qBOUNCE: a quantum bouncing ball gravity spectrometer

Slides:



Advertisements
Similar presentations
NEWTONIAN MECHANICS. Kinematic equations Frictional Force.
Advertisements

The photon, the quantum of light
Advanced Higher Unit 3 Nuclear Magnetic Resonance Spectroscopy.
An electromagnetic analog of gravitational wave memory Midwest Relativity Meeting Milwaukee, WI Oct. 25, 2013.
Lecture 14 Fission and Fusion. Elementary Particles. Nuclear Fission Nuclear Fusion Fundamental Interaction (Forces) Elementary Particles.
Cosmodynamics. Quintessence and solution of cosmological constant problem should be related !
Nuclear Physics UConn Mentor Connection Mariel Tader.
Structure of Atoms Rutherford's model of the atom was a great advance, however, it does not give an satisfactory treatment of the electrons. To improve.
Symposium on philosophy and the empirical sciences 16:15Welcome Jaakko Hintikka: Natural philosophy in quantum theory and quantum theory in natural philosophy.
ISP Astronomy Gary D. Westfall1Lecture 6 The Nature of Light Light and other forms of radiation carry information to us from distance astronomical.
Atomic Precision Tests and Light Scalar Couplings Philippe Brax IPhT Saclay « The Proton Radius Puzzle » Workshop, Trento November 2012 P.B and C. Burrage,
PHY 042: Electricity and Magnetism Introduction Prof. Pierre-Hugues Beauchemin.
Williams Research Gravity Pharis E. Williams 19 th Natural Philosophy Alliance Albuquerque, NM July, 2012.
Geneva, October 2010 Dark Energy at Colliders? Philippe Brax, IPhT Saclay Published papers :
Gravity at Micron Hartmut Abele. Hartmut Abele, Universität Heidelberg 2 Galileo in Pisa Objekt: Neutron Höhe: ~ 50  m Fallhöhe > 50  m Fallhöhe < 50.
CERN, January 2009 Evading the CAST bound with a chameleon Philippe Brax, IPhT Saclay.
1 Introduction to quantum mechanics (Chap.2) Quantum theory for semiconductors (Chap. 3) Allowed and forbidden energy bands (Chap. 3.1) What Is An Energy.
Planet Earth Force Laws in Nature - Dynamics kinds - sources - strengths - ranges - mediators.
1 Martin L. Perl SLAC National Accelerator Laboratory Holger Mueller Physics Department, University California-Berkeley Talk.
Fundamental Principles of General Relativity  general principle: laws of physics must be the same for all observers (accelerated or not)  general covariance:
Ch ; Lecture 26 – Quantum description of absorption.
The atom and its nucleus By the end of this chapter you should be able to: appreciate that atomic spectra provide evidence for an atom that can only take.
Atomic Models Scientist studying the atom quickly determined that protons and neutrons are found in the nucleus of an atom. The location and arrangement.
PART 1 MECHANICS. Chapter 1 : GENERAL INTRODUCTION ( MEASUREMENT) 1.1The Development of Science 1.1.1Definition of physics A science to study matter and.
1 Chapter 7 Atomic Structure. 2 Light n Made up of electromagnetic radiation n Waves of electric and magnetic fields at right angles to each other.
Strong fields and recycled accelerator parts as a laboratory for fundamental physics Joerg Jaeckel † M. Ahlers *,H. Gies x, J. Redondo**, A. Ringwald **
Quantum interferometric visibility as a witness of general relativistic proper time Bhubaneswar, 21 st December 2011 M. Zych, F. Costa, I. Pikovski, Č.
Anthropology Series In the Beginning How did the Universe begin? Don’t know!
