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Author

Christian Schubert

Other affiliations: German Aerospace Center
Bio: Christian Schubert is an academic researcher from Leibniz University of Hanover. The author has contributed to research in topics: Atom interferometer & Interferometry. The author has an hindex of 24, co-authored 76 publications receiving 2313 citations. Previous affiliations of Christian Schubert include German Aerospace Center.


Papers
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Journal ArticleDOI
TL;DR: In this paper, a new experiment using matter-wave interferometry confirms that different atoms free fall in gravity at the same rate in the same way as other atoms in the universe.
Abstract: A new experiment using matter-wave interferometry confirms that different atoms free fall in gravity at the same rate.

298 citations

Journal ArticleDOI
Yousef Abou El-Neaj1, Cristiano Alpigiani2, Sana Amairi-Pyka3, Henrique Araujo4, Antun Balaž5, Angelo Bassi6, Lars Bathe-Peters7, Baptiste Battelier8, Aleksandar Belić5, Elliot Bentine9, Jose Bernabeu10, Andrea Bertoldi8, Robert Bingham11, Robert Bingham12, Diego Blas13, Vasiliki Bolpasi14, Kai Bongs15, Sougato Bose16, Philippe Bouyer8, T. J. V. Bowcock17, William B. Bowden18, Oliver Buchmueller4, Clare Burrage19, Xavier Calmet20, Benjamin Canuel8, Laurentiu Ioan Caramete, Andrew Carroll17, Giancarlo Cella6, Vassilis Charmandaris14, S. Chattopadhyay21, S. Chattopadhyay22, Xuzong Chen23, Maria Luisa Chiofalo24, J. P. Coleman17, J. P. Cotter4, Y. Cui25, Andrei Derevianko26, Albert De Roeck27, Goran S. Djordjevic28, P. J. Dornan4, Michael Doser27, Ioannis Drougkakis14, Jacob Dunningham20, Ioana Dutan, Sajan Easo11, G. Elertas17, John Ellis29, John Ellis13, John Ellis27, Mai El Sawy30, Mai El Sawy31, Farida Fassi, D. Felea, Chen Hao Feng8, R. L. Flack16, Christopher J. Foot9, Ivette Fuentes19, Naceur Gaaloul32, A. Gauguet33, Remi Geiger34, Valerie Gibson35, Gian F. Giudice27, J. Goldwin15, O. A. Grachov36, Peter W. Graham37, Dario Grasso24, Maurits van der Grinten11, Mustafa Gündoğan3, Martin G. Haehnelt35, Tiffany Harte35, Aurélien Hees34, Richard Hobson18, Jason M. Hogan37, Bodil Holst38, Michael Holynski15, Mark A. Kasevich37, Bradley J. Kavanagh39, Wolf von Klitzing14, Tim Kovachy40, Benjamin Krikler41, Markus Krutzik3, Marek Lewicki13, Marek Lewicki42, Yu-Hung Lien16, Miaoyuan Liu23, Giuseppe Gaetano Luciano6, Alain Magnon43, Mohammed Mahmoud44, Sudhir Malik4, Christopher McCabe13, J. W. Mitchell21, Julia Pahl3, Debapriya Pal14, Saurabh Pandey14, Dimitris G. Papazoglou45, Mauro Paternostro46, Bjoern Penning47, Achim Peters3, Marco Prevedelli48, Vishnupriya Puthiya-Veettil49, J. J. Quenby4, Ernst M. Rasel32, Sean Ravenhall9, Jack Ringwood17, Albert Roura50, D. O. Sabulsky8, M. Sameed51, Ben Sauer4, Stefan A. Schäffer52, Stephan Schiller53, Vladimir Schkolnik3, Dennis Schlippert32, Christian Schubert32, Haifa Rejeb Sfar, Armin Shayeghi54, Ian Shipsey9, Carla Signorini24, Yeshpal Singh15, Marcelle Soares-Santos47, Fiodor Sorrentino6, T. J. Sumner4, Konstantinos Tassis14, S. Tentindo55, Guglielmo M. Tino56, Guglielmo M. Tino6, Jonathan N. Tinsley56, James Unwin57, Tristan Valenzuela11, Georgios Vasilakis14, Ville Vaskonen29, Ville Vaskonen13, Christian Vogt58, Alex Webber-Date17, André Wenzlawski59, Patrick Windpassinger59, Marian Woltmann58, Efe Yazgan60, Ming Sheng Zhan60, Xinhao Zou8, Jure Zupan61 
Harvard University1, University of Washington2, Humboldt University of Berlin3, Imperial College London4, University of Belgrade5, Istituto Nazionale di Fisica Nucleare6, Technical University of Berlin7, University of Bordeaux8, University of Oxford9, University of Valencia10, Rutherford Appleton Laboratory11, University of Strathclyde12, King's College London13, Foundation for Research & Technology – Hellas14, University of Birmingham15, University College London16, University of Liverpool17, National Physical Laboratory18, University of Nottingham19, University of Sussex20, Northern Illinois University21, Fermilab22, Peking University23, University of Pisa24, University of California, Riverside25, University of Nevada, Reno26, CERN27, University of Niš28, National Institute of Chemical Physics and Biophysics29, Beni-Suef University30, British University in Egypt31, Leibniz University of Hanover32, Paul Sabatier University33, University of Paris34, University of Cambridge35, Wayne State University36, Stanford University37, University of Bergen38, University of Amsterdam39, Northwestern University40, University of Bristol41, University of Warsaw42, University of Illinois at Urbana–Champaign43, Fayoum University44, University of Crete45, Queen's University Belfast46, Brandeis University47, University of Bologna48, Cochin University of Science and Technology49, German Aerospace Center50, University of Manchester51, University of Copenhagen52, University of Düsseldorf53, University of Vienna54, Florida State University55, University of Florence56, University of Illinois at Chicago57, University of Bremen58, University of Mainz59, Chinese Academy of Sciences60, University of Cincinnati61
TL;DR: The Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE) as mentioned in this paper is a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments.
Abstract: We propose in this White Paper a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments. This interdisciplinary experiment, called Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE), will also complement other planned searches for dark matter, and exploit synergies with other gravitational wave detectors. We give examples of the extended range of sensitivity to ultra-light dark matter offered by AEDGE, and how its gravitational-wave measurements could explore the assembly of super-massive black holes, first-order phase transitions in the early universe and cosmic strings. AEDGE will be based upon technologies now being developed for terrestrial experiments using cold atoms, and will benefit from the space experience obtained with, e.g., LISA and cold atom experiments in microgravity.

259 citations

Journal ArticleDOI
28 Oct 2019
TL;DR: In this paper, the authors discuss the associated scientific and technological challenges and highlights recent advances of atom interferometry in metrology, geophysics, space, civil engineering, oil and minerals exploration, and navigation.
Abstract: Since the first proof-of-principle experiments over 25 years ago, atom interferometry has matured to a versatile tool that can be used in fundamental research in particle physics, general relativity and cosmology. At the same time, atom interferometers are currently moving out of the laboratory to be used as ultraprecise quantum sensors in metrology, geophysics, space, civil engineering, oil and minerals exploration, and navigation. This Perspective discusses the associated scientific and technological challenges and highlights recent advances. Quantum sensors based on atom interferometry are moving from fundamental research towards commercial applications in metrology, geophysics, space, civil engineering, oil and minerals exploration, and navigation, but a number of challenges need to be overcome.

227 citations

Journal ArticleDOI
TL;DR: The spacetime explorer and quantum equivalence principle space test satellite mission, proposed as a medium-size mission within the Cosmic Vision program of the European Space Agency (ESA), aims for testing general relativity with high precision in two experiments by performing a measurement of the gravitational redshift of the Sun and the Moon by comparing terrestrial clocks, and by performing the universality of free fall of matter waves in the gravitational field of Earth comparing the trajectory of two Bose-Einstein condensates of 85Rb and 87Rb as mentioned in this paper.
Abstract: The theory of general relativity describes macroscopic phenomena driven by the influence of gravity while quantum mechanics brilliantly accounts for microscopic effects. Despite their tremendous individual success, a complete unification of fundamental interactions is missing and remains one of the most challenging and important quests in modern theoretical physics. The spacetime explorer and quantum equivalence principle space test satellite mission, proposed as a medium-size mission within the Cosmic Vision program of the European Space Agency (ESA), aims for testing general relativity with high precision in two experiments by performing a measurement of the gravitational redshift of the Sun and the Moon by comparing terrestrial clocks, and by performing a test of the universality of free fall of matter waves in the gravitational field of Earth comparing the trajectory of two Bose–Einstein condensates of 85Rb and 87Rb. The two ultracold atom clouds are monitored very precisely thanks to techniques of atom interferometry. This allows to reach down to an uncertainty in the Eotvos parameter of at least 2 × 10−15. In this paper, we report about the results of the phase A mission study of the atom interferometer instrument covering the description of the main payload elements, the atomic source concept, and the systematic error sources.

181 citations


Cited by
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Journal Article
TL;DR: The first direct detection of gravitational waves and the first observation of a binary black hole merger were reported in this paper, with a false alarm rate estimated to be less than 1 event per 203,000 years, equivalent to a significance greater than 5.1σ.
Abstract: On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10(-21). It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203,000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410(-180)(+160) Mpc corresponding to a redshift z=0.09(-0.04)(+0.03). In the source frame, the initial black hole masses are 36(-4)(+5)M⊙ and 29(-4)(+4)M⊙, and the final black hole mass is 62(-4)(+4)M⊙, with 3.0(-0.5)(+0.5)M⊙c(2) radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.

4,375 citations

Proceedings Article
14 Jul 1996
TL;DR: The striking signature of Bose condensation was the sudden appearance of a bimodal velocity distribution below the critical temperature of ~2µK.
Abstract: Bose-Einstein condensation (BEC) has been observed in a dilute gas of sodium atoms. A Bose-Einstein condensate consists of a macroscopic population of the ground state of the system, and is a coherent state of matter. In an ideal gas, this phase transition is purely quantum-statistical. The study of BEC in weakly interacting systems which can be controlled and observed with precision holds the promise of revealing new macroscopic quantum phenomena that can be understood from first principles.

3,530 citations

Journal ArticleDOI
TL;DR: In this article, the authors present a review of the application of atomic physics to address important challenges in physics and to look for variations in the fundamental constants, search for interactions beyond the standard model of particle physics and test the principles of general relativity.
Abstract: Advances in atomic physics, such as cooling and trapping of atoms and molecules and developments in frequency metrology, have added orders of magnitude to the precision of atom-based clocks and sensors. Applications extend beyond atomic physics and this article reviews using these new techniques to address important challenges in physics and to look for variations in the fundamental constants, search for interactions beyond the standard model of particle physics, and test the principles of general relativity.

1,077 citations

Journal Article
TL;DR: In particular, the role of mesons, isobars and quarks in nuclear structure and the use of complex nuclei for probing fundamental symmetries is discussed in this paper.

665 citations