Ferromagnetism in neutron matter

Slides:



Advertisements
Similar presentations
Spin order in correlated electron systems
Advertisements

Topological current effect on hQCD at finite density and magnetic field Pablo A. Morales Work in collaboration with Kenji Fukushima Based on Phys. Rev.
Microscopic time-dependent analysis of neutrons transfers at low-energy nuclear reactions with spherical and deformed nuclei V.V. Samarin.
How do nuclei rotate? 5. Appearance of bands. Deformed mean field solutions This is clearly the case for a well deformed nucleus. Deformed nuclei show.
January 23, 2001Physics 8411 Elastic Scattering of Electrons by Nuclei We want to consider the elastic scattering of electrons by nuclei to see (i) how.
Spin polarization phenomena in dense nuclear matter Alexander Isayev Kharkov Institute of Physics and Technology Ukraine.
Lesson 9 Dipoles and Magnets. Class 27 Today we will: learn the definitions of electric and magnetic dipoles. find the forces, torques, and energies on.
Pavel Bakala Eva Šrámková, Gabriel Török and Zdeněk Stuchlík Institute of Physics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo.
ELECTRON SPIN RESONANCE Nathan Farwell and Dylan Prendergast SYSTEM SETUP. In this experiment we examine the aspects of microwave spectroscopy. We investigated.
Monte Carlo Simulation of Ising Model and Phase Transition Studies
Possible neutron star compositions Spin evolution of neutron stars.
Physics 2225: Magnetic Fields Purpose of this Minilab Learn about the shape and strength of the magnetic fields created by magnetic dipoles. Determine.
Subir Sachdev Yale University Phases and phase transitions of quantum materials Talk online: or Search for Sachdev on.
Physical Chemistry 2nd Edition
Monte Carlo Simulation of Ising Model and Phase Transition Studies By Gelman Evgenii.
Magnetic Material Engineering. Chapter 6: Applications in Medical and Biology Magnetic Material Engineering.
Calculating the moment of inertia of neutron stars Jacobus Diener Stellenbosch University, RSA Dr Alan Dzhioev and Prof Victor Voronov Bogoliubov Laboratory.
A Comparison of a Mean Field Theoretic Approach to Ferromagnetism with Experimental Results Patrick Yarbrough- Department of Physics and Engineering The.
Essential Knowledge 1.A.4: Atoms have internal structures that determine their properties. a. The number of protons in the nucleus determines the number.
Quadrupole moments of neutron stars and strange stars Martin Urbanec, John C. Miller, Zdenek Stuchlík Institute of Physics, Silesian University in Opava,
Effects of self-consistence violations in HF based RPA calculations for giant resonances Shalom Shlomo Texas A&M University.
Lecture 20: More on the deuteron 18/11/ Analysis so far: (N.B., see Krane, Chapter 4) Quantum numbers: (J , T) = (1 +, 0) favor a 3 S 1 configuration.
Equation Of State and back bending phenomenon in rotating neutron stars 1 st Astro-PF Workshop – CAMK, 14 October 2004 Compact Stars: structure, dynamics,
Type I and Type II superconductivity
Lecture 19 Magnetism and Matter Learning Objective: to examine some aspects of magnetic properties of materials Transformers Motors Generators (for examples)
Ferromagnetism in nuclear matter (and how it relates to neutron stars) Jacobus Diener (PhD student) Supervisors: Prof FG Scholtz and Prof HB Geyer Department.
Influence of Lorentz violation on the hydrogen spectrum Manoel M. Ferreira Jr (UFMA- Federal University of Maranhão - Brazil) Colaborators: Fernando M.
Example: Find the electric field at point P Rework of this example (21.6 in book)
Plasma - What It Is, What It isn’t A Shocking Exposé with Investigations by McGourty and Rideout.
Pavel Bakala Martin, Urbanec, Eva Šrámková, Gabriel Török and Zdeněk Stuchlík Institute of Physics, Faculty of Philosophy and Science, Silesian University.
Spontaneous symmetry breaking and rotational bands S. Frauendorf Department of Physics University of Notre Dame.
Evan Knight and Adam Mali UCORE, Summer ‘07 Under Prof. James Imamura and Kathy Hadley.
 Nature of nuclear forces, cont.  Nuclear Models lecture 3&4.
Lecture X Magnetism and Matter Learning Objective: to examine some aspects of magnetic properties of materials.
Atoms: The Building Blocks of Matter Unit 2.  Introduction to the Atom Modern Atomic Theory Subatomic Particles Isotopes Ions Essential Standards and.
Non-Fermi Liquid Behavior in Weak Itinerant Ferromagnet MnSi Nirmal Ghimire April 20, 2010 In Class Presentation Solid State Physics II Instructor: Elbio.
NEUTRON SKIN AND GIANT RESONANCES Shalom Shlomo Cyclotron Institute Texas A&M University.
Spin Precession Animation “DEMO”
Passage of magnetostatic waves through the lattice on the basis of the magnon crystal. Performed by Lanina Mariya, III year student, Faculty of Nonlinear.
Operated by Jefferson Science Association for the U.S. Department of Energy Thomas Jefferson National Accelerator Facility Page 1 Check directly vs data.
Magnetic Resonance Imaging Glenn Pierce, King’s College London, Department of Physics Introduction Edward Purcell and Felix Bloch were both awarded the.
ELECTROWEAK UNIFICATION Ryan Clark, Cong Nguyen, Robert Kruse and Blake Watson PHYS-3313, Fall 2013 University of Texas Arlington December 2, 2013.
Some theoretical aspects of Magnetars Monika Sinha Indian Institute of Technology Jodhpur.
PROPERTIES OF HIGH-ENERGY ISOSCALAR MONOPOLE EXCITATIONS IN MEDIUM-HEAVY MASS SPHERICAL NUCLEI M. L. Gorelik 1), S. Shlomo 2), B. A. Tulupov 3), M. H.
Crystal Ball Collaboration Meeting, Basel, October 2006 Claire Tarbert, Univeristy of Edinburgh Coherent  0 Photoproduction on Nuclei Claire Tarbert,
ON EXISTENCE OF HALO ORBITS IN COMPACT OBJECTS SPACETIMES Jiří Kovář Zdeněk Stuchlík & Vladimír Karas Institute of Physics Silesian University in Opava.
Spin Wave Model to study multilayered magnetic materials Sarah McIntyre.
Biot-Savart Law for a Single Charge Electric field of a point charge: Moving charge makes a curly magnetic field: B units: T (tesla) = kg s -2 A -1 The.
The role of isospin symmetry in medium-mass N ~ Z nuclei
ШАПКА DNA-Single Walled Carbon Nanotube Hybrids:
Charge in very strong EM field
I shall present a many body problem which is:
Predicting the BRAING INDEX OF INTERMITTENT AND NULLING PULSARS
Spontaneous Symmetry Breaking and Analogies to the Higgs-Mechanism
The Electronic Structure of Atoms
MAGNETIC MATERIALS. MAGNETIC MATERIALS – Introduction MAGNETIC MATERIALS.
dark matter Properties stable non-relativistic non-baryonic
The Magnetic Properties of the Anti-collinear Phase under the Effects of a Uniform External Magnetic Field in a Two Dimensional Square Planar System By.
Hydrogen Atom Returning now to the hydrogen atom we have the radial equation left to solve The solution to the radial equation is complicated and we must.
Experiment Experiment: thing ferromagnetic films
Check directly vs data That is, apply new effective force directly to calculate nuclear properties using Hartree-Fock (as for usual well known force)
Nuclear Physics, JU, Second Semester,
Nuclear Magnetic Resonance (NMR) Spectroscopy
10.3 NMR Fundamentals nuclear spin calculations and examples
Efrain J. Ferrer Paramagnetism in Compact Stars
Samara State University, Samara, Russia
Magnetic Fields (1) Elliott.
How do nuclei rotate? 5. Appearance of bands.
Nuclear Magnetic Resonance
Constraining the Nuclear Equation of State via Nuclear Structure observables 曹李刚 中科院近物所 第十四届全国核结构大会,湖州,
Presentation transcript:

Ferromagnetism in neutron matter ...and how it could apply to neutron stars JPW Diener1 , FG Scholtz1,2, HB Geyer1, GC Hillhouse3 1 Institute of Theoretical Physics, Stellenbosch University 2 National Institute for Theoretical Physics, Stellenbosch 3 New York Institute of Technology, Nanjing, China

Introduction We are investigating pulsar/neutron star matter. One of the densest states of matter. Aiming to better understand the magnetic field of these stars. Pulsars are made up (in part at least) of nuclear matter. We are investigating the spontaneous magnetisation of neutron matter.

Ferromagnetism Ferromagnetism is a property of any system that can undergo a phase transition from an unmagnetised to a magnetised state. (Ferro)magnetised matter Unmagnetised matter

Neutrons Neutrons are neutral particles, with spin ±½. Dipole moment reacts to a external magnetic field. Aligned dipole moments induce a magnetic field. Spontaneous magnetisation will occur if a stable, lower energy (magnetic) configuration is available. Neutron with the magnetic dipole moment

Relativity Relativistic description of ferromagnetism. Relativity: Albert Einstein’s most famous equation: More general form: Considering plane waves solution and natural units (ћ = c = 1) Non-relativistic energy-momentum relationship:

Neutron matter dispersion relationship

Magnetic neutron matter Including the magnetic field in a relativistic fashion, the energy-momentum relationship is modified: For zero momentum: (External) magnetic field introduces a specific direction, breaking spherical symmetry.

Neutron matter dispersion relationship (2)

Magnetised vs unmagnetised system

Ferromagnetic state External magnetic field makes a lower energy state available. If lower energy state is favoured, a magnetic field is induced. Ferromagnetic state would be stable if the induced magnetic field is equal to the external field.

Conclusions and way forward Have shown that lower energy state exists. Strength of induced magnetic field as function of density still unknown. To be calculated. Compare to experimental known properties of the neutron to determine accuracy. If there is agreement, then we would be able to predict at what densities a ferromagnetic phase would present itself.

Acknowledgements This research is support by the SA SKA project, and, Stellenbosch University.