Large extra dimensions and CAST Biljana Lakić Rudjer Bošković Institute, Zagreb Joint ILIAS-CAST-CERN Axion Training, , CERN Joint ILIAS-CAST-CERN.
The Higgs Boson Observation (probably) Not just another fundamental particle… July 27, 2012Purdue QuarkNet Summer Workshop1 Matthew Jones Purdue University.
Dark matter and hidden U(1) X (Work in progress, In collaboration with E.J. Chun & S. Scopel) Park, Jong-Chul (KIAS) August 10, 2010 Konkuk University.
M. Cobal, PIF 2006/7 Feynmann Diagrams. M. Cobal, PIF 2006/7 Feynman Diagrams 
“Planck 2009” conference Padova May 2009 Facing Dark Energy in SUGRA Collaboration with C. van de Bruck, A. Davis and J. Martin.
T. K. Ng (HKUST) The classical Universe Plan: This lecture: Review Pre-relativity/Quantum Mechanics picture of our physical universe You will learn some.
Monday, Feb. 7, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #6 Monday, Feb. 7, 2005 Dr. Jae Yu 1.Nature of the Nuclear Force Short Range Nature.
Dark Energy at Future Colliders: Testing the True Nature of Dark Energy in Black Hole Evaporations Jörg Jäckel Rencontres des Moriond March 2005 Michael.
XXXVI th Recontres de Moriond Very High Energy Phenomena in the Universe 22 January 2001 Ephraim Fischbach Department of Physics Purdue University, West.
Microwave Spectroscopy of the Autoionizing 5d 3/2 n l States of Barium Edward Shuman Tom Gallagher.
Spherical Collapse and the Mass Function – Chameleon Dark Energy Stephen Appleby, APCTP-TUS dark energy workshop 5 th June, 2014 M. Kopp, S.A.A, I. Achitouv,
ANTIHYDROGEN Gravitational States above material surface A. Voronin P.Froelich V.Nesvizhevsky.
Clare Burrage Université de Genève. Axion-like particles (ALPs) are scalars or pseudo-scalars which couple to photons Scalars Pseudo-scalars Assume no.
Rough Science We are stranded on a desert island, but since we are scientists, we will need to study our surroundings. The problem is, we don’t have our.
Standard Model of Particle Physics
Solutions of Schrodinger Equation
PHYS 3446 – Lecture #23 Symmetries Why do we care about the symmetry?
CHAPTER 6 Structure of the Atom
Atomic Models Scientist studying the atom quickly determined that protons and neutrons are found in the nucleus of an atom. The location and arrangement.
Gravitational Quantum States of Antihydrogen
Relativity + Quantum + Gravity
Detecting Chameleons in the Laboratory
The Standard Model of the Atom
General Physics (PHY 2140) Lecture 33 Modern Physics Atomic Physics
dark matter Properties stable non-relativistic non-baryonic
Quantum One. Quantum One So what is quantum mechanics, anyway?
Based on the work submitted to EPJC
Atomic Physics & Quantum Effects
cosmodynamics quintessence fifth force
THE GOD PARTICLE 1 Shashwat Mandal & Christian Bach 5
Lecture 29 Oscillation, linear superposition, and wave
Interaction of Radiation with Matter
Square Barrier Barrier with E>V0
The Standard Model The Standard Model combines the electromagnetic, weak, and strong forces (= interactions). Bosons with spin 1 communicate the force.
AS Physics Unit 1 1 Matter and Radiation Ks5 AS Physics AQA 2450
Chapter Fourteen: The Atom
Nuclear Energy Chapter 25 6/1/2019.
Advanced Pharmaceutical Analysis
Universal Forces.
A Swampland Update Cumrun Vafa Harvard University PASCOS 2019
Closing Remarks Developing the AEDGE Programme AEDGE CERN
Presentation transcript:

