A 40 W, 780 nm laser system with compensated dual beam splitters for atom interferometry
Minjeong Kim, Remy Notermans, Chris Overstreet, Joseph Curti, Peter Asenbaum, Mark A. Kasevich
aa r X i v : . [ phy s i c s . a t o m - ph ] A ug A 40 W, 780 nm laser system with compensated dual beam splitters for atominterferometry
Minjeong Kim, Remy Notermans, ∗ Chris Overstreet, Joseph Curti, Peter Asenbaum, and Mark A. Kasevich † Stanford University, Stanford, CA 94305 (Dated: August 3, 2020)We demonstrate a narrow-linewidth 780 nm laser system with up to 40 W power and a frequencymodulation bandwidth of 230 MHz. Efficient overlap on nonlinear optical elements combines twopairs of phase-locked frequency components into a single beam. Serrodyne modulation with ahigh-quality sawtooth waveform is used to perform frequency shifts with > .
5% efficiency overtens of MHz. This system enables next-generation atom interferometry by delivering simultaneous,Stark-shift-compensated dual beam splitters while minimizing spontaneous emission.
Narrow-linewidth, high-power laser systems are of sub-stantial interest due to their applications in atomicphysics and precision measurement; in particular, theperformance of precise atom interferometers is often lim-ited by the characteristics of the laser that diffracts andinterferes the atoms [1–4]. Such experiments requirehigh-power lasers with low phase noise [5], frequencyagility of tens to hundreds of MHz [6], and an opticalspectrum that contains frequency components separatedby tens of GHz or more [7]. Low-noise, frequency agilelasers with more than 1 . .
24 nm, which is the rubidium D resonance, and thefrequency span can be varied by up to 2 GHz. The fre-quency of each component can be shifted by serrodynemodulation of the 1560 nm laser with efficiency > . . . π . FrequencyBlue Bragg pairRed Bragg pair f!f" ΔfSingle-photonresonance
FIG. 1. Optical spectrum. The spectrum consists of two pairsof frequencies (Red Bragg pair and Blue Bragg pair) on ei-ther side of the single-photon resonance. In the configurationdescribed in this work, ∆ f = 370 GHz. The frequency differ-ences f and f can be tuned independently by tens of MHz.Figure is not to scale. PPLNPPLNPPLN PPLN
ISOISO /4/4 PL ... PL ... (a) (b)(c) f f! IPG 3 IPG 1IPG 4 IPG 2
FIG. 2. Schematic of the laser system. The (red, blue) beams denote (1560 nm, 780 nm) light. Figure is not to scale. NKT:NKT Photonics fiber laser, EOM: electro-optic modulator, PL: phase lock, IPG: IPG Photonics fiber amplifier, λ /2: half-waveplate, λ /4: quarter-wave plate, PPLN: periodically-poled lithium niobate crystal, SPDM: short-pass dichroic mirror, BD: beamdump, AOM: acousto-optic modulator, ISO: Faraday isolator, aGP fiber: aeroGuide-Power polarization-maintaining single-mode fiber. (a) Beam profile of 780 nm light at 6 W produced by IPG 1 at a distance of 100 cm after the aGP fiber outputcollimator; (b) serrodyne modulation setup; (c) frequency doubling optics. OC2 controller.The output of each PPLN crystal passes through ashortpass dichroic mirror (SPDM) to deflect the remain-ing 1560 nm light into a beam dump. Each 780 nm beamproceeds into a plano-convex lens and is collimated to awaist of 1 . ∼
30 GHzand the 780 nm light from the first crystal is detuned by370 GHz, the 780 nm light from the first crystal passesthrough the second crystal without substantial alterationas the 1560 nm light is frequency doubled. The output ofthe second crystal consists of a beam that contains both780 nm frequency components. This method providesan efficient way to overlap the two 780 nm frequencieswithout much loss. The total 780 nm power in bothpaths after doubling at full power is up to 40 W. On each beam path, an acousto-optic modulator(AOM) controls the beam intensity. The diffracted beamcontinues along the path while the undiffracted beam ispicked off and directed to a beam dump. A RF synthe-sizer (Moglabs Agile RF Synthesizer RF-421) supplies the80 MHz RF signals that drive the two AOMs. The ampli-tude of each RF signal is shaped by a voltage-controlledattenuator (Mini Circuits Frequency Mixer ZP-1H+, ZP-1LH) that is controlled by an arbitrary function gener-ator (Tektronix AFG3102). This technique allows theproduction of laser pulses with arbitrary shape.The diffracted beam from each AOM is sent through aFaraday isolator to protect from back reflections and thencoupled into a 5 m polarization-maintaining single-modefiber (NKT Photonics aeroGuide-Power) with ∼ . µ m) and customized collimators (OZ Op-tics, HPUCO-15-780-P). Fig. 2(a) shows the beam profileof the fiber output at a distance of 100 cm from the colli-mator. To image the 6 W beam, the beam was pulsed onfor 10 µ s at a repetition rate of 1 Hz. The weak hexagonal -40 0-20 20 40-80-60-20-400-40 0-20 20 40-80-60-20-400 (a)(b) N o r m a li z e d p o w e r ( d B m ) N o r m a li z e d p o w e r ( d B m ) Frequency (MHz)
FIG. 3. Log plots of the reconstructed optical spectra ofthe serrodyne-modulated beam and the unmodulated carrier.The modulated spectrum (red curve) is normalized to theunmodulated carrier (blue curve) power. (a) 3 MHz modu-lation. The efficiency is 98 . −
41 dB below peak power and the largest sideband sup-pressed to − . . −
30 dB, and largest sidebandsuppression of −
26 dB. structure in the tails gets less pronounced while propa-gating due to its higher divergence. Otherwise, the beamprofile is Gaussian and has no noticeable fringes or aber-rations.The frequency of each beam can be shifted by phasemodulation of the 1560 nm lasers via the EOMs. For acarrier signal with amplitude E and frequency ω , thephase-modulated signal is given by E = E exp [ i ( ω t + h φ ( t ))] (1)where h is the modulation depth and φ ( t ) is the modu-lation waveform. We employ serrodyne modulation [12]to suppress undesired sidebands. The idea of serrodynemodulation is to use φ ( t ) = ω m t mod (2 π/h ) (2)as the modulation waveform, where ω m is the desiredfrequency shift. In the ideal case, serrodyne modula-tion transfers all the carrier power to a single sideband with frequency ω + ω m . However, bandwidth limitationsprovide a lower bound on the fall time of the sawtoothwaveform described by Eq. 2 and lead to additional side-bands in the phase-modulated spectrum. The efficiencyof serrodyne modulation thus depends on the bandwidthof the applied waveform.In our apparatus, the sawtooth waveform is generatedby an arbitrary waveform generator (AWG, TektronixAWG5014) with an analog bandwidth of 230 MHz. Thevoltage output level of the AWG is sufficient to reach V π of the EOMs without the use of an external amplifier.Note that the voltage required to achieve the serrodynecondition for a frequency doubled system is half of whatis required for a non-doubled system. Fig. 3 shows a logplot of the unmodulated input and the modulated outputspectra for 3 MHz and 28 MHz modulation. Negative-frequency modulation can be carried out by applying anegative-slope sawtooth from the negative output port ofthe AWG. For 3 MHz modulation, the transfer efficiencyis 98 .
5% with the carrier suppressed by −
41 dB and thelargest sideband suppressed by − . . −
30 dB, and the largest sideband is suppressed by −
26 dB. In both cases, the amplitude of the sawtoothmodulation was 2 .
29 V pp . The serrodyne modulationwas tested at frequencies of up to 400 MHz, where the ef-ficiency is 63 .
3% at a modulation amplitude of 4 .
