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Articles: 2'143'162
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08 December 2021
 
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Results 1 to 20 of 819'893 for query "by". (0.07 sec.)

[    1    2    3    4    5    10    ]   Next
1.
Status of the Hadronic Light-by-Light Contribution to the Muon Anomalous Magnetic Moment
Johan Bijnens; Joaquim Prades;
29 Jan 2007
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2.
Measurement of Non-Random Event-by-Event Fluctuations of Average Transverse Momentum in sqrt(s_NN)=200 GeV Au+Au and p+p Collisions
the PHENIX Collaboration: S.S. Adler; et al;
6 Oct 2003   /  Phys.Rev.Lett. 93 (2004) 092301
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3.
Wigner's new physics frontier: Physics of two-by-two matrices, including the Lorentz group and optical instruments
Sibel Baskal; Elena Georgieva; Y. S. Kim;
31 Oct 2003
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4.
Interstellar extinction by fractal polycrystalline graphite clusters?
A.C. Andersen; J.A. Sotelo; V.N. Pustovit; G.A. Niklasson;
14 Nov 2001   /  2002, Electromagnetic and Light Scattering by Non-spherical Particles, Army Research Laboratory (ISBN 0-9702316-2-8), 1-4
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5.
Lattice points on the plane ax+by+cz=d and the diophantine system ax+by+cz=d ex+fy+gz=h
Konstantine Zelator;
12 May 2008
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6.
Validation of Time-Distance Helioseismology by Use of Realistic Simulations of Solar Convection
Junwei Zhao; Dali Georgobiani; Alexander G. Kosovichev; David Benson; Robert F. Stein; Åke Nordlund;
19 Dec 2006
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7.
How to Measure Specific Heat Using Event-by-Event Average $p_T$ Fluctuations
M. J. Tannenbaum; PHENIX Collaboration;
1 Dec 2005
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8.
Suppressing cluster cooling flows by multiple AGN activity
Adi Nusser; Joseph Silk; Arif Babul; PostScript; PDF; Other formats; SLAC-SPIRES HEP; to; by; NASA ADS;
27 Feb 2006
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9.
The Large Scale Geometry of Nilpotent-by-Cyclic Groups
Ashley Reiter Ahlin;
14 Jul 2005
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10.
Reshape of the Bunch-by-bunch BPM Signal to a Turn-by-turn Matrix during the Fast RF Frequency-sweeping Time in Booster
Xi Yang; Charles M. Ankenbrandt; James Lackey; Vic Scarpine;
6 Dec 2004
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11.
Bright OB stars in the Galaxy.II. Wind variability in O supergiants as traced by H-alpha
N. Markova; J. Puls; S. Scuderi; H. Markov;
31 May 2005
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12.
Reducing Thermoelastic Noise in Gravitational-Wave Interferometers by Flattening the Light Beams
Erika D'Ambrosio; Richard O'Shaughnessy; Sergey Strigin; Kip S. Thorne; Sergey Vyatchanin;
20 Sep 2004
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13.
Imaging extrasolar planets by stellar halo suppression in separately-corrected color bands
Johanan L. Codona; Roger Angel;
18 Feb 2004   /  Astrophys.J. 604 (2004) L117-L120
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14.
Ultra High Energy Cosmic Rays, Z-Shower and Neutrino Astronomy by Horizontal-Upward Tau Air-Showers
D. Fargion;
24 Jun 2003   /  Xth Neutrino Telescope Conference-Venice,Ed. by Milla Baldo Ceolin, 11-14 March 2003,Ed.Papergraf.,Vol-II, 433-455,2003.
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15.
Comment on "Detection of small comets with a ground-based telescope" by Frank and Sigwarth
R. L. Mutel; J. D. Fix;
2 Jul 2003
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16.
Clump Development by the Nickel Bubble Effect in Supernovae
Chih-Yueh Wang;
26 Jun 2003   /  Astrophys.J. 626 (2005) 183-194
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17.
Explaining the Observed Polarization from Brown Dwarfs by Single Dust Scattering
Sujan Sengupta;
25 Dec 2002   /  Astrophys.J. 585 (2003) L155-L158
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18.
Hadronic light-by-light scattering contribution to g_{mu}-2
Andreas Nyffeler;
25 Oct 2002   /  Nucl.Phys.Proc.Suppl. 116 (2003) 225-229
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19.
Quantum size effects in the low temperature layer-by-layer growth of Pb on Ge(001)
L. Floreano; D. Cvetko; F. Bruno; G. Bavdek; A. Cossaro; R. Gotter; A. Verdini; A. Morgante;
15 Nov 2002   /  Prog. Surf. Sci. 72 (2003) 135
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20.
Hadronic light-by-light corrections to the muon g-2: the pion-pole contribution
Marc Knecht; Andreas Nyffeler;
6 Nov 2001   /  Phys.Rev. D65 (2002) 073034
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