A passion for precision Theodor W. Hnsch Max-Planck-Institute for - - PowerPoint PPT Presentation

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A passion for precision Theodor W. Hnsch Max-Planck-Institute for - - PowerPoint PPT Presentation

Stockholm 2005 A passion for precision Theodor W. Hnsch Max-Planck-Institute for Quantum Optics, Garching, and Ludwig-Maximilians-University, Munich Stockholm, Dec. 8, 2005 University of Heidelberg, 1964 - 1970 Ali Javan Bill Bennett


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Stockholm 2005

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Max-Planck-Institute for Quantum Optics, Garching, and Ludwig-Maximilians-University, Munich

Theodor W. Hänsch

A passion for precision

Stockholm, Dec. 8, 2005

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Peter Toschek

University of Heidelberg, 1964 - 1970

Helium-Neon gas lasers Saturation spectroscopy without Doppler broadening Quantum interference in coupled 3-level systems

Christoph Schmelzer

John Hall . . . Ali Javan Bill Bennett Vladilen Lethokov Venia Chebotaev

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Peter Toschek

University of Heidelberg, 1964 - 1970

Helium-Neon gas lasers Saturation spectroscopy without Doppler broadening Quantum interference in coupled 3-level systems

Christoph Schmelzer

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Arthur L. Schawlow

Stanford University, 1970 - 1986

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T.W.H., Optics and Photonics News February 2005

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x 15 000

T.W.Hänsch, I.S. Shahin, and A.L. Schawlow, Nature 235, 63 (1972)

Spectrum of H

Hydrogen Balmer Spectrum

T.W. Hänsch, I.S. Shahin, and A.L. Schawlow, Nature 235, 63 (1972)

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cesium clocks

  • ptical

atomic clocks

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Hydrogen 1S-2S two-photon transition

(natural line width: 1.3 Hz)

T.W. Hänsch, S.A. Lee, R. Wallenstein, and C. Wieman, Phys. Rev. Lett. 34, 307 (1975), ...

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Max-Planck-Institute for Quantum Optics, Garching, and Ludwig-Maximilians-University, Munich, 1986 -

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Wasserstoff Spektrum

!"/" = 4.3 10 530 Hz @ 243 nm

#13

2S signal [cps]

Hydrogen 1S-2S resonance

d e t u n i n g [ k H z @ 2 4 3 n m ]

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R y d b e r g c

  • n

s t a n t R

∞ T h e R y d b e r g c

  • n

s t a n t i s d e t e r m i n e d p r i m a r i l y b y c

  • m

p a r i s

  • n
  • f

t h e

  • r

y a n d e x p e r i m e n t f

  • r

e n e r g y l e v e l s i n h y d r

  • g

e n a n d d e u t e r i u m . νH ( 1 S1/2 − 2 S1/2 ) = 3 4 R∞ c

 

1 − me mp + 1 1 4 8 α2 − 2 8 9 α3 π l n α−2 − 1 4 9

  • α

Rp λC

2

+ · · ·

 

D i r a c ( 1 S1/2 − 2 S1/2 ) = 2 4 6 6 6 8 5 4 1 1 8 k H z Q E D ( 1 S1/2 − 2 S1/2 ) = − 7 1 2 4 7 3 6 k H z O t h e r ( 1 S1/2 − 2 S1/2 ) = · · · νH ( 1 S1/2 − 2 S1/2 ) = 2 4 6 6 6 1 4 1 3 1 8 7 k H z

Hydrogen 1S-2S two-photon transition

A cornerstone in the least squares adjustment of the fundamental constants (P. Mohr, B. Taylor, NIST)

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A dream... (Ali Javan, 1963)

Extend microwave frequency counting techniques into the optical region.

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Garching frequency interval divider chain (1997)

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Optical frequency comb

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Optical Frequency Comb frequency

beat note detector beam splitter

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Optical Frequency Comb Synthesizer

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fm = m frep + foffset

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femtosecond laser frequency comb synthesizer

  • 100 000 ultra-stable lasers at once
  • revolutionary optical wave meter
  • frequency counter from DC to UV
  • clockwork for optical atomic clocks
  • ultra-stable microwave source
  • . . .
  • enabling tool for fundamental measurements
  • arbitrary optical waveform synthesizer?
  • . . .
  • source of phase-stabilized femtosecond pulses
  • key to attosecond physics
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This is a simple idea! What took so long?

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Stanford, 1978: 500 GHz laser frequency comb

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phase velocity group velocity

carrier-envelope phase slips

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carrier-envelope phase slips

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carrier-envelope phase slips and offset frequency

f0 = (∆ϕ/2π)fr

J.N. Eckstein, Ph.D. Thesis, Stanford University, 1978

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D.E. Spencer, P.N. Kean, and W. Sibbett, Opt. Lett. 16, 42 (1991)

Kerr lens mode-locking

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femtosecond white light continuum

intensity-dependent refractive index: self-phase-modulation, self-focusing, shock wave formation, . . .

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?

