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2. Cold atoms in space: community workshop summary and proposed road-map

Author

Alonso, Iván, Alpigiani, Cristiano, Altschul, Brett, Araújo, Henrique, Arduini, Gianluigi, Arlt, Jan, Badurina, Leonardo, Balaž, Antun, Bandarupally, Satvika, Barish, Barry C., Barone, Michele, Barsanti, Michele, Bass, Steven, Bassi, Angelo, Battelier, Baptiste, Baynham, Charles F. A., Beaufils, Quentin, Belić, Aleksandar, Bergé, Joel, Bernabeu, Jose, Bertoldi, Andrea, Bingham, Robert, Bize, Sébastien, Blas, Diego, Bongs, Kai, Bouyer, Philippe, Braitenberg, Carla, Brand, Christian, Braxmaier, Claus, Bresson, Alexandre, Buchmueller, Oliver, Budker, Dmitry, Bugalho, Luís, Burdin, Sergey, Cacciapuoti, Luigi, Callegari, Simone, Calmet, Xavier, Calonico, Davide, Canuel, Benjamin, Caramete, Laurentiu-Ioan, Carraz, Olivier, Cassettari, Donatella, Chakraborty, Pratik, Chattopadhyay, Swapan, Chauhan, Upasna, Chen, Xuzong, Chen, Yu-Ao, Chiofalo, Maria Luisa, Coleman, Jonathon, Corgier, Robin, Cotter, J. P., Michael Cruise, A., Cui, Yanou, Davies, Gavin, De Roeck, Albert, Demarteau, Marcel, Derevianko, Andrei, Di Clemente, Marco, Djordjevic, Goran S., Donadi, Sandro, Doré, Olivier, Dornan, Peter, Doser, Michael, Drougakis, Giannis, Dunningham, Jacob, Easo, Sajan, Eby, Joshua, Elertas, Gedminas, Ellis, John, Evans, David, Examilioti, Pandora, Fadeev, Pavel, Fanì, Mattia, Fassi, Farida, Fattori, Marco, Fedderke, Michael A., Felea, Daniel, Feng, Chen-Hao, Ferreras, Jorge, Flack, Robert, Flambaum, Victor V., Forsberg, René, Fromhold, Mark, Gaaloul, Naceur, Garraway, Barry M., Georgousi, Maria, Geraci, Andrew, Gibble, Kurt, Gibson, Valerie, Gill, Patrick, Giudice, Gian F., Goldwin, Jon, Gould, Oliver, Grachov, Oleg, Graham, Peter W., Grasso, Dario, Griffin, Paul F., Guerlin, Christine, Gündoğan, Mustafa, Gupta, Ratnesh K., Haehnelt, Martin, Hanımeli, Ekim T., Hawkins, Leonie, Hees, Aurélien, Henderson, Victoria A., Herr, Waldemar, Herrmann, Sven, Hird, Thomas, Hobson, Richard, Hock, Vincent, Hogan, Jason M., Holst, Bodil, Holynski, Michael, Israelsson, Ulf, Jeglič, Peter, Jetzer, Philippe, Juzeliūnas, Gediminas, Kaltenbaek, Rainer, Kamenik, Jernej F., Kehagias, Alex, Kirova, Teodora, Kiss-Toth, Marton, Koke, Sebastian, Kolkowitz, Shimon, Kornakov, Georgy, Kovachy, Tim, Krutzik, Markus, Kumar, Mukesh, Kumar, Pradeep, Lämmerzahl, Claus, Landsberg, Greg, Le Poncin-Lafitte, Christophe, Leibrandt, David R., Lévèque, Thomas, Lewicki, Marek, Li, Rui, Lipniacka, Anna, Lisdat, Christian, Liu, Mia, Lopez-Gonzalez, J. L., Loriani, Sina, Louko, Jorma, Luciano, Giuseppe Gaetano, Lundblad, Nathan, Maddox, Steve, Mahmoud, M. A., Maleknejad, Azadeh, March-Russell, John, Massonnet, Didier, McCabe, Christopher, Meister, Matthias, Mežnaršič, Tadej, Micalizio, Salvatore, Migliaccio, Federica, Millington, Peter, Milosevic, Milan, Mitchell, Jeremiah, Morley, Gavin W., Müller, Jürgen, Murphy, Eamonn, Müstecaplıoğlu, Özgür E., O’Shea, Val, Oi, Daniel K. L., Olson, Judith, Pal, Debapriya, Papazoglou, Dimitris G., Pasatembou, Elizabeth, Paternostro, Mauro, Pawlowski, Krzysztof, Pelucchi, Emanuele, Pereira dos Santos, Franck, Peters, Achim, Pikovski, Igor, Pilaftsis, Apostolos, Pinto, Alexandra, Prevedelli, Marco, Puthiya-Veettil, Vishnupriya, Quenby, John, Rafelski, Johann, Rasel, Ernst M., Ravensbergen, Cornelis, Reguzzoni, Mirko, Richaud, Andrea, Riou, Isabelle, Rothacher, Markus, Roura, Albert, Ruschhaupt, Andreas, Sabulsky, Dylan O., Safronova, Marianna, Saltas, Ippocratis D., Salvi, Leonardo, Sameed, Muhammed, Saurabh, Pandey, Schäffer, Stefan, Schiller, Stephan, Schilling, Manuel, Schkolnik, Vladimir, Schlippert, Dennis, Schmidt, Piet O., Schnatz, Harald, Schneider, Jean, Schneider, Ulrich, Schreck, Florian, Schubert, Christian, Shayeghi, Armin, Sherrill, Nathaniel, Shipsey, Ian, Signorini, Carla, Singh, Rajeev, Singh, Yeshpal, Skordis, Constantinos, Smerzi, Augusto, Sopuerta, Carlos F., Sorrentino, Fiodor, Sphicas, Paraskevas, Stadnik, Yevgeny V., Stefanescu, Petruta, Tarallo, Marco G., Tentindo, Silvia, Tino, Guglielmo M., Tinsley, Jonathan N., Tornatore, Vincenza, Treutlein, Philipp, Trombettoni, Andrea, Tsai, Yu-Dai, Tuckey, Philip, Uchida, Melissa A., Valenzuela, Tristan, Van Den Bossche, Mathias, Vaskonen, Ville, Verma, Gunjan, Vetrano, Flavio, Vogt, Christian, von Klitzing, Wolf, Waller, Pierre, Walser, Reinhold, Wille, Eric, Williams, Jason, Windpassinger, Patrick, Wittrock, Ulrich, Wolf, Peter, Woltmann, Marian, Wörner, Lisa, Xuereb, André, Yahia, Mohamed, Yazgan, Efe, Yu, Nan, Zahzam, Nassim, Zambrini Cruzeiro, Emmanuel, Zhan, Mingsheng, Zou, Xinhao, Zupan, Jure, and Zupanič, Erik

