richard packard- superfluid gyroscopes

Upload: proklus

Post on 06-Apr-2018

231 views

Category:

Documents


0 download

TRANSCRIPT

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    1/17

    Superfluid Gyroscopes

    Richard PackardUCB

    March 30, 2005

    LBNL

    Instrumentation Colloquium

    Why are sensitive gyroscopes useful?

    What superfluid properties are relevant?

    How does a superfluid gyro operate?

    Who are the Berkeley scientists involved?

    1

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    2/17

    Why?

    1. Rotational Seismology

    To detect rotational seismic waves causes by

    anisotropies in the crust inner core boundary. To

    determine torques on buildings due to seismic events.

    2. Geodesy

    To monitor small changes in the Earths rotation.

    Data used to investigate terrestrial processes and to

    update the GPS navigation system

    Presently monitored with VLBI array of radio

    telescopes. Resolution is better than 10-9E with 24hour averaging time. ( Hzradx sec104

    12)

    3. Inertial navigation

    To guide ships and planes inertially with precision

    equal to GPS. ( Hzradx sec10510

    )

    4. Tests of general relativity: frame dragging-gravito-

    magnetic field of the Earth. (similar requirements

    to geodesy)

    2

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    3/17

    What?

    Superfluid (Quantum fluid)

    Finite number of the particles in a single quantum

    state

    4He T=2.17K

    3He Tc=10-3K

    Simple wave function

    ie=

    Apply current operator and find: sss vm

    j ==h2

    where

    = mvs

    h

    = mhndlvs Quantized vortex lines (Feynman,

    1954)

    3

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    4/17

    How?

    1.4He phase slip gyroscope

    The rotation forces the fluid to move (almost) like a

    rigid body, thus creating a phase gradient.

    == 02;0 lvRRdlv as

    ( )l

    Al

    RRva

    rr== 22

    if R~50cm and , velocity amplification is 10nml 50~ 7

    4

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    5/17

    How can we monitor flow through the small

    aperture?

    Phase slip concept:(Anderson 1964)

    Superfluid accelerates until reaching a

    critical velocity at which a (thermally

    activated) phase slip occurs.

    velocity decrement is:

    ml

    hvs =

    5

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    6/17

    Phase slip gyroscope

    Single quantized phase slips

    Staircase pattern

    6

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    7/17

    gyro on a chip

    Reorientation with respect to Earths axis

    T~0.3K

    7

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    8/17

    Multiturn gyro

    The 4He phase slip gyro is ultimately limited by the kBT

    fluctuations responsible for the phase slip nucleation

    process.

    8

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    9/17

    2. The3He Quantum Interference Gyroscope

    Relies on the dc-Josephson effect

    L

    PL

    | |

    R

    PR

    dc-Josephson equation

    = sincII

    ac-Josephson equation (a disguised F=ma )

    hh

    Pm

    dt

    d =

    = 3

    2

    For fixed P=PL-PRthe current oscillates at frequency

    h

    Pmfj

    = 3

    2

    9

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    10/17

    Arrays (65x65=4225) of small (~60nm) apertures

    behave as weak links for 3He. T

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    11/17

    Interference gyroscope

    The effective critical current of the entire device is

    modulated by the rotation flux threading the ring (see

    Feynman vol 3 chap 21)

    3

    *

    2

    2cos2

    mh

    AII cc

    rr

    =

    11

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    12/17

    A prototype gyro based on this principle in Saclay finds

    Hzx E /1053

    for a 6cm2 device.

    The 3He interference gyroscope is not limited by

    thermal fluctuations and is potentially the most

    sensitive gyroscope: BUT it requires 1mK technology

    which is not user friendly to gyro users.

    12

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    13/17

    4He quantum whistle gyroscope

    (A work in progress)

    Discovery 2004: Near T~2.1K

    +

    =

    = Ts

    P

    h

    m

    h

    mf

    j

    44

    0 1 2 30

    1

    2

    3

    4

    5

    (1030

    J)

    Frequ

    ency(kHz)

    13

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    14/17

    Amplitude fluctuation noise seems ~ 10-3! Thermal

    fluctuations seem suppressed by 1/N where N=4225.

    A proposed4He quantum whistle gyroscope

    Rotation induces a phase shift between the two aperture

    arrays. This leads to interference at the microphone.

    4

    4

    2

    1

    4

    2

    1 m

    ARR

    mldv

    mld s

    h

    rr

    h

    rr

    h

    rr ====

    14

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    15/17

    Features:

    Low noise of the 3He interferencegyroscope

    Cryocooler temperatures (T~2K)

    Possible turn key operation. Noadvanced cryogenic techniques required

    by the user.

    15

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    16/17

    Summary

    Quantum phase coherence in superfluidscan detect absolute rotation

    In 4He quantized phase slip phenomena candetect rotation. Operating temperature

    (T~0.3K) leads to simpler cryogenics but

    thermal noise limits rotation resolution

    In 3He a sine-like current-phase relationleads to the superfluid analog of a dc

    SQUID. Potentially very low noise but high

    tech cryogenics. (T

  • 8/3/2019 Richard Packard- Superfluid Gyroscopes

    17/17

    Who?

    Keith Schwab

    Neils Bruckner

    Ray Simmonds

    Alosha Marchenkov

    Seamus Davis

    Stefano Vitale

    Emile Hoskinson

    Yuki Sato

    Supported by NSF and NASA

    (Alternate ideas for support sponsors

    appreciated)

    17