C.W.F. Everitt
Stanford University
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Featured researches published by C.W.F. Everitt.
Classical and Quantum Gravity | 2001
John Mester; R. Torii; Paul Worden; N. A. Lockerbie; S. Vitale; C.W.F. Everitt
The Satellite Test of the Equivalence Principle (STEP) will test the equality of fall of objects in Earth orbit to an accuracy approaching one part in 108 by measuring the difference in rate of fall of test cylinders in cryogenic differential accelerometers in a drag-free satellite. This paper describes the current baseline design and principles used in the design of the STEP mission.
Advances in Space Research | 1989
John P. Turneaure; C.W.F. Everitt; Bradford W. Parkinson; Doron Bardas; John V. Breakwell; Sasha Buchman; W.S. Cheung; D.E. Davidson; D. DeBra; William M. Fairbank; Salah El-Din Feteih; D. Gill; R. Hacker; G. M. Keiser; James M. Lockhart; Barry Muhlfelder; Richard T. Parmley; Xinhua Qin; M.A. Taber; R.A. Van Patten; Y.M. Xiao; Pingli Zhou
The Gravity-Probe-B Relativity Gyroscope Experiment (GP-B) will measure the geodetic and frame-dragging precession rates of gyroscopes in a 650 km high polar orbit about the earth. The goal is to measure these two effects, which are predicted by Einsteins General Theory of Relativity, to 0.01% (geodetic) and 1% (frame-dragging). This paper presents the development progress for full-size prototype flight hardware including the gyroscopes, gyro readout and magnetic shielding system, and an integrated ground test instrument. Results presented include gyro rotor mass-unbalance values (15–86 nm) due the thickness variations of the thin niobium coating on the rotor, interior sphericities (163–275 nm peak-to-valley) of fused-quartz gyro housings produced by tumble lapping, gyro precession rates (gyroscopes at 5 K) which imply low mass-unbalance components parallel to the gyro axis (23–62 nm), and demonstration of a magnetic shielding factor of 2×1010 for the gyro readout system with one shielding component missing (the gyro rotor). All of these results are at or near flight requirements for the GP-B Science Mission, which is expected to be launched in 1995.
International Journal of Modern Physics A | 1996
Paul S. Wesson; J. Ponce De Leon; Hongya Liu; Bahram Mashhoon; D. Kalligas; C.W.F. Everitt; A. Billyard; Paul H. Lim; James M. Overduin
We unify the gravitational field with its source by considering a new type of 5D manifold in which space and time are augmented by an extra dimension which induces 4D matter. The classical tests of relativity are satisfied, and for solitons we obtain new effects which can be tested astrophysically. The canonical cosmological models are in agreement with observations, and we gain new insight into the nature of the big bang. Our inference is that the world may be pure geometry in 5D.
Classical and Quantum Gravity | 2015
C.W.F. Everitt; Barry Muhlfelder; D. DeBra; Brad Parkinson; John P. Turneaure; A S Silbergleit; E B Acworth; M Adams; Ronald J. Adler; William J. Bencze; J E Berberian; R J Bernier; K A Bower; Robert W. Brumley; Sasha Buchman; K Burns; B. Clarke; John Conklin; M L Eglington; G Green; Gregory M. Gutt; D H Gwo; G Hanuschak; X He; M I Heifetz; David Hipkins; T. Holmes; R A Kahn; G. M. Keiser; J. Kozaczuk
The Gravity Probe B mission provided two new quantitative tests of Einsteins theory of gravity, general relativity (GR), by cryogenic gyroscopes in Earths orbit. Data from four gyroscopes gave a geodetic drift-rate of −6601.8 ± 18.3 marc-s yr−1 and a frame-dragging of −37.2 ± 7.2 marc-s yr−1, to be compared with GR predictions of −6606.1 and −39.2 marc-s yr−1 (1 marc-s = 4.848 × 10−9 radians). The present paper introduces the science, engineering, data analysis, and heritage of Gravity Probe B, detailed in the accompanying 20 CQG papers.
Advances in Space Research | 2003
John P. Turneaure; C.W.F. Everitt; Brad Parkinson; Doron Bardas; Sasha Buchman; D. DeBra; H. J. Dougherty; Dale Gill; J. Grammer; G. B. Green; Gregory M. Gutt; D.-H. Gwo; M. Heifetz; N.J. Kasdin; G. M. Keiser; John A. Lipa; J.M. Lockhart; John Mester; Barry Muhlfelder; R.T. Parmley; A S Silbergleit; M. Sullivan; M. A. Taber; R.A. Van Patten; R. H. Vassar; S. Wang; Y.M. Xiao; P. Zhou
Abstract Gravity Probe B is an experiment to measure the geodetic and frame-dragging precessions, relative to the “fixed” “stars”, of a gyroscope placed in a 650 km altitude polar orbit about the earth. For Einsteins general relativity, the precessions are calculated to be 6.6 arcsec/yr for the geodetic precession and 0.042 arcsec/yr for the frame-dragging precession. The goal of the experiment is to measure these precessions to better than 0.01% and 1%, respectively. This paper gives an overview of the experiment and a discussion of the flight hardware development and its status. This paper also includes an estimate of the geodetic and frame-dragging errors expected for the experiment.
Advances in Space Research | 2000
Paul Worden; R. Torii; John Mester; C.W.F. Everitt
Abstract The foundation of modern gravitational theory is the Equivalence Principle. General Relativity is incompatible with theories of other fundamental forces such as QED, suggesting that it is incomplete. For example, there may be additional forces coupled to baryon number or spin. In this case the Equivalence Principle may be violated below the experimentally verified level of one part in 10 12 . A violation could provide crucial information for new theories. A team of US and European scientists has assembled to do the Satellite Test of the Equivalence Principle (STEP) with the goal of improving this measurement to 1 part in 10 18 . In STEP two or more test masses “fall” around the earth in a drag free satellite. A difference in the rate of fall appears as a periodic difference in their acceleration. The test masses are cooled to less than 2K and are supported by frictionless superconducting bearings. Ultra-sensitive SQUID position sensors measure their relative motion and their common motion is removed by adjustments during acceleration maneuvers. Any Equivalence Principle signal is separated from major disturbances by rotation of the spacecraft. STEP is planned to be launched by 2004, with nominal mission lifetime of 6 months.
Classical and Quantum Gravity | 2015
A S Silbergleit; John Conklin; M I Heifetz; T. Holmes; J. Li; Ilya Mandel; V G Solomonik; K Stahl; Paul Worden; C.W.F. Everitt; M Adams; J E Berberian; William J. Bencze; B. Clarke; A Al-Jadaan; G. M. Keiser; J. Kozaczuk; M Al-Meshari; Barry Muhlfelder; Michael Salomon; David I. