E. G. Adelberger
University of Washington
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Featured researches published by E. G. Adelberger.
Physical Review Letters | 2007
D. J. Kapner; Ted Cook; E. G. Adelberger; Jens H. Gundlach; B. R. Heckel; C. D. Hoyle; H. E. Swanson
We conducted three torsion-balance experiments to test the gravitational inverse-square law at separations between 9.53 mm and 55 microm, probing distances less than the dark-energy length scale lambda(d)=[4 -root](variant Plancks over 2pic/rho(d) approximately 85 microm. We find with 95% confidence that the inverse-square law holds (|alpha|<or=1) down to a length scale lambda=56 microm and that an extra dimension must have a size R<or=44 microm.
Reviews of Modern Physics | 1998
E. G. Adelberger; Sam M. Austin; John N. Bahcall; A. B. Balantekin; Gilles Bogaert; Lowell S. Brown; L. Buchmann; F. Edward Cecil; Arthur E. Champagne; Ludwig de Braeckeleer; C.A. Duba; S. R. Elliott; Stuart J. Freedman; Moshe Gai; G. Goldring; C. R. Gould; Andrei Gruzinov; W. C. Haxton; K. M. Heeger; Ernest M. Henley; Calvin W. Johnson; Marc Kamionkowski; R.W. Kavanagh; S. E. Koonin; K. Kubodera; Karlheinz Langanke; Tohru Motobayashi; V.R. Pandharipande; P. D. Parker; R. G. H. Robertson
We review and analyze the available information on the nuclear-fusion cross sections that are most important for solar energy generation and solar neutrino production. We provide best values for the low-energy cross-section factors and, wherever possible, estimates of the uncertainties. We also describe the most important experiments and calculations that are required in order to improve our knowledge of solar fusion rates.
Annual Review of Nuclear and Particle Science | 2003
E. G. Adelberger; and B.R. Heckel; Ann E. Nelson
▪ Abstract We review recent experimental tests of the gravitational inverse-square law and the wide variety of theoretical considerations that suggest the law may break down in experimentally accessible regions.
Physical Review Letters | 2001
C. D. Hoyle; U. Schmidt; B. R. Heckel; E. G. Adelberger; Jens H. Gundlach; D. J. Kapner; H. E. Swanson
Motivated by higher-dimensional theories that predict new effects, we tested the gravitational 1/r(2) law at separations ranging down to 218 microm using a 10-fold symmetric torsion pendulum and a rotating 10-fold symmetric attractor. We improved previous short-range constraints by up to a factor of 1000 and find no deviations from Newtonian physics.
Physical Review Letters | 2008
Stephan Schlamminger; K.-Y. Choi; T.A. Wagner; Jens H. Gundlach; E. G. Adelberger
We used a continuously rotating torsion balance instrument to measure the acceleration difference of beryllium and titanium test bodies towards sources at a variety of distances. Our result Deltaa(N),(Be-Ti)=(0.6+/-3.1)x10(-15) m/s2 improves limits on equivalence-principle violations with ranges from 1 m to infinity by an order of magnitude. The Eötvös parameter is eta(Earth,Be-Ti)=(0.3+/-1.8)x10(-13). By analyzing our data for accelerations towards the center of the Milky Way we find equal attractions of Be and Ti towards galactic dark matter, yielding eta(DM,Be-Ti)=(-4+/-7)x10(-5). Space-fixed differential accelerations in any direction are limited to less than 8.8x10(-15) m/s2 with 95% confidence.
Physical Review D | 2004
C. D. Hoyle; U. Schmidt; E. G. Adelberger; Jens H. Gundlach; B. R. Heckel; D.J. Kapner; H. E. Swanson
Motivated by a variety of theories that predict new effects, we tested the gravitational
Reviews of Modern Physics | 2010
E. G. Adelberger; Antonio Garcia; R. G. H. Robertson; K. A. Snover; A. B. Balantekin; K. M. Heeger; Michael J. Ramsey-Musolf; D. Bemmerer; A. R. Junghans; C. A. Bertulani; Jiunn-Wei Chen; H. Costantini; P. Prati; M Couder; E Uberseder; M. Wiescher; Richard H. Cyburt; B. Davids; Sj Freedman; M Gai; D Gazit; L. Gialanella; G. Imbriani; U. Greife; M Hass; W. C. Haxton; T Itahashi; K. Kubodera; K Langanke; D Leitner
{1/r}^{2}
Classical and Quantum Gravity | 2012
T.A. Wagner; E. G. Adelberger; Jens H. Gundlach; Stephan Schlamminger
law at separations between 10.77 mm and
Physical Review Letters | 2002
A. R. Junghans; E. C. Mohrmann; K. A. Snover; T. D. Steiger; E. G. Adelberger; J. M. Casandjian; H. E. Swanson; L. Buchmann; S. H. Park; A. Zyuzin
137\ensuremath{\mu}\mathrm{m}
Publications of the Astronomical Society of the Pacific | 2008
Tara Murphy; E. G. Adelberger; James Battat; Larry N. Carey; C. D. Hoyle; P. LeBlanc; Eric Leonard Michelsen; Kenneth Nordtvedt; A. E. Orin; Jana D. Strasburg; Christopher W. Stubbs; H. E. Swanson; E. Williams
using two different 10-fold azimuthally symmetric torsion pendulums and rotating 10-fold symmetric attractors. Our work improves upon other experiments by up to a factor of about 100. We found no deviation from Newtonian physics at the 95% confidence level and interpret these results as constraints on extensions of the standard model that predict Yukawa or power-law forces. We set a constraint on the largest single extra dimension (assuming toroidal compactification and that one extra dimension is significantly larger than all the others) of