Workshop  ·  First independent edition  ·  2026

Carnot 2026 — Photonic Heat Engines

A two-day workshop on optical refrigeration, radiation-balanced lasers, and high-power laser source development.

A laser run backwards is a refrigerator. Everything interesting happens in between.

Dedicated to the memory of Mansoor Sheik-Bahae, 1956–2023.

Dates24–25 October 2026
VenuePAIS, University of New Mexico
CityAlbuquerque, New Mexico
FormatSingle track, discussion-focused

Announcements

  • Carnot 2026 is complete. Thank you to everyone who came to Albuquerque, and to the speakers, the poster presenters and the jury.
  • Exit survey. If you attended, please do not forget to fill out the survey sent to all of you on Monday, 26 October. Thank you to everyone who has already completed it. Your answers help us make the next event even better, and it takes two to three minutes. If the email did not reach you, write to carnot.workshop@gmail.com and we will send it.
  • Photos. We will soon be uploading pictures from the workshop. Once posted, you will find them under the Photos tab above.
  • Program. The final technical program is available as a PDF.
  • Carnot 2027 will be held at the University of Notre Dame in South Bend, Indiana. Dates and the call for participation will be announced here. Stay tuned.

In memoriam

Mansoor Sheik-Bahae

1956 – 2023

Carnot 2026 is dedicated to Mansoor Sheik-Bahae, who passed away in July 2023, aged 67. Born in Isfahan, a descendant of the seventeenth-century polymath Sheikh Bahāʾi, Mansoor came to the United States to study electrical engineering, taking his doctorate at SUNY Buffalo in 1987. He joined CREOL in its founding year and moved to the University of New Mexico in 1994, rising to Distinguished Professor — the highest honor UNM gives its faculty — and becoming the first director of its Optical Science and Engineering program.

With Eric Van Stryland and colleagues, Mansoor invented the Z‑scan: one beam, a moving sample, a detector, and from it the sign and magnitude of a material’s optical nonlinearity. It remains the standard measurement, and the two of them shared Optica’s R. W. Wood Prize for it in 2012. He then found a link that had been thought impossible — Kramers–Kronig relations are linear, so they ought not to connect nonlinear quantities. The way through was to linearize the problem by treating nondegenerate absorption, two photons of different frequency, which made nonlinear refraction predictable from two-photon absorption. A Fellow of Optica and of SPIE, he was also a senior member of the IEEE.

In 1995 Mansoor began working with Richard Epstein on cooling solids with light, and led that effort for the next twenty-seven years, directing the Consortium for Laser Cooling in Solids from 2004 to 2022. The group established Yb:YLF as the material the field now builds on, and in 2022 cooled a load to 125 K. He worked out the theory of radiation-balanced lasers, and his group built the first ones; others carried it from there to the first cooling of Yb-doped silica. And when he pulled the mirror stack out of a semiconductor disk laser, it opened a field — the MECSEL — that now reaches as far as sodium guide stars.

Cooling a semiconductor was something he was deeply passionate about seeing, and he never got the chance. His co-authors called it his unfulfilled dream. One session of this workshop goes straight at that problem. Another continues his work on radiation-balanced lasers. A deep thinker, Mansoor never stopped pondering the fundamental limits of noise, entropy and engine efficiency. He would have loved to be at this workshop with all of us. His presence is missed dearly!

Richard Epstein, Denis Seletskiy and Eric Van Stryland, “Mansoor Sheik-Bahae (1956–2023),” Nature Photonics 17, 833–834 (2023).