Published
2022
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4. Scientific assessment of the CARIOQA-PMP quantum accelerometer pathfinder

Author

Schilling, Manuel, Battalier, Baptiste, Forsberg, René, Gaaloul, Naceur, Gruber, Thomas, von Klitzing, Wolf, Lévèque, Thomas, Migliaccio, Federica, Müller, Jürgen, Pereira dos Santos, Franck, and Zahzam, Nassim

Abstract

Satellite gravimetry is a unique tool to monitor the Earth’s mass variations. Satellite missions like GRACE and GRACE Follow-On provide insights into the time-variable gravity field on a global scale to further improve our understanding of climate change processes and geophysical phenomena on scales of a few hundreds of kilometres. The users of gravity field products, however, require higher accuracies and a better spatial and/or temporal resolution, which are not met yet. The current GRACE-FO mission is not only limited by its observational geometry but also by limitations of current instruments, like electrostatic accelerometers. These challenges are partly tackled by current ESA and NASA initiatives to realise satellite gravimetry missions with overlapping mission lifetimes at different orbits. The sensor issue is addressed by the Cold Atom Rubidium Interferometer in Orbit for Quantum Accelerometer – Pathfinder Mission Preparation (CARIOQA-PMP) project. The main goal of CARIOQA-PMP is the preparation of a pathfinder mission with view to demonstrating an atom-quantum accelerometer in space within this decade and to realise a technological and programmatic roadmap for a quantum space gravimetry mission meeting user demands from a wide range of applications. This presentation will give an overview of the scientific activities within CARIOQA-PMP. These include the definition of the quantum pathfinder mission concept, the development of tools to simulate the quantum accelerometer and to estimate its performance, and to evaluate current end-user requirements, including the development of mission designs addressing these needs.CARIOQA-PMP is funded by the European Union., The 28th IUGG General Assembly (IUGG2023) (Berlin 2023)

Published
2023

5. CARIOQA : a pathfinder for space atom interferometry

Author

Beaufils, Quentin, Allard, Baptiste, Battelier, Baptiste, Bouyer, P., Fallet, Christine, Gaaloul, Naceur, Gauguet, Alexandre, Lévèque, Thomas, Pereira dos Santos, Franck, Rasel, Ernst, Schubert, Christian, Systèmes de Référence Temps Espace (SYRTE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Collisions Agrégats Réactivité (LCAR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche « Matière et interactions » (FeRMI), Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Photonique, Numérique et Nanosciences (LP2N), Université de Bordeaux (UB)-Institut d'Optique Graduate School (IOGS)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Leibniz Universität Hannover=Leibniz University Hannover, and Pereira Dos Santos, Franck

Subjects
[PHYS]Physics [physics], [PHYS] Physics [physics]
Published
2022

6. Design of a dual species atom interferometer for space

Author

Schuldt, Thilo, Schubert, Christian, Krutzik, Markus, Bote, Lluis Gesa, Gaaloul, Naceur, Hartwig, Jonas, Ahlers, Holger, Herr, Waldemar, Posso-Trujillo, Katerine, Rudolph, Jan, Seidel, Stephan, Wendrich, Thijs, Ertmer, Wolfgang, Herrmann, Sven, Kubelka-Lange, André, Milke, Alexander, Rievers, Benny, Rocco, Emanuele, Hinton, Andrew, Bongs, Kai, Oswald, Markus, Franz, Matthias, Hauth, Matthias, Peters, Achim, Bawamia, Ahmad, Wicht, Andreas, Battelier, Baptiste, Bertoldi, Andrea, Bouyer, Philippe, Landragin, Arnaud, Massonnet, Didier, Lévèque, Thomas, Wenzlawski, Andre, Hellmig, Ortwin, Windpassinger, Patrick, Sengstock, Klaus, von Klitzing, Wolf, Chaloner, Chris, Summers, David, Ireland, Philip, Mateos, Ignacio, Sopuerta, Carlos F., Sorrentino, Fiodor, Tino, Guglielmo M., Williams, Michael, Trenkel, Christian, Gerardi, Domenico, Chwalla, Michael, Burkhardt, Johannes, Johann, Ulrich, Heske, Astrid, Wille, Eric, Gehler, Martin, Cacciapuoti, Luigi, Gürlebeck, Norman, Braxmaier, Claus, and Rasel, Ernst

Published
2015
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7. CARIOQA : a test bench for space atom interferometry - Mission definition and performances evaluation

Author

Beaufils, Quentin, Allard, Baptiste, Battelier, Baptiste, Bouyer, P., Fallet, Christine, Gaaloul, Naceur, Gauguet, Alexandre, Lévèque, Thomas, Pereira dos Santos, Franck, Rasel, Ernst, Schubert, Christian, Systèmes de Référence Temps Espace (SYRTE), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Collisions Agrégats Réactivité (LCAR), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Fédération de recherche « Matière et interactions » (FeRMI), Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Centre National de la Recherche Scientifique (CNRS)-Institut National des Sciences Appliquées - Toulouse (INSA Toulouse), Institut National des Sciences Appliquées (INSA)-Université de Toulouse (UT)-Institut National des Sciences Appliquées (INSA)-Centre National de la Recherche Scientifique (CNRS), Laboratoire Photonique, Numérique et Nanosciences (LP2N), Université de Bordeaux (UB)-Institut d'Optique Graduate School (IOGS)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), Leibniz Universität Hannover=Leibniz University Hannover, Etienne Augé, Jacques Dumarchez and Jean Trân Thanh Vân, and Pereira Dos Santos, Franck

Subjects
[PHYS]Physics [physics], [PHYS] Physics [physics]
Abstract

International audience

Published
2022

8. 1.5 µm - optical frequency standard iodine stabilized in the 10-15 range for space-mission applications

Author

Philippe, Charles, Le Targat, Rodolphe, Holleville, David, Lours, Michel, Wolf, Peter, Lévèque, Thomas, Le Goff, Roland, Acef, Ouali, Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Métrologie des fréquences optiques, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), and SODERN

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; We report on the development of an optical frequency standard (OFS) operating in the C-Telecom band, stabilized in the 10-15 range, using Doppler-free spectroscopy of iodine hyperfine line around 514 nm. To bridge the frequency gap between infrared (IR) and green domains, we operate an efficient frequency tripling process of the IR laser diode, with two cascaded nonlinear Lithium Niobate crystals. We have implemented an original optical arrangement which allows a high efficiency optical power conversion (P  P), yielding to 300 mW at 514 nm. The generated green optical power is 20 times higher than the optical level required for the frequency stabilization purpose. We have demonstrated a residual frequency instability of 4.8 x 10-14 τ-1/2 with a minimum value of 6 x 10-15 conferred to a butterfly laser diode emitting at 1542 nm. A novel demonstrator-fully fibered iodine stabilized laser system is under development to match several space missions requirements

Published
2017

11. A COMPACT FREQUENCY STABILIZED TELECOM LASER DIODE FOR SPACE APPLICATIONS

Author

Philippe, Charles, Holleville, David, Le Targat, Rodolphe, Wolf, Peter, Lévèque, Thomas, Le Goff, Roland, Martaud, Emmanuelle, Acef, Ouali, Henry, Florence, Systèmes de Référence Temps Espace (SYRTE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS), Métrologie des fréquences optiques, Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Centre National d'Études Spatiales [Toulouse] (CNES), and SODERN

Subjects
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], [PHYS.ASTR] Physics [physics]/Astrophysics [astro-ph]
Abstract

International audience; We report on a Telecom laser diode (LD) frequency stabilization to a narrow iodine hyperfine line in the green range, after frequency tripling process using fibered nonlinear waveguide PPLN crystals. We have generated up to 300 mW optical power in the green range (~514 nm) from 800 mW of infrared power (~1542 nm), corresponding to a nonlinear conversion efficiency  = P3/P ~ 36%. Less than 10 mW of the generated green power are used for Doppler-free spectroscopy of 127I2 molecular iodine, and therefore- for the frequency stabilization purpose. The frequency tripling optical setup is very compact (< 5 l), fully fibered, and could operate over the full C-band of the Telecom range (1530 nm 1565 nm). Several thousands of hyperfine iodine lines may thus be interrogated in the 510 nm 521 nm range. We build up an optical bench used at first in free space configuration, using the well-known modulation transfer spectroscopy technique (MTS), in order to test the potential of this new frequency standard based on the couple 1.5 µm laser / iodine molecule. We have already demonstrated a preliminary frequency stability of 4.8 x 10-14  -1/2 with a minimum value of 6 x 10-15 reached after 50 s of integration time, conferred to a laser diode operating at 1542.1 nm. We focus now our efforts to expand the frequency stability to a longer integration time in order to meet requirements of many space experiments, such earth gravity missions, inters satellites links or space to ground communications. Furthermore, we investigate the potential of a new approach based on frequency modulation technique (FM), associated to a 3rd harmonic detection of iodine lines to increase the compactness of the optical setup.

Published
2016

14. Free space optical link to a tethered balloon for frequency transfer and chronometric geodesy.

Author

Maron N, Fernandez S, Esnault FX, Lévèque T, Muzeau T, and Wolf P

Abstract

We present the results of an optical link to a corner cube on board a tethered balloon at 300 m altitude including a Tip/Tilt compensation for the balloon tracking. Our experiment measures the carrier phase of a 1542 nm laser, which is the useful signal for frequency comparison of distant clocks. An active phase noise compensation of the carrier is implemented, demonstrating a fractional frequency stability of 8 × 10 -19 after 16 s averaging, which slightly (factor ∼ 3) improves on best previous links via an airborne platform. This state-of-the-art result is obtained with a transportable set-up that enables a fast field deployment.

Published
2024
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