I.Laktineh, IPNL 1 Nagoya, 2006 Studying the neutron quantum states in the gravitational field “using nuclear emulsion technique” Motivations Motivations.

Slides:



Advertisements
Similar presentations
TRIUMF UCN workshop, 2007 Solid state physics experiments with UCN E. Korobkina.
Advertisements

1 The structure and evolution of stars Lecture 3: The equations of stellar structure Dr. Stephen Smartt Department of Physics and Astronomy
X X X X X10 14.
The photon, the quantum of light
Tomsk Polytechnic University1 A.S. Gogolev A. P. Potylitsyn A.M. Taratin.
FARADAY ROTATION Gennady Voronov In this experiments we experimentally determine the Verdet constant of a glass rod with specification SF-59 to be rad/mT*cm.
Energy Chapter 10 What is Energy?
Microscopic time-dependent analysis of neutrons transfers at low-energy nuclear reactions with spherical and deformed nuclei V.V. Samarin.
Copyright © 2009 Pearson Education, Inc. Force on an Electric Charge Moving in a Magnetic Field.
Monday, Nov. 11, 2013PHYS , Fall 2013 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #17 Monday, Nov. 11, 2013 Dr. Jaehoon Yu Alpha Particle.
1 Recap Heisenberg uncertainty relations  The product of the uncertainty in momentum (energy) and in position (time) is at least as large as Planck’s.
MARS flux simulations - update Sergei Striganov Fermilab June 3, 2009.
Chamber Dynamic Response Modeling Zoran Dragojlovic.
The Work Being Done at the Ion Beam Laboratory at Texas A&M University Van D. Willey Columbia High School Under the Direction of Lin Shao Assistant Professor.
Lecture 2110/24/05. Light Emission vs. Absorption Black body.
Analysis of Light Single-  Hypernuclei Events in Nuclear Emulsion Detected with Overall-scanning Method MYINT KYAW SOE, Kazuma NAKAZAWA, Kaoru HOSHINO,
Collisions & Center of Mass Lecturer: Professor Stephen T. Thornton
Exploring The Quantum Department of Physics Entering the FreezerThe Age of the Qubit HOTCOLD Quantum properties emerge at extremes of energy. We work with.
Tuesday, Nov. 25, 2014PHYS , Fall 2014 Dr. Jaehoon Yu 1 PHYS 1443 – Section 004 Lecture #24 Tuesday, Nov. 25, 2014 Dr. Jaehoon Yu Refresher: Simple.
Rotational Motion and the Law of Gravity
Gravity at Micron Hartmut Abele. Hartmut Abele, Universität Heidelberg 2 Galileo in Pisa Objekt: Neutron Höhe: ~ 50  m Fallhöhe > 50  m Fallhöhe < 50.
Chapter 9: Radioactivity and Nuclear Reactions The last chapter we will study!
We can find Gravitational Potential Energy r mm GrU 21 )( 
I.Laktineh GranSasso MAY 2003 Stopping  /  at PSI dE/dX Measurement Bern, Naples,Neuchatel,Lyon Aim: to identify stopping pions and muons in the bricks.
ChE 553 Lecture 12 Theory Of Sticking 1. Objective Develop a qualitative understanding of sticking Go over some models for the process 2.
Abab presents today. A closer look at the production process of a movie soundtrack. What elements are affecting recorded sound quality ?
Wednesday, Nov. 6, 2013PHYS , Fall 2013 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #16 Wednesday, Nov. 6, 2013 Dr. Jaehoon Yu Barriers and.
DE/dX measurement by OPERA film Tsutomu Fukuda (Nagoya Univ) Emulsion work shop (11/12,2005)
Physics Lecture 15 10/29/ Andrew Brandt Wednesday October 29, 2014 Dr. Andrew Brandt 0. Hw’s due on next 3 Mondays, test on Nov Wells+Barriers.
Wednesday, Oct. 17, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #13 Wednesday, Oct. 17, 2012 Dr. Jaehoon Yu Properties.
Wave-Particle Duality - the Principle of Complementarity The principle of complementarity states that both the wave and particle aspects of light are fundamental.
The Nuts and Bolts of First-Principles Simulation Durham, 6th-13th December : Computational Materials Science: an Overview CASTEP Developers’ Group.
