Stabilizing Carrier-Envelope Phase in AMO Physics Research
Stabilizing Carrier-Envelope Phase
Brett Chrisler
Kansas State University REU 2015
Mentor: Dr. Vinod Kumarappan
Atomic, Molecular, and Optical (AMO) Physics
Mentor: Dr. Vinod Kumarappan
Postdoctoral: Rajesh Kushawaha
Graduate: Huynh Lam
Kansas Light Source (KLS) located in the James R. Macdonald
Laboratory at Kansas State University
KLS Laser
800 nm wavelength
3 millijoules/pulse at 25 femtoseconds/pulse
2kHz
Project Background
Peak Electric Field
Peak Pulse Envelope
Carrier-Envelope (CE) Phase
[1] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating-
Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009.
Abstract. 4. Print.
Offset
Mode-Locked Lasers
Sequences of pulses on the order of femtoseconds result.
Each mode is set apart at the same interval leading to a frequency comb.
Crystal (e.g. Ti:Sapphire) starts the lasing process and creates a gain spectrum
and allows modes under this spectrum specifically to become excited.
[3] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating-
Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009.
Abstract. 9. Print.
Offset Frequency
Phase velocity -> Carrier-Wave
Not the same = Carrier-Envelope Phase Shift
Group velocity -> Envelope
[4] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating-
Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009.
Abstract. 16. Print.
Pulse
Dashed line – Same
Solid line – Different
Original f-to-2f Setup
[5] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating-
Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009.
Abstract. 28. Print.
Area changed
Current f-to-2f Setup
L
L
L
L
PPKTP
PBS
PBS
Sapphire
Delay Stage
DBS
S
F
Camera
Grating
λ
/2
λ
/2
λ
/2
P
P
–
P
e
r
i
s
c
o
p
e
L
–
L
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n
s
D
B
S
–
D
i
c
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r
o
i
c
B
e
a
m
s
p
l
i
t
t
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r
P
P
K
T
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–
P
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-
P
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P
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m
T
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a
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l
P
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o
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p
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λ
/
2
–
H
a
l
f
-
W
a
v
e
p
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e
P
B
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–
P
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z
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F
-
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–
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l
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A
L
–
A
s
p
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s
70 mm
200 mm
532 nm
1064 nm
Broadening the spectrum
Octave – f and 2f
Second Harmonic Generation
Doubled frequency
CEP Experiment
532 nm and 1064 nm
Broadened Spectrum
[5] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating-
Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009.
Abstract. 18. Print.
L
L
Sapphire
DBS
Results
Fringes appeared on camera on
both beams indicating diffraction
patterns in the beams themselves.
There was some movement in the
camera, which would indicate
overlap and an interference
between the two. However, this
was extremely difficult to
determine due to noise.
Future Improvements
Rid of fringe/diffraction pattern on beam.
Use better positioning of lenses to allow smaller movements for sapphire crystal
with stage.
Allow for rotation of the sapphire crystal to have better control on the beam.
Add an iris before the second lens to help with collimating the beam.
Put irises in the path to the periscope for alignment.
Collect data from a photo-diode.
Overall, more time and precision can allow this experiment to succeed.
Acknowledgments
This program is funded by the National Science Foundation through grant
number
PHYS-1461251
. Any opinions, findings, and conclusions or
recommendations expressed in this material are those of the author(s)
and do not necessarily reflect the views of the National Science
Foundation.
Dr. Vinod Kumarappan
Rajesh Kushawaha
Huynh Lam
Dr. Bret Flanders
Dr. Kristan Corwin
Fellow REU students
Exploring the stabilization of carrier-envelope phase in Atomic, Molecular, and Optical (AMO) physics research at Kansas State University's Light Source facility. Mentored by Dr. Vinod Kumarappan, the project delves into mode-locked lasers, offset frequencies, and the intricate setup of f-to-2f arrangements for advancing precision in laser technology.
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Presentation Transcript
Stabilizing Carrier-Envelope Phase Brett Chrisler Kansas State University REU 2015 Mentor: Dr. Vinod Kumarappan
Project Background Atomic, Molecular, and Optical (AMO) Physics Mentor: Dr. Vinod Kumarappan Postdoctoral: Rajesh Kushawaha Graduate: Huynh Lam Kansas Light Source (KLS) located in the James R. Macdonald Laboratory at Kansas State University KLS Laser 800 nm wavelength 3 millijoules/pulse at 25 femtoseconds/pulse 2kHz
Carrier-Envelope (CE) Phase Peak Electric Field Peak Pulse Envelope Offset [1] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating- Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009. Abstract. 4. Print.
Mode-Locked Lasers Sequences of pulses on the order of femtoseconds result. Each mode is set apart at the same interval leading to a frequency comb. Crystal (e.g. Ti:Sapphire) starts the lasing process and creates a gain spectrum and allows modes under this spectrum specifically to become excited. [3] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating- Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009. Abstract. 9. Print.
Offset Frequency Pulse Phase velocity -> Carrier-Wave Not the same = Carrier-Envelope Phase Shift Group velocity -> Envelope Dashed line Same Solid line Different [4] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating- Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009. Abstract. 16. Print.
Original f-to-2f Setup [5] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating- Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009. Abstract. 28. Print. Area changed
Current f-to-2f Setup L PPKTP L Camera Delay Stage /2 532 nm 1064 nm F PBS /2 /2 DBS S PBS L L Sapphire Grating P 200 mm 70 mm P Periscope L Lens DBS Dichroic Beamsplitter PPKTP Periodically-Poled Potassium Titanyl Phosphate /2 Half-Waveplate PBS Polarizing Beamsplitter Cube F- Filter S Slit AL Aspheric Lens
Broadened Spectrum Broadening the spectrum Octave f and 2f Second Harmonic Generation Doubled frequency CEP Experiment 532 nm and 1064 nm [5] Moon, Eric Wayne. "Carrier-Envelope Phase Stabilization of Grating- Based Chirped-Pulse Amplifiers." Diss. Kansas State U, 2009. Abstract. 18. Print.
L L Sapphire
Results Fringes appeared on camera on both beams indicating diffraction patterns in the beams themselves. There was some movement in the camera, which would indicate overlap and an interference between the two. However, this was extremely difficult to determine due to noise.
Future Improvements Rid of fringe/diffraction pattern on beam. Use better positioning of lenses to allow smaller movements for sapphire crystal with stage. Allow for rotation of the sapphire crystal to have better control on the beam. Add an iris before the second lens to help with collimating the beam. Put irises in the path to the periscope for alignment. Collect data from a photo-diode. Overall, more time and precision can allow this experiment to succeed.
Acknowledgments This program is funded by the National Science Foundation through grant number PHYS-1461251. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation. Dr. Vinod Kumarappan Rajesh Kushawaha Huynh Lam Dr. Bret Flanders Dr. Kristan Corwin Fellow REU students
