m-c. angoninand ph. tourrenc- cold atom interferometer in a satellite : orders of magnitude of the...

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    Cold atom interferometer

    in a satellite :orders of magnitude of the

    tidal effects

    M-C. Angonin and Ph. Tourrenc

    ERGA / LERMA

    Universit Pierre et Marie CurieObservatoire de Paris

    and

    CNRS

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    Goal

    atomic wave interferometer in a free falling satellite

    + telescope pointing toward far away star

    acceleration and rotation

    general parametrized description

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    Principle

    * Determination of the local metric to the third order

    comoving with an idealized device

    * Define someperturbations* Compute thephase shift

    * Order of magnitude of each term

    * Select the terms that cannot be modelized

    norcancelled

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    Do we have a possibility to observe

    Lense-Thirring effect ?

    If Yes : How shall we proceed ?

    If No : Why not ?

    And what can be done presently ?

    The case of HYPER

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    Atomic Sagnac Unit

    2 Ramsey-Bordinterferometers

    Shift between the two centres : OSOs

    HYPER

    Spin around u 1 : angle t ,

    angular velocity ddt

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    Local metric

    00 1 2U

    0k2

    r3J r 1

    2U w

    ds2 g00 dt2 2g0kdx

    kdt gikdxidx k

    Geometrical units : G c 1

    U)(h ikikikik 21+=+=

    Lense-Thirring

    21 J2Mr Rr UU P2 cos S M,P, etc,

    J1

    J*

    1

    82

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    Parameters

    MrOrbital velocity : 2.5105( HYPER)O1

    rl=Size of the orbit :

    : X d lSize of the experimental set -up 60 cm

    vAtom velocity :

    Orders of magnitude

    Eccentricity of the orbit < l1/2 O1

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    )()0( , kuu

    = Tetrad comoving with the satellite

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    The metric comoving with the set-up (Li & Ni 1979)

    locityangular velocal:onacceleratilocal:

    r

    r

    a

    ab 0

    g 0 0 1 2 a x a x

    2

    x

    2

    U, i k xi x k 1

    3U, i k j x

    i x kx j

    g 0 k xk

    23 R 0 i k j x i x j

    gm n m n1

    3R i m j n x

    i x j .

    + d2 l3 O6

    + d2 l5/2 O5

    + d2 l2 O4

    measured by comovingaccelerometers and gyroscopes

    0 T d S TSpin

    Aberration + deflexion

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    B 2 t

    t

    t dt with

    The phase shift on one atomic beam(WKB approximation L & T 1976)

    t h 00 2h0kvatk h kjvat

    k vatj

    and matomc2

    Lense-Thirring effect c Jr3

    10 14 rad s 1( HYPER)

    ccuracy on Lense Thirring phase shift within the present framework :

    %)( 182 vMJ

    d

    HYPER

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    can be calculated at the required accuracywith the assumption (??)

    O6accuracy of the present expansion

    xxrr // 410r

    d2 l3mod

    2J

    r3

    3 J n

    r3 n1 M

    4 r2 n w x vg A Lense-Thirring

    2 u 1 x vat B spin of the satellite

    2

    M

    r2 u 1 n x v at 2 u 1 a x v at C aberration

    M

    r3x2 n

    23 x D tidal effect

    2 a OS x E residual acceleration

    v at atomic velocity 20 cm s 1 O2 c

    1 w : coupling to a preferred frame

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    First conclusion :

    Tidal effects on HYPER

    Perfectly symmetric interferometers superimposed

    with precision < 2 nm

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    SunJupiterEarth

    10-14 rad.s-1 10-12 rad.s-1 10-13 rad.s-1 Lense-Thirring

    18 % 1.5 % 90 %Accuracy

    2 10-12 10-12 6 10-13Tidal effects

    U/U < l d O2

    No !

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    We measure and11

    2

    212

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    Spinning satellite

    : spin angular position: orbital angular position

    1 2vatc 2

    2 cTD2

    r

    K1 K2

    Lense-Thirring ; 2

    Geometry of the set-up 2 ; 2; 2+; 22 ;2+2

    Change of the local field 2; 2+; 22 ;2+2

    during the flight time of the atoms

    Preferred frame

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    Conclusion

    Spinning the satellite

    A polar, circular orbit with (?)

    The high sensitivity to geometrical defect.

    de Sitter/Thomas effect,54

    1 10,10

    2/ =

    Bibliography

    Angonin et al., GRG, 2004

    Tourrenc et al., GRG, 2004

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    = Tetrad comoving with the satellite)()0( , kuu

    M R J J J 2 r

    4,4 mm 6400 km 145 cm 2 10 3 10 6 7000 km

    Geometry of the set up2 T 2

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    2 + 2

    2 2

    2

    cteM

    r 2cos 2

    3Mr 1 sin2

    4 sin 22

    r cos 23

    r

    3Mr

    1 sin 2

    8sin 2 2

    2

    r cos 2 23

    r

    Mr 4

    1 sin 2 sin 2 2

    Mr 4

    1 sin 2 sin 2 2

    3Mr

    1 sin 2

    8sin 2 2

    2

    r cos 2 23

    r

    : spin angular position

    : orbital angular position

    Geometry of the set-up

    Change of the local fields during

    the flight time of the atoms2 cTD2

    r 1017

    1 2v atc 2

    2 cTD2

    rK1 K2

    r 6 10

    10v atTD cTD

    r2 r

    3/2

    1010

    v t 2 cTD2

    2 cT 2

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    2

    2 +

    2vat

    r 2 1024

    1 2v atc 2

    2 cTDr

    K1 K22 cTD

    r10 17Lense-Thirring

    Preferred frame

    r 6 1010

    Geometry

    vat

    r 1014

    Aberration

    Change of the localfields during the flight

    time of the atom

    2vatJ

    r2

    cos J32

    M

    rcos sin sin

    1

    r

    6vatJ

    r2 cos 2 J 2

    M

    r 1 sin cos cos 2

    32

    M

    rcos 1 sin

    2sin 2

    1

    r

    vatM

    r 1w

    3 2 2 sin sin

    2

    M

    r1 sin cos cos 2

    3M

    2 rcos 1 sin

    2sin 2

    1

    r

    10 10