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Articles: 2'506'133
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26 April 2024
 
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Results 1 to 20 of 1'607 for query "A.Cumming". (0.02 sec.)

[    1    2    3    4    5    10    ]   Next

1.
On the possibility of a helium white dwarf donor in the presumed ultracompact binary 2S 0918-549
J.J.M. in 't Zand; A. Cumming; M.V. van der Sluys; F. Verbunt; O.R. Pols;
27 Jun 2005
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2.
Supersymmetric and Shape-Invariant Generalization for Nonresonant and Intensity-Dependent Jaynes-Cummings Systems
A.N.F. Aleixo; A.B. Balantekin; M.A. Candido Ribeiro;
4 Dec 2000   /  J.Phys. A34 (2001) 1109-1128
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3.
Progress in Absorber R&D 2: Windows
D. M. Kaplan; E. L. Black; K. W. Cassel; S. Geer; M. Popovic; S. Ishimoto; K. Yoshimura; L. Bandura; M. A. Cummings; A. Dyshkant; D. Kubik; D. Hedin; C. Darve; Y. Kuno; D. Errede; M. Haney; S. Majewski; M. Reep; D. Summers;
15 Aug 2001
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4.
Superbursts at near-Eddington mass accretion rates
J.J.M. in 't Zand; R. Cornelisse & A. Cumming;
5 Jul 2004
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5.
Progress in Absorber R&D for Muon Cooling
D. M. Kaplan; E. L. Black; M. Boghosian; K. W. Cassel; R. P. Johnson; S. Geer; C. J. Johnstone; M. Popovic; S. Ishimoto; K. Yoshimura; L. Bandura; M. A. Cummings; A. Dyshkant; D. Hedin; D. Kubik; C. Darve; Y. Kuno; D. Errede; M. Haney; S. Majewski; M. Reep; D. Summers;
15 Aug 2001   /  Nucl.Instrum.Meth. A503 (2003) 392-395
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6.
Generalized Jaynes-Cummings Model with Intensity-Dependent and Non-resonant Coupling
A. N. F. Aleixo; A. B. Balantekin; M. A. Candido Ribeiro;
12 May 2000
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7.
Supersymmetric and Shape-Invariant Generalization for Non-resonant Jaynes-Cummings Systems
A. N. F. Aleixo; A. B. Balantekin; M. A. Candido Ribeiro;
12 May 2000
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8.
A Generalized Jaynes-Cummings Hamiltonian and Supersymmetric Shape-Invariance
A.N.F. Aleixo; A.B. Balantekin; M.A. Candido Ribeiro;
13 Dec 1999   /  J.Phys. A33 (2000) 3173-3178
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9.
Exactly solvable non-Hermitian Jaynes-Cummings-type Hamiltonian admitting entirely real spectra from supersymmetry
Pijush K. Ghosh;
17 Dec 2004   /  J.Phys. A38 (2005) 7313-7324
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10.
Quantum Entangled Supercorrelated States in the Jaynes-Cummings Model
A. K. Rajagopal; K. L Jensen; F. W. Cummings;
26 Mar 1999   /  Phys.Lett. A259 (1999) 285-290
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11.
SN 1994W: evidence of explosive mass ejection a few years before explosion
Nikolai N. Chugai; Robert J. Cumming; Sergei I. Blinnikov; Peter Lundqvist; Alexei V. Filippenko; Aaron J. Barth; Angela Bragaglia; Douglas C. Leonard; Thomas Matheson; Jesper Sollerman;
8 Sep 2003
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12.
The Thermal Evolution following a Superburst on an Accreting Neutron Star
Andrew Cumming; Jared Macbeth;
15 Dec 2003   /  Astrophys.J. 603 (2004) L37-L40
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13.
An Object-Oriented Approach to Partial Wave Analysis
John P. Cummings; Dennis P. Weygand;
10 Sep 2003
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14.
Lifetime Testing 700 MHz RF Windows for the Accelerator Production of Tritium Program
K. A. Cummings; M. D. Borrego; J. DeBaca; J. S. Harrison; M. B. Rodriguez; D. M. Roybal; W. T. Roybal; S. C. Ruggles; P. A. Torrez; G. D. White;
14 Aug 2000   /  eConf C000821 (2000) THE04
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15.
The type IIn supernova 1994W: evidence for the explosive ejection of a circumstellar envelope
Nikolai N. Chugai; Sergei I. Blinnikov; Robert J. Cumming; Peter Lundqvist; Angela Bragaglia; Alexei V. Filippenko; Douglas C. Leonard; Thomas Matheson; Jesper Sollerman;
19 May 2004   /  Mon.Not.Roy.Astron.Soc. 352 (2004) 1213
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16.
Jaynes-Cummings model with degenerate atomic levels
V.A.Reshetov;
26 Feb 2000
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17.
Entanglement Sharing in the Two-Atom Tavis-Cummings Model
T. E. Tessier; I. H. Deutsch; A. Delgado; I. Fuentes-Guridi;
2 Jun 2003   /  Phys. Rev. A 68, 062316 (2003).
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18.
Models for Type I X-Ray Bursts with Improved Nuclear Physics
S. E. Woosley; A. Heger; A. Cumming; R. D. Hoffman; J. Pruet; T. Rauscher; H. Schatz; B. A. Brown; M. Wiescher;
24 Jul 2003
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19.
Recoherence in the entanglement dynamics and classical orbits in the N-atom Jaynes-Cummings model
Renato M. Angelo; Kyoko Furuya; M. Carolina Nemes; Giancarlo Q. Pellegrino;
20 Jun 2001   /  Phys. Rev. A 64, 043801 (2001)
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20.
Field Purification in the intensity-dependent Jaynes-Cummings model
D.S. Freitas; A. Vidiella-Barranco; J.A. Roversi;
15 Oct 1998   /  Phys.Lett. A249 (1998) 275-280
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