Can two white light pulses interfere?

  • M. Bellini and T.W. Hänsch, Opt. Lett. 25, 1049 (2000)

Florence, Italy, February 1997

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LENS, Florence, Italy, February 1997 camcorder electronic notebook

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detection of comb lines with beat signals

  • Dr. Thomas Udem
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Testing the uniform spacing of the comb lines Experimental uniformity: 3 x 10-17

  • Th. Udem, J. Reichert, R. Holzwarth, and T.W. Hänsch, Opt. Lett. 24, 881 (1999)
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1998: first absolute frequency measurement with a laser comb

Hydrogen 1S-2S spectrometer

70 THz comb

June 1999: Paris Cs fountain clock October 1998: HP Cs clock

first femtosecond pulses with controlled carrier-envelope phase

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1s-2S frequency

f(1S-2S) = 2 466 061 413 187 103 (46) Hz (hyperfine centroid)

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Octave-spanning frequency combs

“Photonic Crystal Fiber”

J.C. Knight, W.J. Wadsworth, P. St. Russel University of Bath, UK

„Rainbow Fiber“

(Lucent Technologies, 1999)

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  • R. Holzwarth et al.,
  • Phys. Rev. Lett 85, 2264 (2000)
  • D. Jones et al.,

Science 288, 635 (2000) T.W. Hänsch, Witnessed disclosure (March 30, 1997)

CEO CEO

Self-referencing frequency comb

fCEO

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Single-Laser Optical Frequency Comb Synthesizer

Ti:Sapphire mode-locked laser

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frequency combs, 2005

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Science, 303, 1843 (2004)

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measuring the frequency of hydrogen with a laser comb

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2003: Hydrogen 1S-2S spectrometer

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Hydrogen spectrometer, February 2003

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PHARAO transportable cesium fountain clock

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Frequency comb synthesizer

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  • M. Fischer et al., PRL 92, 230802 (2004)
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Hydrogen 1S-2S frequency

  • Feb. 2003: f(1S-2S) = (2 466 061 102 474 851 34) Hz

relative uncertainty: 1.4 x 10 -14 A difference of (-29 57) Hz in 44 months equals a relative drift of the 1S-2S transition frequency of (3.2 6.3) x 10 per year

  • 15
  • 14

June 1999: f(1S-2S) = (2 466 061 102 474 870 46) Hz relative uncertainty: 1.9 x 10 (F=1 to F!=1 hyperfine component)

± ±

± ±

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M.T. Murphy, J.K. Webb, and V.V. Flambaum, MNRAS 345, 609 (2003)

Further evidence for a variable fine structure constant from KECK/HIRES QSO absorption spectra

˙ α/α ≤ +(6.4 ± 1.35) × 10−16yr−1

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Limits on the time variation of the electromagnetic fine-structure constant in the low energy limit from absorption lines in the spectra of distant quasars

  • R. Srianand, H. Chand, P. Petitjean, and B. Aracil, PRL 92, 121302 (2004)

−2.5 × 10−16 ≤ ˙ α/α ≤ +1.2 × 10−16yr−1

M.T. Murphy, J.K. Webb, and V.V. Flambaum, MNRAS 345, 609 (2003)

Further evidence for a variable fine structure constant from KECK/HIRES QSO absorption spectra

˙ α/α ≤ +(6.4 ± 1.35) × 10−16yr−1

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hydrogen

Hydrogen, 1999-2003: M. Fischer et al., PRL 92, 230802 (2004)

˙ α/α

  • 10−15yr−1

˙ µCs/µCs

  • 10−14yr−1
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hydrogen hydrogen mercury+

Mercury+, 2000-2002: S. Bize et al., PRL 90, 150802 (2003)

˙ α/α

  • 10−15yr−1

˙ µCs/µCs

  • 10−14yr−1

Hydrogen, 1999-2003: M. Fischer et al., PRL 92, 230802 (2004)

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hydrogen

Mercury+, 2000-2002: S. Bize et al., PRL 90, 150802 (2003)

˙ α/α

  • 10−15yr−1

˙ µCs/µCs

  • 10−14yr−1

Hydrogen, 1999-2003: M. Fischer et al., PRL 92, 230802 (2004)

ytterbium+

Ytterbium+, 2000-2003, E. Peik et al., PRL 93, 230802 (2004)

hydrogen mercury+

1σ area

˙ α/α = (−0.3 ± 2.0) × 10−15yr−1 ˙ µCs/µCs = (2.4 ± 6.8) × 10−15yr−1

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Optical clock - some candidates

Laser-cooled trapped ions Hg+, In+, Yb+, Sr+, Ca+, ... Cold neutral atoms: H, Ca, Sr, Yb, Ag, ... Molecules: I2, C2H4, ...

