. J. Eggen, D. Lynden-Bell, and A. R. Sandage 1962, ApJ, No. 136, p. 748 Presented by:
Evolution of magnetic fields in galaxies Dmitry Sokoloff Moscow State University Moscow, Russia in collaboration with R.Beck, T.G.Arshakian, M.Krause,
1. 2 Apologies from Ed and Karl-Heinz
Chapter 19.
The Birth of Solar Systems A solar system The disk condenses and dissipates Collapse of and interstellar cloud Formation of a protostar and disk.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
Flux emergence: An overview of thin flux tube models George Fisher, SSL/UC Berkeley.
New Mechanism of Generation of Large-Scale Magnetic Field in Turbulence with Large-Scale Velocity Shear I. ROGACHEVSKII, N. KLEEORIN, E. LIVERTS Ben-Gurion.
ASTR100 (Spring 2008) Introduction to Astronomy Galaxy Evolution & AGN Prof. D.C. Richardson Sections
Cosmological MHD Hui Li Collaborators: S. Li, M. Nakamura, S. Diehl, B. Oshea, P. Kronberg, S. Colgate (LANL) H. Xu, M. Norman (UCSD), R. Cen (Princeton)
Plasma Dynamos UCLA January 5th 2009 Steve Cowley, UKAEA Culham and Imperial Thanks to Alex Schekochihin, Russell Kulsrud, Greg Hammett and Mark Rosin.
Physics of fusion power Lecture 7: particle motion.
A generic test for Modified Gravity Models* Emre Onur Kahya University of Florida * astro-ph/
Gradient of Scalar Field In Cartesian co-ordinates:
(MNRAS 327, 610, 2001 & 347, 1234, 2004) David Churches, Mike Edmunds, Alistair Nelson - Physics & Astronomy, Cardiff University - Physics & Astronomy,
Galaxy Mass Star Number/Density Counting stars in a given volume
Magnetic dynamo over different astrophysical scales Axel Brandenburg & Fabio Del Sordo (Nordita) with contributions from many others seed field primordial.
Universal Gravitation Chapter 8. Isaac Newton and Gravity Newton realized an apple falls because of force Moon follows circular path, force needed Newton.
Space physics EF2245 Tomas Karlsson Space and Plasma Physics School of Electrical Engineering EF2245 Space Physics 2009.
Effect of Magnetic Helicity on Non-Helical Turbulent Dynamos N. KLEEORIN and I. ROGACHEVSKII Ben-Gurion University of the Negev, Beer Sheva, ISRAEL.
Physics 681: Solar Physics and Instrumentation – Lecture 19 Carsten Denker NJIT Physics Department Center for Solar–Terrestrial Research.
Star Formation. Introduction Star-Forming Regions The Formation of Stars Like the Sun Stars of Other Masses Observations of Brown Dwarfs Observations.
JP ©1 2 3 Stars are born, grow up, mature, and die. A star’s mass determines its lifepath. Let M S = mass of the Sun = ONE SOLAR MASS Stellar Evolution.
Chapter 19 Star Formation
Galaxy Formation and Dark Galaxies John Schreiber.
Overshoot at the base of the solar convection zone What can we learn from numerical simulations? Matthias Rempel HAO / NCAR.
Plasma universe Fluctuations in the primordial plasma are observed in the cosmic microwave background ESA Planck satellite to be launched in 2007 Data.
 E-field lines originate on positive charges and terminate on negative charges (Gauss’ Law)  B-field lines always form closed loops.  Changing B-field.
© 2010 Pearson Education, Inc. Chapter 21 Galaxy Evolution.
By: Rose Zimmerman. Main Points  Shape  Classification  Properties  Large Magellanic Cloud  Small Magellanic Cloud  Dwarf Irregular Galaxy  Stars.
Propagation and acceleration of High Energy CRs
The Magneto-Rotational Instability and turbulent angular momentum transport Fausto Cattaneo Paul Fischer Aleksandr Obabko.
A computer graphic investigation of a possible mechanisim for the origin of planetary motion Russell Lowke CSCIE-236, Final Project, May 25th 2005.
The Matter Force The Matter Force By By Ray Fleming Ray Fleming.
Gravitation Ch 5: Thornton & Marion. Integral for of Gauss’ Law For spherically symmetric cases, g is in the radial direction, and so is n-hat.
Spiral Triggering of Star Formation Ian Bonnell, Clare Dobbs Tom Robitaille, University of St Andrews Jim Pringle IoA, Cambridge.
Gravitational Field Strength
Gravitational Potential Energy Consider an object a distance r from the center of the Earth. Where would the object need to be so that the gravitational.
Space physics EF2245 Tomas Karlsson Space and Plasma Physics School of Electrical Engineering EF2245 Space Physics 2010.
Chapter 21 Galaxy Evolution Looking Back Through Time Our goals for learning How do we observe the life histories of galaxies? How did galaxies.
ANGULAR MOMENTUM TRANSPORT BY MAGNETOHYDRODYNAMIC TURBULENCE Gordon Ogilvie University of Cambridge TACHOCLINE DYNAMICS
Seeding the ICM: Primordial or Astrophysical? Jungyeon Cho Chungnam National University, Korea Cho & Yoo (2012; ApJ) Cho (2013; PRD) Cho (2014, ApJ) Origin.
Star Formation. Chapter 19 Not on this Exam – On the Next Exam!
Laser target interactions, and space/solar physics simulation experiments (Seed funding project) Laser-target: Boris Breizman, Alex Arefiev, Mykhailo Formyts'kyi.
The Milky Way Galaxy • Introduction • Structure • Formation
Plasma outflow from dissipationless accretion disks
Types of Forces Chapter 9.1.
Chapter 21 Galaxy Evolution
Chapter 21 Galaxy Evolution and Black Holes
The Sun.
Hideki Maki Department of Physics, Rikkyo University
Presentation transcript:

Generation of Magnetic Fields in Gravitationally Forming Structures in the Early Universe Russell M. Kulsrud Princeton Plasma Physics Laboratory

OUTLINE PROPERTIES OF OUR GALACTIC MAGNETIC FIELD STANDARD DISC DYNAMO THEORY PROTOGALACTIC ORIGIN

OUR GALACTIC MAGNETIC FIELD The field is toroidal. Its strength is 2 microgauss. It varies in radius possibly changing every spiral arm or about one kiloparsec. It does not change in the direction perpendicular to the disc. Figure 1: The galactic magnetic field

THE ALPHA-OMEGA DISC DYNAMO THEORY THE THEORY CONSERVES FLUX, SO TO WORK IT HAS TO EXPEL NEGATIVE FLUX THIS IS VERY DIFFICULT BECAUSE THE GALACTIC DISC IS IN A DEEP POTENTIAL WELL AND THE FLUX MUST CARRY MATTER OUT WITH IT Figure 2: The escape of negative flux in the Alpha- Omega dynamo.

OTHER ORIGINS The Galaxy was originally a plasma in the form of a protogalaxy » 100kpc with a mass of solar masses. It resulted from a gravitational collapse and smaller parts also suffered gravitational collapse creating many small shocks.

Shocks Creating Turbulence These shocks produced vorticity, turbulence, weak magnetic fields (Biermann) and heating that led to the support of the protogalaxy against gravity.

k

The Magnetic Differential Equation

The Solution

B 0 =6£10 -6 gauss lnB/B0 lnk/k0

CONCLUSION Magnetic Fields may have already been generated before our galaxy was fully formed due to plasma processes in the preceding protogalaxy. This may be a common phenomenon.