1 dE/dx  Let’s next turn our attention to how charged particles lose energy in matter  To start with we’ll consider only heavy charged particles like.
INSTITUT MAX VON LAUE - PAUL LANGEVIN V.V.Nesvizhevsky QUARKS-2008 Neutron scattering and extra short-range interactions - Neutron constraints.
1 The structure and evolution of stars Lecture 3: The equations of stellar structure.
Gluing machine (scanning at the edge…) G. Sirri for Bologna Group.
Results from particle beam tests of the ATLAS liquid argon endcap calorimeters Beam test setup Signal reconstruction Response to electrons  Electromagnetic.
Muon absolute flux measurement in anti-neutrino mode A.Ariga 1, C. Pistillo 1, S. Aoki 2 1 University of Bern, 2 Kobe University.
Wednesday, Oct. 31, 2012PHYS , Fall 2012 Dr. Amir Farbin 1 PHYS 3313 – Section 001 Lecture #16 Wednesday, Oct. 31, 2012 Dr. Amir Farbin Reflection.
Contents Introduction (motivation of precise measurements of neutron lifetime, history of experimental accuracy improvement). a. Result of neutron lifetime.
Quantum Chemistry: Our Agenda Postulates in quantum mechanics (Ch. 3) Schrödinger equation (Ch. 2) Simple examples of V(r) Particle in a box (Ch. 4-5)
Pion-Induced Fission- A Review Zafar Yasin Pakistan Institute of Engineering and Applied Sciences (PIEAS) Islamabad, Pakistan.
Spring 2002 Lecture #18 Dr. Jaehoon Yu 1.Simple Harmonic Motion 2.Energy of the Simple Harmonic Oscillator 3.The Pendulum Today’s Homework Assignment.
Physics 207: Lecture 13, Pg 1 Lecture 13 Goals: Assignments: l HW5, due tomorrow l For Wednesday, Read all of Chapter 10 Chapter 9 Chapter 9  Employ.
Neutron exposure at CERN Mitsu KIMURA 19 th July 2013.
1 CMS Sensitivity to Quark Contact Interactions with Dijets Selda Esen (Brown) Robert M. Harris (Fermilab) DPF Meeting Nov 1, 2006.
Ellipsometer B 許恭銓. Problem Overview We have a thin layer of oxide on a Si substrate and we want to find its thickness by using an ellipsometer.
INSTITUT MAX VON LAUE - PAUL LANGEVIN V.V.Nesvizhevsky Institute Laue-Langevin, Grenoble.
The Atom Three Basic Particles. Proton Nucleus of atom Positive charge # of protons (p + ) = atomic number Contain much of the mass of the atom.
Quantum optical experiment on measurement of the gravitational force acting on the neutron Session of the Programme Advisory Committee for Nuclear Physics.
PHY 151: Lecture Motion of an Object attached to a Spring 12.2 Particle in Simple Harmonic Motion 12.3 Energy of the Simple Harmonic Oscillator.
INSTITUT MAX VON LAUE - PAUL LANGEVIN Measurement of parity-violating asymmetries in the reactions of light nuclei with polarized neutrons ( 6.
Lecture 5. Particle Properties of Waves (cont’d)
7/3/2016Milano Consiglio di Sezione AEGIS: a moirè deflectometer for antimatter Marco G. Giammarchi Istituto Nazionale Fisica Nucleare - Milano A E g I.
ANTIHYDROGEN Gravitational States above material surface A. Voronin P.Froelich V.Nesvizhevsky.
qBOUNCE: a quantum bouncing ball gravity spectrometer
Nuclear emulsions One of the eldest particle detectors, still used in particle physics experiment (CHORUS, DONUT, OPERA) for its unique peculiarities:
T. Ariga AEC-LHEP, University of Bern
PHYS 3313 – Section 001 Lecture #16
Solutions of Schrodinger Equation
Latest results from the superfluid-helium UCN source SUN2 at ILL
HOPE – a magnetic UCN trap to measure the neutron lifetime
Using ultracold neutrons to constrain the neutron electric dipole moment Tamas Budner.
New concept of light ion acceleration from low-density target
Joint Institute for Nuclear Research, Dubna, Russia
The Strong Nuclear Force
Gravitational Quantum States of Antihydrogen
Chapter 27 Early Quantum Theory
Fragmentation cross sections of Fe26+, Si14+ and C6+ ions of 0
Study of charm hadroproduction Tau neutrino production at CERN SPS
Presentation transcript:

I.Laktineh, IPNL 1 Nagoya, 2006 Studying the neutron quantum states in the gravitational field “using nuclear emulsion technique” Motivations Motivations Results obtained with CR39 Results obtained with CR39 Perspectives with emulsion Perspectives with emulsion

Nagoya, 2006I.Laktineh, IPNL2 "Let us consider another possibility, an atom held together by gravity alone. For exemple, we might have two neutrons in a bound state. When we calculate the Bohr radius of such an atom, we find that it would be 10 8 light years, and that the atomic binding energy would be Rydbergs. There is then little hope of ever observing gravitational effects on systems which are simple enough to be calculable in quantum mechanics." Brian Hatfield, in "Feynman Lectures on Gravitation" ; R.P. Feynman, F.B. Morinigo, W.G. Wagner, Ed. Brian Hatfield Addison-Wesley Publishing Company, 1995, p. 11

Nagoya, 2006I.Laktineh, IPNL3 Neutrons in gravitational field 1,41 2,46 3, Academic exercise

Nagoya, 2006I.Laktineh, IPNL4 Some history Solution of Schrödinger equation with linear potential 1928 : Solution of Schrödinger equation with linear potential 1928 : G. Breit, Phys Rev 32 (1928) 273 First attempts of ultra cold neutron storage at JINR (Dubna) in 1968 : First attempts of ultra cold neutron storage at JINR (Dubna) in 1968 : V.I. Luschikov et al., JETP Lett 9 (1969) , proposal to look for quantum energy levels using ultra old neutrons : 1976, proposal to look for quantum energy levels using ultra old neutrons : V.I. Luschikov, Physics Today 42 (1977) 51; V.I. Luschikov and A.I. Frank, JETP Lett 28 (1978) 559 First observations of the quantum states in a gravitational field at ILL/France in 1999 : First observations of the quantum states in a gravitational field at ILL/France in 1999 : V.V.Nesvizhevsky et al., Nature 415 (2002) 297; V.V.Nesvizhevsky et al., Nature 415 (2002) 297; Phys Rev D87 (2003)

Nagoya, 2006I.Laktineh, IPNL5 Institut Laue Langevin, Grenoble/France ILL ESRF LPSC/IN2P3 100 km from Lyon

Nagoya, 2006I.Laktineh, IPNL6 requirements To observe quantum states in gravitational field - neutral particle - long lifetime ultracold neutron - small mass (E<2 µeV, V<6 m/s) - weak energy (very low temperature) A well provided by -a mirror with: - elastic diffusion at least 99,99% - absorption negligible vertical - inelastic diffusion < speed -a gravitational field

Nagoya, 2006I.Laktineh, IPNL7 Experiment setup 10 cm Vh = few m/s Vv = few mm/s x

Nagoya, 2006I.Laktineh, IPNL8 Detector

Nagoya, 2006I.Laktineh, IPNL9 Neutrons in gravitational field 1,41 2,46 3, Academic exercise

Nagoya, 2006I.Laktineh, IPNL10 Wave function

Nagoya, 2006I.Laktineh, IPNL11 Procedure After the exposure to the UCN beam one has to - take out the Uranium (U235) layer - itch the CR39 to produce the tracks - scan the CR39 The observation of the quantum states of neutrons in gravitational field can then be obtained by “visualizing” the square wave function module using the neutron impact density. Many problems were to be addressed: -The Z zero position should be determined for the whole CR39 plate -The mechanics precision should be less than 1  But Itching leads to the CR39 curvature as well as scratches…

Nagoya, 2006I.Laktineh, IPNL12 Etching of uranium coating The etching may curve the detector in following manner: For this reason reference lines were used to estimate the curvature

Nagoya, 2006I.Laktineh, IPNL13 First results Nesvizhevsky et al., J. Phys. C40 (2005) 479 Results obtained by semi automatic scannig

Nagoya, 2006I.Laktineh, IPNL14 What the automatic scanning can provide? The semi-automatic scanning suffers from some drawbacks 1) It lasts about two months for each plate leading to uncertainties on the absolute position due to temperature and mechanics 2) Human intervention introduces subjective decisions which thus differ from one operator to another. 3) CR39 degradation with time if not properly protected

Nagoya, 2006I.Laktineh, IPNL15 What the automatic scanning can provide? At the French Scanning station we adapted the ESS to scan some of the exposed CR39. At the French Scanning station we adapted the ESS to scan some of the exposed CR39. The tracks are limited to the surface with a maximum penetration of 10 microns. The tracks are limited to the surface with a maximum penetration of 10 microns tomographic layers were used  1h/plate tomographic layers were used  1h/plate. All the tracks were found except those of large angle All the tracks were found except those of large angle (tg  > 5) (tg  > 5) Scratches dues to itching process simulated fake tracks Scratches dues to itching process simulated fake tracks “however automatic scanning can be controlled easily and quickly by a manual scanning” “however automatic scanning can be controlled easily and quickly by a manual scanning”

Nagoya, 2006I.Laktineh, IPNL16 What the automatic scanning can provide? In a new run with more statistics is expected CR39 is a good detector but its relatively bad surface planarity and the scratches left by the Uranium itching convince us to try to use emulsion. However emulsion density is about twice the CR39 one ( 3 vs 1.3) which means that ions will produce very short tracks CR39 is a good detector but its relatively bad surface planarity and the scratches left by the Uranium itching convince us to try to use emulsion. However emulsion density is about twice the CR39 one ( 3 vs 1.3) which means that ions will produce very short tracks (< 5 microns) which are hard to work out. (< 5 microns) which are hard to work out. Diluted emulsion of microns thickness can be of great help. Indeed the tracks can be seen from the side opposite to the U235 covered side limiting the scratches Diluted emulsion of microns thickness can be of great help. Indeed the tracks can be seen from the side opposite to the U235 covered side limiting the scratches effects effects In both cases tracking algorithms capable of finding horizontal tracks are on preparation. In both cases tracking algorithms capable of finding horizontal tracks are on preparation.

Nagoya, 2006I.Laktineh, IPNL17 Conclusion The automatic scanning development we engaged for OPERA can be a wonderful tool for amazing and very interesting application. Ultra cold neutrons is one of those topics that our scanning system can perform with negligible systematics. (quantum states, 5th force search, axions…) The emulsion can be a competitive and even better one but we need help from our Japanese colleagues.