Paul trap Atom chip Optical lattice Atomic fountain

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Accuracy of clocks

  • ptical

atomic clocks

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Applications for (better) Atomic Clocks

  • Precision Spectroscopy
  • Time and frequency metrology
  • Clock synchronization over large distances
  • Very long baseline interferometry (VLBI)
  • Higher performance satellite navigation (Galileo)
  • Precise tracking of remote space probes
  • Telecommunication, network synchronization
  • Variability of earth"s rotation
  • Geodesy with millimeter precision
  • Pulsar periods
  • Test of special and general relativity
  • Check constancy of fundamental constants
  • ....
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curiosity-driven research

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Towards frequency combs and ultraprecise spectroscopy in the extreme ultraviolet

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Generation of high harmonics

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Can two high harmonics pulses interfere?

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Experiments at Lund Laser Center:

  • R. Zerne et al., Phys. Rev. Lett. 79, 1006 (1997)
  • M. Bellini et al., Phys. Rev. Lett. 81, 297 (1998)
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xenon gas jet sapphire

  • utput

coupler XUV out input pulses build-up cavity High harmonic generation at 112 MHz

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Intra-cavity high harmonic generation

  • Ch. Gohle et al., Nature 436, 234 (2005)

injected: 22 fs pulse duration, 0.65 W average, 200 kW peak circulating: 27 fs pulse duration, 45 W average, 15 MW peak #

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High harmonic generation at 112 MHz

  • Ch. Gohle et al., Nature 436, 234 (2005)
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Thomas Udem Christoph Gohle Maximilian Herrmann

60 nm

He+

Two-photon spectroscopy of He+ 1S-2S with XUV frequency comb

Helium ion

in Paul trap

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  • M. Abgrall, P. Adel, J. Alnis, T. Andreae, R.G. Beausoleil,
  • M. Bellini, S. Bergesson, L.A. Bloomfield, U. Boesl, C. Bordé,
  • A. Clairon, B. Couillaud, S.M. Curry, P. Dabkiewicz,
  • K. Danzmann, J.N. Eckstein, K.S.E. Eikema, P. Fendel,
  • A. Ferguson, M. Fischer, C.J. Foot, H. Geiger, H. Gerhardt,
  • C. Gohle, J.E.M. Goldsmith, B. Gross, M. Haas, J.L. Hall,
  • A. Hemmerich, M. Herrmann, T. Heupel, E.A. Hildum,
  • R. Holzwarth, A. Huber, U. Jentschura, R. Kallenbach,

S.G. Karshenboim, N. Kolachevsky, M. Kourogi, F. Krausz,

  • P. Kubina, P. Laurent, S.A. Lee, D. Leibfried, J.C. Knight,
  • W. König, A. Matveev, D.A. McIntyre, D. Meschede, T. Mukai,

M.H. Nayfeh, M. Niering, K. Pachucki, A. Pahl, P. Pokasov,

  • M. Prevedelli, J. Reichert, L. Ricci, P.St.J. Russel, C. Salomon,

A.L. Schawlow, F. Schmidt-Kaler, D. Schropp, H.A. Schüssler,

  • S. Seel, G.W. Series, I.S. Shahin, P. Toschek, R. Teets,
  • W. Vassen, V. Vuletic, W.J. Wadsworth, R. Wallenstein, J. Walz,

E.Weber, M. Weitz, C. Wieman, R. Wynands, Th. Udem,

  • C. Zimmermann, M. Zimmermann
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  • M. Abgrall, P. Adel, J. Alnis, T. Andreae, R.G. Beausoleil,
  • M. Bellini, S. Bergesson, L.A. Bloomfield, U. Boesl, C. Bordé,
  • A. Clairon, B. Couillaud, S.M. Curry, P. Dabkiewicz,
  • K. Danzmann, J.N. Eckstein, K.S.E. Eikema, P. Fendel,
  • A. Ferguson, M. Fischer, C.J. Foot, H. Geiger, H. Gerhardt,
  • C. Gohle, J.E.M. Goldsmith, B. Gross, M. Haas, J.L. Hall,
  • A. Hemmerich, M. Herrmann, T. Heupel, E.A. Hildum,
  • R. Holzwarth, A. Huber, U. Jentschura, R. Kallenbach,

S.G. Karshenboim, N. Kolachevsky, M. Kourogi, F. Krausz,

  • P. Kubina, P. Laurent, S.A. Lee, D. Leibfried, J.C. Knight,
  • W. König, A. Matveev, D.A. McIntyre, D. Meschede, T. Mukai,

M.H. Nayfeh, M. Niering, K. Pachucki, A. Pahl, P. Pokasov,

  • M. Prevedelli, J. Reichert, L. Ricci, P.St.J. Russel, C. Salomon,

A.L. Schawlow, F. Schmidt-Kaler, D. Schropp, H.A. Schüssler,

  • S. Seel, G.W. Series, I.S. Shahin, P. Toschek, R. Teets,
  • W. Vassen, V. Vuletic, W.J. Wadsworth, R. Wallenstein, J. Walz,

E.Weber, M. Weitz, C. Wieman, R. Wynands, Th. Udem,

  • C. Zimmermann, M. Zimmermann
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Tack så mycket Tack så mycket

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