Temperature Dependent Energy Levels of Electrons...

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Temperature Dependent Energy Levels of Electrons on Liquid Helium Royal Holloway University of London Bill Bailey, Parvis Fozooni, Phil Glasson, Peter Frayne, Khalil Harrabi, Mike Lea. + Eddy Collin, Grenoble

Transcript of Temperature Dependent Energy Levels of Electrons...

Page 1: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature Dependent

Energy Levels of Electrons

on Liquid Helium

Royal Holloway

University of London

Bill Bailey, Parvis Fozooni, Phil Glasson, Peter Frayne,

Khalil Harrabi, Mike Lea.

+ Eddy Collin, Grenoble

Page 2: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave absorption

Sweep DC

Modulation AC

WaveguidePutley detector

(InSb bolometer)

Cell

56 mm2.1

mm

Electrodes

Lock-in

1 kHz

Ez

+

CW microwaves

(165 GHz - 220 GHz)

ERF

e-

Cell

2

Segmented

Corbino

Polarising

Grid

Page 3: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave System 1Microwaves for Electrons on Helium

Rydberg

resonance

190 GHz

Ez = 10.7 kV/m

PIN

modulator

90 7.5 GHz

30 mW

Phase locked

to 10 MHz

180 15 GHz

5 mW2 ns risetime

Isolator Amplifier Attenuator

Mechanical

Chopper

300 Hz

Cryostat

WR10

Waveguide

WR5

Mode transformer

+ 7dBTuning

WR28

SS

3

Frequency

Doubler

Reference

Cavity

Tuning

Gunn

Oscillator

Peter Frayne

Royal Holloway

Page 4: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave System 2Microwaves for Electrons on Helium

CellFundamental

Waveguide

WR 5

Bandpass

Filter

f = 1 GHz

1 dB loss

Mylar

window

+ In O-ring

Glass/metal

seal

Tuning

1.3 K

0.1 K

0.6 K

4.2 K

WR28

SS

Options

• Thermal filter

• Thermal break

WR 5

Microwaves

Cryostat

WR28

SS

4

Chip

Page 5: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Rydberg states – liquid 4He

5

2m

1m

0for

0for )(4

)(

0

0

2

0

zV

zbz

ZezU

f12 = 119.3 GHz0for 4

)(0

2

0

zz

ZezU

Image charge

)(4

Z

2m

RE e

m

Stark tuning U(z) = U0(z) + eEzz

Experiment for Ez = 0:

f12 = 125.9 GHz at 1.2 K

Grimes et al:

Page 6: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Stark Tuning Resonance

Brown, Grimes,

Zipfel, 1976

120

140

160

180

200

220

240

0 5 10 15 20

Ez

(kV/m)

189.6 GHz

10.6 kV/m

5.06 GHz/(kV/m)

f 12

(GH

z)

1.5 K

Low power

Resonant frequency f12 increases with EZ

Ground state to first excited Rydberg state

6

4He

Page 7: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature dependent resonance

Low temperatures

Inhomogenous broadening

Medium temperatures

Inhomogenous broadening

convoluted with a Lorentzian

High temperatures

Lorentzian

Resonance frequency decreases

as the temperature increases

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0

0.2

0.4

0.6

0.8

1

21.8 22 22.2 22.4 22.6

Collin et al (2005)Figure 8

Absorp

tion

V (volts)

1.004 K

0.855 K

0.553 K

0.304 K

1 GHz

189.6 GHz

Page 8: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Inhomogeneous broadening

8

100 MHz

0.1 0.08 0.06 0.04 0.02 00

0.2

0.4

0.6

0.8

1

Voltage/V

Abso

rpti

on

Disk

LorentzianDisk + edges

Data at 0.25 K

• Lineshape independent

of T < 0.5 K

• Inhomogeneous broadening

Peaks from Ez variation (0.3%)?

• Non-parallel disk electrodes:

Parabolic lineshape

• 8 m across 50 mm

• = 0.17 mrad = 35” arc

• Lorentzian contribution small?

