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description Publicationkeyboard_double_arrow_right Article , Preprint 2007 NetherlandsAmerican Physical Society (APS) D. B. Chitwood; T. I. Banks; M. J. Barnes; S. Battu; R. M. Carey; S. Cheekatmalla; S. M. Clayton; J. Crnkovic; Kenneth M. Crowe; P. T. Debevec; S. Dhamija; W. Earle; A. Gafarov; K. L. Giovanetti; T. P. Gorringe; F. Gray; M. Hance; D. W. Hertzog; M. F. Hare; P. Kammel; B. Kiburg; J. Kunkle; B. Lauss; I. Logashenko; K. R. Lynch; R. McNabb; J. P. Miller; Françoise Mulhauser; C. J. G. Onderwater; C. S. Oezben; Q. Peng; C. C. Polly; Susanne Rath; B. L. Roberts; V. Tishchenko; G. D. Wait; J. Wasserman; D. M. Webber; P. Winter; P. A. Zolnierczuk; null null; C. S. Özben;The mean life of the positive muon has been measured to a precision of 11 ppm using a low-energy, pulsed muon beam stopped in a ferromagnetic target, which was surrounded by a scintillator detector array. The result, tau_mu = 2.197013(24) us, is in excellent agreement with the previous world average. The new world average tau_mu = 2.197019(21) us determines the Fermi constant G_F = 1.166371(6) x 10^-5 GeV^-2 (5 ppm). Additionally, the precision measurement of the positive muon lifetime is needed to determine the nucleon pseudoscalar coupling g_P. Comment: As published version (PRL, July 2007)
Physical Review Lett... arrow_drop_down Physical Review LettersArticle . 2007Physical Review LettersArticle . 2007Data sources: OD-Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.99.032001&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu43 citations 43 popularity Average influence Top 10% impulse Top 10% Powered by BIP!
more_vert Physical Review Lett... arrow_drop_down Physical Review LettersArticle . 2007Physical Review LettersArticle . 2007Data sources: OD-Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.99.032001&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2010American Physical Society (APS) NSERCNSERCAuthors: Justin Khoury; Paul J. Steinhardt;Justin Khoury; Paul J. Steinhardt;The universe can be made flat and smooth by undergoing a phase of ultra-slow (ekpyrotic) contraction, a condition achievable with a single, canonical scalar field and conventional general relativity. It has been argued, though, that generating scale-invariant density perturbations, requires at least two scalar fields and a two-step process that first produces entropy fluctuations and then converts them to curvature perturbations. In this paper, we identify a loophole in the argument and introduce an ekpyrotic model based on a single, canonical scalar field that generates nearly scale-invariant curvature fluctuations through a purely "adiabatic mechanism" in which the background evolution is a dynamical attractor. The resulting spectrum can be slightly red with distinctive non-gaussian fluctuations. Comment: 5 pages. v2: Minor corrections. v3: Expanded discussion of attractor property, included numerical work confirming scale invariance, improved notation, and added references
Physical Review Lett... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.104.091301&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu51 citations 51 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert Physical Review Lett... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.104.091301&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2017 United StatesAmerican Physical Society (APS) NSERCNSERCAuthors: Aidan Chatwin-Davies; Achim Kempf; Robert T. W. Martin;Aidan Chatwin-Davies; Achim Kempf; Robert T. W. Martin;We calculate the impact of quantum gravity-motivated ultraviolet cutoffs on inflationary predictions for the cosmic microwave background spectrum. We model the ultraviolet cutoffs fully covariantly to avoid possible artifacts of covariance breaking. Imposing these covariant cutoffs results in the production of small, characteristically $k-$dependent oscillations in the spectrum. The size of the effect scales linearly with the ratio of the Planck to Hubble lengths during inflation. Consequently, the relative size of the effect could be as large as one part in $10^5$; i.e., eventual observability may not be ruled out. Comment: 5 pages, 3 figures - v2: minor corrections, added references -v3: harmonize with published version
Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.119.031301&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu9 citations 9 popularity Average influence Average impulse Top 10% Powered by BIP!