qBOUNCE: a quantum bouncing ball gravity spectrometer Presentation by Lucas van Sloten (s2297604) & Jelle Thole (s2183110), adaption of the talk of Hartmut Abele at the QU7 Symposium

Outline Introduction Theory Experimental Setup Results & Discussion Conclusion

Introduction qBOUNCE is an experiment of the University of Vienna, which uses Ultra Cold Neutrons (UCN) to probe the laws of gravity at the micron-scale These UCNs are used to do spectroscopy, which is the indirect measurement of energies through frequencies

Introduction Spectroscopy has in general been restricted to electromagnetic interactions (e.g. Atomic Clocks, Rabi Spectroscopy) Here instead of radiofrequency magnetic fields, mechanics is used From: https://www.khanacademy.org

Motivation Newton's gravitational law has not been tested at the sub- millimeter level, the qBOUNCE experiment allows for this This new test of Newton’s gravitational law grants possible insights into new physics UCNs allow for a very precise test of these physics

Motivation Fifth forces/String Theories The Equivalence Principle Possible Neutron Electric Charge Dark Matter Dark Energy

Fifth forces/String Theories Fifth forces that are only effective at small scales or folded up string-type extra dimensions at these scales can modify Newton’s potential in the following way: This alpha can be measured through a shift in the energy levels of the experiment

Weak Equivalence principle Using the two type of experiments of qBOUNCE we can measure both the characteristic energy and length scale of the experiment This allows for a test whether inertial mass and gravitational mass are the same, thus testing the weak equivalence principle

Dark matter Very light bosonic dark matter candidates can be detected through the macroscopic forces they mediate This force would show itself by a deviation from Newton’s law at short distances qBOUNCE looks for particles that mediate a spin- dependent force, axions in particular, directly These particles would induce an energy shift

Dark Energy Dark energy might be some kind of cosmological constant or it might be a quintessence type of scalar field A kind of scalar field that qBOUNCE looks for are chameleon fields Chameleon fields couple to matter, it is this coupling that qBOUNCE can test directly, through a shift in energy levels

Theory So basically we have these UCNs, which are subject to a linear gravity potential, leading to the following Schrödinger equation: Solutions of this Schrödinger equations are the Airy functions:

Airy Functions Now the Airy Functions for this gravitational potential have the following characteristic length, energy and time scale: The discrete quantum states this airy function solution has are the ones qBOUNCE uses for the spectroscopy

Quantum States From: arXiv 1510.03078

Two possible experiments Gravity Resonance Spectroscopy (GRS) Can be used to determine the energy differences between the states with high precision Quantum Bouncing Ball (QBB) Can be used to determine the distance scale of the wave packet

Ultra-Cold Neutron Source A reactor provides the neutrons due to a fission process Fast neutrons cant get through the bends, while neutrons that are too slow cant overcome gravity From: www.ILL.eu

Why neutrons? Neutrons are insensitive to electric fields The energy eigenstates are non-equidistant, this allows for resonance spectroscopy The lowest states are in the range of several pico-eV’s, giving very high accuracy

Experimental setup (GRS) I : Prepare system in lower bound states II : Excite the system with vibrating mirror III : Remove higher energy states again IV : Measure the surviving neutrons From arXiv 1512.09314

Experimental setup (GRS) Converts an energy measurement into a frequency measurement, which can be done with very high precision. The GRS method is analogous to Rabi’s method for measuring nuclear magnetic moments From arXiv 1512.09314

Simularities of GRS and Rabi’s magnetic resonance spectroscopy Rabi’s magnetic spectroscopy Gravity Resonance Spectroscopy

Experimental setup (QBB) I: Prepares the neutrons in a superposition of the lowest states II: The neutrons fall down a step which converts them into a superposition of higher states, which evolves in time III: The neutrons are detected with a position sensative detector I II III From Physics Procedia 17 (2011) 4-9

Experimental setup (QBB) As the neutron is reflected by the mirror its wave- function shows aspects of quantum interference As the neutrons are detected one obtains the probability distribution of the neutrons Region I Region II Simulated probability distribution of the QBB (From: arXiv 1510.03078)

Experimental difficulties The effects of the rough surface of the upper glass mirror on the quantum states are difficult to predict The QBB experiment requires position-sensitive detectors with high spatial resoltution and low background The step between the two mirrors in the QBB experiment needs to be very stable for several days The accuracy of the experiments is restricted by the strength of the UCN sources.

Results & Discussion From: arXiv 1510.03078

Axion Exclusion

Results & Discussion From: arXiv 1512.09134

Results & Discussion Transition frequency fore the transition: Transition frequency for the transition:

Fifth Force & Chameleon Fields Exclusion

Results & Discussion From: arXiv 1510.03078

From: arXiv 1510.03078

Quantum Bouncing Ball Up to now not enough precision to give definite results There is a need for more data analysis, which in oncoming years will probably give conclusive evidence on the weak equivalence principle

Conclusion/outlook The GRS and QBB experiments can contribute in answering a wide range of scientific questions Stronger UCN sources and better detectors will likely improve the accuracy in the future