Non-parallel electrodes

Page 9: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

21.8 21.9 22 22.1 22.20

0.2

0.4

0.6

0.8

1

Convolution

9

Lorentzian Cell

-response

Measured

21.8 21.9 22 22.1 22.20

0.2

0.4

0.6

0.8

1

21.8 21.9 22 22.1 22.20

0.2

0.4

0.6

0.8

1

vvLvVGVS d),()()(G(V)Inhomogeneous

broadeningIntrinsic

linewidth

Convolution

Output = Lorentzian L(V) Cell response G(V)

0.9 K0.3 KFit

volts volts volts

Fit γ = 106 MHz

22

/),(

vvL

v=V-V0

Use lineshape at 0.3 K as a template

Convolute with a Lorentzian

Fit linewidth to data (T)

Page 10: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave absorption at 189.6 GHz

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Convolution

21.9 21.95 22 22.050

0.2

0.4

0.6

0.8

1

T = 0.498 K

= 0.001 V

= 2.9 MHz

volts

4He

0.3 K

21.9 21.95 22 22.050

0.2

0.4

0.6

0.8

1

T = 0.602 K

= 0.0026 V

= 7.6 MHz

volts

0.3 K

21.85 21.95 22.05 22.150

0.2

0.4

0.6

0.8

1

T = 0.855 K

= 0.0165 V

= 49 MHz

0.3 K

21.7 21.9 22.1 22.30

0.2

0.4

0.6

0.8

1

T = 1.004 K

= 0.098 V

= 288 MHz

volts 0.3 K

Page 11: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave linewidth (T)

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Theory:

T. Ando, J.Phys.Soc Japan, 44,765 (1976)

gasβbNaT Ripplon Gas atom

Scattering

β = 1.6

[H. Isshiki et al.J.Phys.Soc Japan (2007):

β = 2.1 (3He); 1.6 (4He)]

β = 1

4He

Page 12: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature dependent linewidth

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H. Isshiki et al.J.Phys.Soc Japan 76, 094704 (2007)

β = 2.1 (3He); 1.6 (4He)

gasβbNaT

Page 13: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature dependent resonance f12

f12 (T) = f12 (0) f12 (T)

800 MHz at 1 K

f12 (T) T5/2 or

T7/3

b

13

Ripplons?

f12 = 189.6 GHz

Low power limit

4He

Page 14: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature dependent resonance

2-ripplon processes:

Lamb shift

Ripplon induced Lamb shift

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Theory:

Mark Dykman,

Denis Konstantinov

et al (2010)

Electron density

0.67 1011 m–2 (▲)

1.0 (▼)

1.5 (♦)

1.7 (●)

2.4 (■)

● - various

4He

f12 (T) = f12 (0) f12 (T)

+ Vapour

Theory

Page 15: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Density dependence of holding field

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)ε/(

)2(

)1ε(ε)ε/( 0 ddD

dDne

ddD

VE z

z

Dd

Vz

D -2d =

D -2d =

Extrapolated to T = 0

Page 16: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Temperature dependence of f12

16

RIKEN4He 3He

Page 17: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Microwave absorption - Coulomb shift

Resonance frequency shifts with

• Power absorbed

• Excited state population

• Electron temperature Te

• Electron density

17

D. Konstantinov et al. PRL 103, 096801 (2009)

D. Konstantinov et al. PRL 98, 235302 (2007)

Ultra-hot Electrons on Liquid 3He: Te < 27 K

Power frequency Rabi

3He

3He

za

f12

Page 18: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Optical bistability in microwave absoprtion

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D. Konstantinov et al. PRL 103, 096801 (2009)

High-powers: Hysteresis in conductivity

( zzz

m

dVVVV )()(1

)'Im(

High-powers: A.C. modulation (10 mV at 1 – 10 kHz)

Complex microwave lineshape

Vmod

t

0.9 0.95 1 1.05 1.10

0.1

0.2

0.3

0.4

0.5

Vz

)( zV

)( zV

3He

Differential

absorption

α‛ = dα/dVz

α

f12 = 189.6 GHz

1.3 K

α

α

Page 19: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Hysteresis Complex Lineshape

21.4 21.6 21.8 22 22.2 22.40.001

0

0.001

0.002

T = 0.9 K Re()

Im()

21.4 21.6 21.8 22 22.2 22.40.001

0

0.001

0.002

Vz (V)

T = 0.5 K

Re()

Im()

19

0

0.05

0.1

0.15

0.97 0.98 0.99 1 1.01 1.02 1.03

E

Re(Line)

Im(Line)

( zzz

m

dVVVV

V

)()(

21

2)Im( off

mV

VV

21)Im( max

off

MHz 50 mV 202 mV

0

1

2

3

1 10 100 1000

o

ff

Power (mV)

)Re( off

)Im( off

T = 0. 5K4He

Inhomogeneous power broadening

Inhomogeneous Coulomb broadening

4He

Page 20: Temperature Dependent Energy Levels of Electrons …lyon/Electrons-on-Helium-Workshop/Lea.pdf•Electron temperature T e •Electron density 17 D. Konstantinov et al. PRL 103, 096801

Conclusions

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• Temperature dependent Rydberg levels

• Inhomogeneous broadening

• Enhanced Ando linewidth

• Microwave absorption bistability (hysteresis)