12 V pp .The modulation angular frequency retains its origi-nal value even after the modulated beam is frequencydoubled [15]. This can be seen from the fact that thefrequency-doubled field is proportional to the square ofthe input field. Squaring Eq. 1, we obtain E = E exp [ i (2 ω t + 2 h φ ( t ))] . (3)Eq. 3 indicates that when the modulated signal is fre-quency doubled, the carrier frequency and the modula-tion depth are doubled, but the modulation frequency ω m remains unchanged.We implement a phase lock to stabilize the relativephase of the two beam paths. The error signal consists ofthe beating signal obtained by interfering a small fractionof the light from each path after the high-power fibers.This signal is amplified, demodulated, low-pass filtered,and used as the input of a PID controller (Liquid Instru-ments Moku:lab PID controller). The PID controller hasan input bandwidth of 200 MHz and an output band-width of >
300 MHz (3 dB point). The error signal andoutput of the PID controller are connected to a SPDTswitch to disable the feedback while the light is off. Theoutput of the PID controller is amplified and applied tothe corresponding EOM.The performance of the phase lock was measured forcontinuous wave (CW) operation and for pulses of du-ration 90 µ s to 2 ms at repetition rates of 100 Hz to1 kHz, the timescales relevant for driving sequential two-photon transitions. Each pulse is initially turned on at alower power for 20 µ s to allow the phase lock to acquire.In CW operation, we observe relative phase noise below −
91 dBc/Hz at an offset of 10 kHz.In summary, we have developed a 780 nm laser sys-tem with up to 40 W in frequency components sepa-rated by 370 GHz. These frequency components are ef-ficiently overlapped on PPLN nonlinear crystals. Serro-dyne modulation using a high-bandwidth sawtooth wave-form allows us to perform highly efficient frequency shifts.This laser system is expected to improve the perfor-mance of current and future high-precision measurementswith atom interferometry. Other experiments that relyon high power lasers with frequency tunability, such astrapped ion experiments [16], can also benefit from thistechnique. The number of frequency components in eachbeam could be increased by including additional nonlin-ear crystals.We acknowledge funding from the Office of Naval Re-search DURIP and the Vannevar Bush Faculty Fellow-ship Program. We thank Agnetta Cleland and MeganNantel for their assistance with this work. ∗ Current address: Atom Computing, Inc., Berkeley, CA94710 † [email protected][1] R. H. Parker, C. Yu, W. Zhong, B. Estey, and H. M¨uller, Science , 191 (2018).[2] P. Asenbaum, C. Overstreet, M. Kim, J. Curti, andM. A. Kasevich, arXiv preprint arXiv:2005.11624 (2020),arXiv:2005.11624 [physics.atom-ph].[3] J. Stuhler, M. Fattori, T. Petelski, and G. M. Tino,Journal of Optics B: Quantum and Semiclassical Optics , S75 (2003).[4] P. W. Graham, J. M. Hogan, M. A. Kasevich, and S. Ra-jendran, Phys. Rev. Lett. , 171102 (2013).[5] P. Asenbaum, C. Overstreet, T. Kovachy, D. D.Brown, J. M. Hogan, and M. A. Kasevich,Phys. Rev. Lett. , 183602 (2017).[6] C. Overstreet, P. Asenbaum, T. Kovachy, R. Noter-mans, J. M. Hogan, and M. A. Kasevich,Phys. Rev. Lett. , 183604 (2018).[7] T. Kovachy, P. Asenbaum, C. Overstreet, C. Donnelly,S. Dickerson, A. Sugarbaker, J. Hogan, and M. Kasevich,Nature , 530 (2015).[8] H. M¨uller, S.-W. Chiow, Q. Long, and S. Chu,Opt. Lett. , 202 (2006).[9] S. Merlet, L. Volodimer, M. Lours, and F. P. Dos Santos,Applied Physics B , 749 (2014).[10] J. Fang, J. Hu, X. Chen, H. Zhu, L. Zhou, J. Zhong,J. Wang, and M. Zhan, Opt. Express , 1586 (2018).[11] R. C. Cumming, Proceedings of the IRE , 175 (1957).[12] D. M. S. Johnson, J. M. Hogan, S. w. Chiow, and M. A.Kasevich, Opt. Lett. , 745 (2010).[13] S. S. San´e, S. Bennetts, J. E. Debs, C. C. N. Kuhn, G. D.McDonald, P. A. Altin, J. D. Close, and N. P. Robins,Opt. Express , 8915 (2012).[14] S.-W. Chiow, T. Kovachy, J. M. Hogan, and M. A. Ka-sevich, Opt. Lett. , 3861 (2012).[15] R. W. Boyd, Nonlinear optics (Academic press, 2019).[16] R. Blatt and D. Wineland, Nature453