Mansoor Sheik-Bahae
Credit: Eric Van Stryland

Selected works

  • 1989Z-scan
    M. Sheik-Bahae, A. A. Said, T.-H. Wei, D. J. Hagan and E. W. Van Stryland, IEEE J. Quantum Electron. 26, 760–769 (1989)
  • 1991Kramers–Kronig and nonlinear refraction
    M. Sheik-Bahae, D. C. Hutchings, D. J. Hagan and E. W. Van Stryland, IEEE J. Quantum Electron. 27, 1296 (1991)
  • 2007Optical refrigeration, review
    M. Sheik-Bahae and R. I. Epstein, Nature Photonics 1, 693–699 (2007)
  • 2010Laser cooling to cryogenic temperatures
    D. V. Seletskiy, S. D. Melgaard, S. Bigotta, A. Di Lieto, M. Tonelli and M. Sheik-Bahae, Nature Photonics 4, 161–164 (2010)
  • 2015Mirrorless semiconductor disk laser — the MECSEL
    Z. Yang, A. R. Albrecht, J. G. Cederberg and M. Sheik-Bahae, Opt. Express 23, 33164–33169 (2015)
  • 2018First all-solid-state optical cryocooler — an infrared sensor cooled to 135 K
    M. P. Hehlen, J. Meng, A. R. Albrecht, E. R. Lee, A. Gragossian, S. P. Love, C. E. Hamilton, R. I. Epstein and M. Sheik-Bahae, Light: Science & Applications 7, 15 (2018)
  • 2019First radiation-balanced disk lasers
    Z. Yang, J. Meng, A. R. Albrecht and M. Sheik-Bahae, Opt. Express 27, 1392–1400 (2019)
  • 2020Theory of radiation-balanced lasers
    M. Sheik-Bahae and Z. Yang, IEEE J. Quantum Electron. 56, 1000109 (2020)
  • 2022A load cooled to 125 K
    J. L. Kock, A. R. Albrecht, R. I. Epstein and M. Sheik-Bahae, Opt. Lett. 47, 4720–4723 (2022)
  • 2022Semiconductor sodium guide-star source
    M. Zhang et al., Opt. Express 30, 42470–42479 (2022)

The premise

Entropy is a design variable, not a bookkeeping detail.

A laser pump is a single narrowband mode; the fluorescence it drives is broadband and leaves in every direction. That difference in entropy between the two light fields is what allows a solid to be cooled with light, and it gives a laser crystal three operating points. When lasing, the quantum defect heats it. Pumped below the mean fluorescence energy, anti-Stokes emission carries heat away — optical refrigeration. In between, the two cancel: a radiation‑balanced laser, whose gain medium carries no net heat load.

Heat limits the average power, beam quality and frequency stability of solid-state lasers. This workshop is about the regime where source design and thermal management stop being separate problems.

Carnot continues the Photonic Heat Engines community, which met for eight editions within a larger photonics meeting through 2024. This is its first independent meeting.

HEAT OUT HEAT IN Laser Quantum defect deposits heat in the crystal. Radiation-balanced laser Defect heating cancels fluorescence cooling. Optical refrigerator Anti-Stokes fluorescence carries heat away.
One material, one pump beam, three operating points. The session colors are taken from this axis: blue where light carries heat out, green where the two cancel, gold where the defect deposits it.

Confirmed speakers

Everyone named here has accepted. Each badge gives the physics, not the session: color for which way the heat goes, shape for the pump.

+Absorption, emission and extraction — work that adds to any column, because it acts on the photonic environment rather than on how the state was excited. Two of its three cells are empty this year.

Richard Epstein

Richard Epstein

University of New Mexico

First demonstration of laser cooling in a solid; rare-earth spectroscopy; cryogenic optical refrigerators.

Cooling · coherent
Hiroki Tanaka

Hiroki Tanaka

Leibniz Institute for Crystal Growth (IKZ), Berlin

Fluoride crystal growth; Yb-doped cooling materials; radiation-balanced laser design.

Cooling · coherent
Peter Pauzauskie

Peter Pauzauskie

University of Washington

Laser refrigeration of nanomaterials; Yb-doped nanocrystals; nanoscale thermometry.

+Cooling · density of states
Masaru Kuno

Masaru Kuno

University of Notre Dame

Semiconductor nanostructures; single-particle spectroscopy; laser cooling of semiconductors.

Cooling · coherent
Matt Sheldon

Matt Sheldon

University of California, Irvine

Nanophotonics and plasmonics; hot-carrier photophysics; luminescence thermodynamics.