more_vert Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.119.031301&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 1997American Physical Society (APS) G. Malka; Julien Fuchs; François Amiranoff; Sophie Baton; R. Gaillard; J. L. Miquel; Henri Pépin; Christophe Rousseaux; Guy Bonnaud; M. Busquet; L. Lours;Relativistic electrons are produced, with energies up to 20MeV, by the interaction of a high-intensity subpicosecond laser pulse (1 {mu}m , 300 fs , 10{sup 19} W/cm{sup 2} ) with an underdense plasma. Two suprathermal electron populations appear with temperatures of 1 and 3MeV. In the same conditions, the laser beam transmission is increased up to 20{percent}{endash}30{percent}. We observe both features along with the evidence of laser pulse channeling. A fluid model predicts a strong self-focusing of the pulse. Acceleration in the enhanced laser field seems the most likely mechanism leading to the second electron population. {copyright} {ital 1997} {ital The American Physical Society}
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.79.2053&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu89 citations 89 popularity Average influence Top 10% impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.79.2053&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2003American Physical Society (APS) Authors: Ronen Segev; Morris Benveniste; Yoash Shapira; Eshel Ben-Jacob;Ronen Segev; Morris Benveniste; Yoash Shapira; Eshel Ben-Jacob;pmid: 12732015
Ordinarily, in vitro neurons self-organize into homogeneous networks of single neurons linked by dendrites and axons. We show that under special conditions they can also self-organize into neuronal clusters, which are linked by bundles of axons. Multielectrode array measurement reveals that the clusterized networks are also electrically active and exhibit synchronized bursting events similar to those observed in the homogeneous networks. From time-lapse recording, we deduced the features required for the neuronal clusterized versus homogeneous self-organization and developed a simple model for testing their validity.
add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.90.168101&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu86 citations 86 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.90.168101&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 1996American Physical Society (APS) NSERCNSERCAuthors: Anatoly Malevanets; Raymond Kapral;Anatoly Malevanets; Raymond Kapral;The existence of stable links and knots is demonstrated in three-dimensional, bistable, chemical media. The reaction-diffusion medium segregates into regions of high and low concentration separated by sharp interfaces. The interfaces repel at short distances so that domains with various topologies are possible depending on the initial conditions and system parameters. Front instabilities can give rise to knotted labyrinthine patterns. A lattice-gas model whose mean-field limit is the FitzHugh-Nagumo equation is described and implemented to carry out the simulations. Comment: 4 pages, typeset by REVTeX
Physical Review Lett... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.77.767&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu20 citations 20 popularity Average influence Top 10% impulse Average Powered by BIP!
more_vert Physical Review Lett... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.77.767&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2015American Physical Society (APS) NSERCNSERCAuthors: Gabriel Kocher; Nikolas Provatas;Gabriel Kocher; Nikolas Provatas;A new phase field crystal (PFC) type theory is presented, which accounts for the full spectrum of solid-liquid-vapor phase transitions within the framework of a single density order parameter. Its equilibrium properties show the most quantitative features to date in PFC modelling of pure substances, and full consistency with thermodynamics in pressure-volume-temperature space is demonstrated. A method to control either the volume or the pressure of the system is also introduced. Non-equilibrium simulations show that 2 and 3-phase growth of solid, vapor and liquid can be achieved, while our formalism also allows for a full range of pressure-induced transformations. This model opens up a new window for the study of pressure driven interactions of condensed phases with vapor, an experimentally relevant paradigm previously missing from phase field crystal theories. Comment: 5 pages, 4 figures, peer reviewed version
arXiv.org e-Print Ar... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.114.155501&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu43 citations 43 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!
more_vert arXiv.org e-Print Ar... arrow_drop_down add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.114.155501&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2013American Physical Society (APS) Authors: Dan Hooper; Wei Xue;Dan Hooper; Wei Xue;pmid: 25166150
The spectrum and morphology of gamma rays from the Galactic center and the spectrum of synchrotron emission observed from the Milky Way's radio filaments have each been interpreted as possible signals of ∼ 7-10 GeV dark matter particles annihilating in the inner Galaxy. In dark matter models capable of producing these signals, the annihilations should also generate significant fluxes of ∼ 7-10 GeV positrons which can lead to a distinctive bumplike feature in a local cosmic ray positron spectrum. In this Letter, we show that while such a feature would be difficult to detect with PAMELA, it would likely be identifiable by the currently operating Alpha Magnetic Spectrometer experiment. As no known astrophysical (i.e., nondark matter) sources or mechanisms are likely to produce such a sharp feature, the observation of a positron bump at around 7-10 GeV would significantly strengthen the case for a dark matter interpretation of the reported gamma-ray and radio anomalies.