Cooling · coherent
Peter Dragic

Peter Dragic

University of Illinois Urbana-Champaign

Optical fiber materials and glass science; Brillouin scattering; fiber laser design.

Balanced · coherent
Michel Digonnet

Michel Digonnet

Stanford University

Rare-earth-doped fiber lasers, amplifiers and sensors; radiation-balanced silica fiber lasers.

Cooling and balanced · coherent
Hanieh Fattahi

Hanieh Fattahi

Max Planck Institute for the Science of Light, Erlangen

Ultrafast and field-resolved optics; sun-pumped radiation-balanced lasers.

Balanced · incoherent
Eli Yablonovitch

Eli Yablonovitch

University of California, Berkeley

Opto-electronic thermodynamics; photon free energy and entropy in emission and absorption; light extraction in LEDs and solar cells.

Cooling · incoherent
Sushrut Ghonge

Sushrut Ghonge

Saint Mary’s College

Thermodynamics of photoluminescent cooling; cooling with incoherent and broadband light.

Cooling · incoherent
Denis Seletskiy

Denis Seletskiy

University of New Mexico

Ultrafast and quantum optics; laser cooling of solids; vacuum-field fluctuations.

Welcome
Joel Bixler

Joel Bixler

Air Force Office of Scientific Research

Program Officer, High-Energy Radiation-Matter Systems (HERMES).

Panel discussion
Christian Schmiegelow

Christian Schmiegelow

Universidad de Buenos Aires

Laser cooling of solids and nanoparticles in electrodynamic traps; cavity-modified electromagnetic environments; Purcell effect and enhanced anti-Stokes emission.

+Cooling · density of states
Pengning Chao

Pengning Chao

Maxwell Labs

Nanophotonics, computational inverse design, and high-power optical refrigeration.

+Cooling · density of states

Organizing committee

Denis SeletskiyUniversity of New Mexico
Masaru KunoUniversity of Notre Dame
Peter PauzauskieUniversity of Washington
Alejandro RodriguezPrinceton University / Maxwell Labs

Local organizing committee

Alexander AlbrechtUniversity of New Mexico
Max GardnerUniversity of New Mexico
Morteza DarvishiUniversity of New Mexico
Ghazaleh AnsariUniversity of New Mexico

Support

Sponsors

Organizations interested in supporting the workshop are welcome to write to carnot.workshop@gmail.com.

Workshop sponsor

Maxwell Labs

With support from

The University of New Mexico, Department of Physics & Astronomy SELA Photonics Triton Photonics

Program

Final, 21 October 2026. The workshop runs from 08:00 on Saturday to 15:00 on Sunday — the program closes at 13:30, and the optional laboratory tours run until 15:00, so a flight from 17:00 onwards is safe. Session themes run along the thermal axis: rare-earth cooling, semiconductor cooling, radiation-balanced lasers, then high-power sources and applications.

Invited talks across six sessionsFlash talksPoster session, with prizes Panel discussionCommunity roadmap and funding sessionLaboratory tours

Download the final program (PDF, 36 pages).

The workshop room in the PAIS building
Talks, flash talks and the panel discussion are in PAIS 1100, the 200-seat auditorium. PAIS 1110 next door takes lunch, the posters and anyone who wants to carry on an argument; the Sunday working groups split into PAIS 1140 and PAIS 1160.

Day One

Saturday 24 October
Registration, arrival, and coffee
0 · Welcome25 minWelcome, how the two days run, and the premise behind Sunday’s roadmap session.
Denis SeletskiyMeet CARNOT: 2026 and beyondUniversity of New Mexico
I · Optical refrigeration — rare earthsChair: Denis Seletskiy · University of New Mexico3 × 30 min
Richard EpsteinI-1Early days of optical refrigerationUniversity of New Mexico
Hiroki TanakaI-2Optical refrigeration in rare-earth-doped fluoride single crystals: beyond Yb:YLFLeibniz Institute for Crystal Growth
Michel DigonnetI-3Anti-Stokes fluorescence cooling in silicate fibersStanford University
Coffee break (30 min)
II · Optical refrigeration — semiconductorsChair: Hiroki Tanaka · Leibniz IKZ, Berlin2 × 30 min
Matt SheldonII-1Optical cooling in all-inorganic perovskite nanocrystalsUniversity of California, Irvine
Masaru KunoII-2Semiconductor laser cooling using CsPbBr3 nanocrystalsUniversity of Notre Dame
Workshop photograph (10 min)In the Lecture Hall, PAIS 1100
Lunch (60 min)Catered on site
III · Nanostructures and engineered environmentsChair: Masaru Kuno · University of Notre Dame3 × 30 min
Peter PauzauskieIII-1Mie-enhanced solid-state laser refrigeration with optically levitated spherical microcavitiesUniversity of Washington
Christian SchmiegelowIII-2Engineering electromagnetic environments for laser cooling of solidsUniversidad de Buenos Aires
Pengning ChaoIII-3Nanophotonic inverse design for optical refrigerationMaxwell Labs
Coffee break (30 min)
IV · High-power and radiation-balanced lasersChair: Peter Pauzauskie · University of WashingtonTalk and panel
Peter DragicIV-1Fibers and fiber materials for power scaling of RBFLsUniversity of Illinois Urbana-Champaign
Panel discussion (60 min)Moderator: Joel Bixler · Air Force Office of Scientific Research
Panelists: Richard Epstein · Ricky Gibson · Peter Dragic · Pengning Chao
Where cryogenic optical refrigerators are actually needed, how far radiation-balanced and high-power lasers can be pushed, and what the two problems have in common
V · Flash talksChair: Denis Seletskiy · University of New Mexico2 min each
Flash talks (15 min)Two minutes and one slide each — the posters follow at the restaurant
Bus to the restaurant (20 min)Board outside PAIS on Redondo Drive at 17:00; a fifteen-minute ride to La Fonda del Bosque, arriving 17:20. Returns to the hotel and to PAIS after dinner
Evening
Poster session and reception (70 min)At La Fonda del Bosque — the boards go up at the restaurant, with light refreshments
Workshop dinnerLa Fonda del Bosque, National Hispanic Cultural Center · poster prizes and photographs

Day Two

Sunday 25 October
Registration, arrival, and coffee
VI · Thermodynamics and broadband sourcesChair: Pengning Chao · Maxwell Labs3 × 30 min
Hanieh FattahiVI-1Solar-pumped radiation-balanced laserMax Planck Institute for the Science of Light
Eli YablonovitchVI-2Opto-electronic thermodynamicsUniversity of California, Berkeley
Sushrut GhongeVI-3Optical cooling with incoherent lightSaint Mary’s College
Coffee break (30 min)
Talks from the poster prize winners10 minutes each
VII · A roadmap for the photonic engine community2 × 30 min + joint discussionA discussion panel on where photonic engines go next and what the field needs to get there, split across Working groups A and B. The moderators then present each group’s summary and take further input before lunch. Sign-up sheets are at the registration desk on Sunday morning — join one group, both, or neither.
Working groups A and B — first round (30 min)Running in parallel, in Rm 1140 and Rm 1160
Second round (30 min)Both groups run again — switch rooms, stay where you are, or sit this one out
Joint discussion with summary from moderators (30 min)Each group reports, then the two halves meet
Lunch (60 min)Catered on site
Closing remarks (10 min)Thanks, and where CARNOT goes next
Lab tours / adjournOptional tours of UNM laboratories · the workshop ends at 15:00

Session themes

0 · WelcomeWelcome and opening remarks — what this workshop is for, and where it is going.
I · Optical refrigeration — rare earthsYb-doped fluorides and silicate fibers, ultrapure crystal growth, and how far the bulk approach can be pushed.
II · Optical refrigeration — semiconductorsPerovskite nanocrystals and bulk crystals; luminescence quantum yield and the parasitics that have kept net cooling out of reach. Claims here are measured against the community’s reporting standard.
III · Nanostructures and engineered environmentsThe other way to push performance: Mie resonances, cavity-modified emission and computational inverse design, rather than better material.
IV · High-power and radiation-balanced lasersPower scaling in both directions — the lasing branch and the cooling branch — and the panel that argues about which limit binds.
V · Flash talksStudents and postdocs presenting work in progress — two minutes and one slide each on Saturday afternoon, then seventy minutes at the boards at the restaurant, before dinner.
VI · Thermodynamics and broadband sourcesSunlight and other incoherent pumps, and the thermodynamic bookkeeping that decides what is allowed.

Students and postdocs

Poster session, with prizes

The posters come from the speakers’ groups and from UNM. Every poster gets a two-minute flash talk on the Saturday afternoon, before the bus leaves for the restaurant, and the boards go up at La Fonda del Bosque, where the session runs from 17:20 until dinner at 18:30. Print at 4 × 3 feet, landscape — the boards cannot take portrait. Mounting material is provided.

Poster prizes — sponsored by SELA Photonics, Triton Photonics and the UNM Department of Physics and Astronomy — are awarded at the workshop dinner, and the winners give short talks on Sunday morning. Our thanks to the poster prize jury: Hanieh Fattahi, Christian Schmiegelow and Masaru Kuno.

Photos

Pictures from the workshop

We are sorting through the photographs from the two days. They will be posted here shortly. If you took pictures you would like included, send them to carnot.workshop@gmail.com.

Venue and travel

Albuquerque, late October

The workshop meets in the Physics, Astronomy and Interdisciplinary Sciences building on the University of New Mexico main campus. Los Alamos, Sandia, the Air Force Research Laboratory and UNM's Center for High Technology Materials are all within reach of the same room — which is why the field's center of gravity has moved here.

Painters moved to New Mexico for the light. At 5,300 feet the air is thin and dry, the blue overhead is harder than seems reasonable, and shadows keep their edges. It is a fitting place to spend two days arguing about photons.

Late October is the best of it — seventies by day, forties after dark, aspen gold still holding on the Sandias, and balloons going up at dawn.

The PAIS building at the University of New Mexico
PAIS from Redondo Drive. The courtyard entrance is on the far side.
Cholla cactus silhouetted against an orange and pink desert sunset
Cholla at sunset. The light is what brought the painters, and it is still the best argument for coming.
Chile ristras hanging above crates of fruit at a roadside stand
Ristras at a roadside stand. Red or green is not a rhetorical question here.
Cholla in the foreground with the Sandia Mountains lit gold behind
The Sandias at the end of the day, from the edge of town. The range runs the whole eastern side of the city.
Red sandstone bluff above juniper and pinyon
Red rock and juniper. The drive out of the valley in almost any direction looks like this.
CENTRAL AVE · US 66 REDONDO DR YALE BLVD PEDESTRIAN MALL CORNELL MALL CORNELL DR Art & Art History Art Museum Popejoy Hall Bookstore Marron Hall Yale Park ART · UNM/POPEJOY P Cornell Parking Structure $1.75 / 30 min $28 all day PAIS 210 Yale Blvd NE ROOMS 1100 · 1110 1140 · 1160 YARD 1 2 3 Hotel Parq Central, 1.2 mi west N Schematic, not to scale
1 PAIS is entered through the courtyard, which opens west onto the pedestrian mall. 2 The bus leaves at 17:00 on Saturday from the stop on Redondo Drive, west of Yale, for the poster session and dinner. 3 Arriving by ART: the UNM/Popejoy station is in the Central median in front of the UNM Bookstore. Leave the platform at its east end and cross Central at the Cornell signal, then north on Cornell to Redondo, west along Redondo, and right into the mall and the courtyard — about seven minutes.

The building

If you can stay an extra day

Sandia Peak TramwayFrom the edge of the city to 10,378 feet in fifteen minutes — a rise of 3,819 feet, and the longest aerial tram in the Americas.
The Very Large ArrayTwenty-seven dishes on the Plains of San Agustin, about two and a half hours southwest. Worth the drive.
Santa Fe and Los AlamosSanta Fe is an hour north. Los Alamos, where this field began, is about ninety minutes.
“Red or green?”The official state question. It refers to chile, you will be asked it, and if you cannot decide the answer is “Christmas.”