Physical Review Lett... arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.110.041302&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu20 citations 20 popularity Average influence Average impulse Top 10% Powered by BIP!
more_vert Physical Review Lett... arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.110.041302&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2001American Physical Society (APS) T. Affolder; D. Amidei; J. Antos; Giorgio Apollinari; Tetsuo Arisawa; T. Asakawa; M. W. Bailey; Virgil E Barnes; Douglas Benjamin; James Bensinger; J. Berryhill; B. Bevensee; Arshad Saleem Bhatti; M. Binkley; R. E. Blair; Craig Blocker; A. Bodek; W. Bokhari; Gino Bolla; A. Brandl; N. Bruner; A. Byon-Wagner; K. L. Byrum; W. Carithers; Duncan Carlsmith; J. Cassada; Andrea Castro; D. Cauz; P. T. Chang; Chunhui Chen; Y. C. Chen; I.E. Chirikov-Zorin; L. Christofek; M. Cordelli; J. Cranshaw; Daniel P Cronin-Hennessy; R. Culbertson; Saverio D'Auria; F. DeJongh; N. Eddy; E. Engels; Q. Fan; R. G. Feild; I. Fiori; G. W. Foster; M. Franklin; J. C. Freeman; Yasuo Fukui; S. Galeotti; Michele Gallinaro; Maurice Garcia-Sciveres; Alan Garfinkel; D. W. Gerdes; P. Giannetti; P. Giromini; V. Glagolev; M. Gold; I. V. Gorelov; Y. Gotra; P. Gris; E. Hafen; R. Handler; W. Hao; Kazuhiko Hara; A. D. Hardman; Kenichi Hatakeyama; A. Heiss; C. Holck; R. J. Hollebeek; John Huth; G. Introzzi; J. Iwai; E. James; Henrik Jeldtoft Jensen; Hiroto Kambara; Teruki Kamon; K. Karr; K. Kelley; M. Kelly; R. D. Kennedy; R. Kephart; Minu Kim; S. H. Kim; Yongsun Kim; M. H. Kirby; S. Klimenko; Kostantinos Kordas; Andrey Korytov; N. Lai; S. Lami; Stephan Lammel; J. Lancaster; R. L. Lander; G. Latino; A. M. Lee; K. Lee; S. Leone; J. B. Liu; Yanwen Liu; O. Lobban; N. S. Lockyer; S. Lusin; Louis Lyons; J. Lys; Kaori Maeshima; L. Malferrari; Mosè Mariotti; A. J. Martin; J. A.J. Matthews; P. Mazzanti; A. Meyer; T. Miao; J. S. Miller; H. Minato; S. Miscetti; Guenakh Mitselmakher; T. Moulik; P. Murat; S. Murgia; S. Nahn; H. Nakada; T. Nakaya; Itsuo Nakano; C. Nelson; H. Niu; T. Ohsugi; W. Orejudos; F. Palmonari; V. Papadimitriou; D. Partos; J. Patrick; T. J. Phillips; G. Piacentino; A. Pompos; O. Pukhov; K. Ragan; D. Reher; F. Rimondi; L. Ristori; M. Riveline; W. J. Robertson; Teresa Rodrigo; A. Safonov; Richard Dante St Denis; W. K. Sakumoto; Pierre Savard; P. Schlabach; E. E. Schmidt; M. P. Schmidt; Sally Seidel; Y. Seiya; T. Shah; Marjorie Shapiro; M. J. Shochet; F. D. Snider; A. Solodsky; J. Spalding; Maria Spiropulu; Leonard Spiegel; F. Strumia; Konstanty Sumorok; T. Suzuki; T. Takano; Masaaki Tanaka; Wendy Taylor; A. S. Thompson; R. Thurman-Keup; W. Trischuk; J. F. de Troconiz; Nicola Turini; G. Velev; R. Vidal; R. Vilar; Igor Volobouev; R. G. Wagner; J. Wahl; C. H. Wang; T. L. Watts; R. C. Webb; A. B. Wicklund; S. Wolbers; S. Wolinski; Xin Wu; J. Wyss; Avraham Yagil; T. Yoshida; I. Yu; Z. Yu; Anna Zanetti; S. Zucchelli;We present the first measurement of the ratio of branching fractions R equivalent to B(t --> Wb)/B(t --> Wq) from pa collisions at roots = 1.8 TeV. The data set corresponds to 109 pb(-1) of data recorded by the Collider Detector at Fermilab during the 1992-95 Tevatron run. We measure R = 0.94(-0.24)(+0.31)(stat + syst) or R > 0.61 (0.56) at 90% (95)% C.L., in agreement with the standard model predictions. This measurement yields a limit on the Cabibbo-Kobayashi-Maskawa quark mixing matrix element \V-tb\ under the assumption of three generations and unitarity.
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You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1103/physrevlett.86.3233&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eu29 citations 29 popularity Average influence Top 10% impulse Top 10% Powered by BIP!
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Preprint , Article 2019 United States, United Kingdom, ItalyAmerican Physical Society (APS) EC | COGS, NSF | Collaborative Research: E..., NSF | Physics Frontier Center a... +6 projectsEC| COGS ,NSF| Collaborative Research: Elements: Software: NSCI: HDR: Building An HPC/HTC Infrastructure For The Synthesis And Analysis Of Current And Future Cosmic Microwave Background Datasets ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| Exploring the Time-Varying Universe at Millimeter Wavelengths with the South Pole Telescope ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,ARC| Discovery Projects - Grant ID: DP150103208 ,NSF| Collaborative Research: The Dark Energy Survey Data Management Operations ,EC| COSMICDAWN ,EC| TESTDESrinivasan Raghunathan; S. Patil; Eric J. Baxter; Bradford Benson; Lindsey Bleem; T. M. Crawford; G. P. Holder; T. McClintock; Christian L. Reichardt; T. N. Varga; Nathan Whitehorn; Peter A. R. Ade; S. Allam; Adam Anderson; Jason E. Austermann; Santiago Avila; Jessica Avva; David Bacon; J. A. Beall; Amy N. Bender; Federico Bianchini; Sebastian Bocquet; David Brooks; D. L. Burke; John E. Carlstrom; J. Carretero; F. J. Castander; C. L. Chang; H. C. Chiang; Robert I. Citron; M. Costanzi; A. T. Crites; L. N. da Costa; Shantanu Desai; H. T. Diehl; J. P. Dietrich; Matt Dobbs; Peter Doel; S. Everett; August E. Evrard; Chang Feng; B. Flaugher; Pablo Fosalba; Joshua A. Frieman; Jason Gallicchio; Juan Garcia-Bellido; Enrique Gaztanaga; Elizabeth George; Tommaso Giannantonio; A. J. Gilbert; Robert A. Gruendl; J. Gschwend; Nikhel Gupta; G. Gutierrez; T. de Haan; N. W. Halverson; N. L. Harrington; Jason W. Henning; Gene C. Hilton; Devon L. Hollowood; W. L. Holzapfel; K. Honscheid; J. D. Hrubes; N. Huang; Johannes Hubmayr; Kent D. Irwin; Tesla E. Jeltema; M. Carrasco Kind; Lloyd Knox; N. Kuropatkin; Ofer Lahav; Adrian T. Lee; Dale Li; Marcos Lima; A. E. Lowitz; M. A. G. Maia; Jennifer L. Marshall; Jeff McMahon; Peter Melchior; Felipe Menanteau; S. S. Meyer; Ramon Miquel; L. M. Mocanu; Joseph J. Mohr; Joshua Montgomery; C. Corbett Moran; Andrew Nadolski; T. Natoli; John P. Nibarger; G. I. Noble; Valentine Novosad; R. L. C. Ogando; Stephen Padin; A. A. Plazas; C. Pryke; David Rapetti; A. K. Romer; A. Roodman; A. Carnero Rosell; Eduardo Rozo; J. E. Ruhl; Eli S. Rykoff; Benjamin Saliwanchik; E. J. Sanchez; J. T. Sayre; V. Scarpine; K. K. Schaffer; Michael Schubnell; S. Serrano; I. Sevilla-Noarbe; C. Sievers; Graeme Smecher; Mathew Smith; Marcelle Soares-Santos; Antony A. Stark; K. T. Story; E. Suchyta; M. E. C. Swanson; Gregory Tarle; Carole Tucker; K. Vanderlinde; T. Veach; J. De Vicente; Joaquin Vieira; Vinu Vikram; Gensheng Wang; W. L. K. Wu; V. G. Yefremenko; Yanxi Zhang;pmid: 31763885
handle: 11368/2970925
We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole signature from stacked images formed by rotating the cluster-centered Stokes $Q/U$ map cutouts along the direction of the locally measured background CMB polarization gradient. Using data from the SPTpol 500 deg$^{2}$ survey at the locations of roughly 18,000 clusters with richness $\lambda \ge 10$ from the Dark Energy Survey (DES) Year-3 full galaxy cluster catalog, we detect lensing at $4.8\sigma$. The mean stacked mass of the selected sample is found to be $(1.43 \pm 0.4)\ \times 10^{14}\ {\rm M_{\odot}}$ which is in good agreement with optical weak lensing based estimates using DES data and CMB-lensing based estimates using SPTpol temperature data. This measurement is a key first step for cluster cosmology with future low-noise CMB surveys, like CMB-S4, for which CMB polarization will be the primary channel for cluster lensing measurements. Comment: 10 pages, 3 figures, 1 table; typos fixed; accepted for publication in PRL
Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu9 citations 9 popularity Top 10% influence Average impulse Top 10% Powered by BIP!
visibility 0visibility views 0 download downloads 5 Powered bymore_vert Caltech Authors arrow_drop_down Physical Review LettersArticleLicense: publisher-specific, author manuscriptData sources: UnpayWalladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
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description Publicationkeyboard_double_arrow_right Article , Preprint 2007 NetherlandsAmerican Physical Society (APS) D. B. Chitwood; T. I. Banks; M. J. Barnes; S. Battu; R. M. Carey; S. Cheekatmalla; S. M. Clayton; J. Crnkovic; Kenneth M. Crowe; P. T. Debevec; S. Dhamija; W. Earle; A. Gafarov; K. L. Giovanetti; T. P. Gorringe; F. Gray; M. Hance; D. W. Hertzog; M. F. Hare; P. Kammel; B. Kiburg; J. Kunkle; B. Lauss; I. Logashenko; K. R. Lynch; R. McNabb; J. P. Miller; Françoise Mulhauser; C. J. G. Onderwater; C. S. Oezben; Q. Peng; C. C. Polly; Susanne Rath; B. L. Roberts; V. Tishchenko; G. D. Wait; J. Wasserman; D. M. Webber; P. Winter; P. A. Zolnierczuk; null null; C. S. Özben;The mean life of the positive muon has been measured to a precision of 11 ppm using a low-energy, pulsed muon beam stopped in a ferromagnetic target, which was surrounded by a scintillator detector array. The result, tau_mu = 2.197013(24) us, is in excellent agreement with the previous world average. The new world average tau_mu = 2.197019(21) us determines the Fermi constant G_F = 1.166371(6) x 10^-5 GeV^-2 (5 ppm). Additionally, the precision measurement of the positive muon lifetime is needed to determine the nucleon pseudoscalar coupling g_P. Comment: As published version (PRL, July 2007)
Physical Review Lett... arrow_drop_down Physical Review LettersArticle . 2007Physical Review LettersArticle . 2007Data sources: OD-Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eu43 citations 43 popularity Average influence Top 10% impulse Top 10% Powered by BIP!
more_vert Physical Review Lett... arrow_drop_down Physical Review LettersArticle . 2007Physical Review LettersArticle . 2007Data sources: OD-Maastricht University | MUMC+ Research Informationadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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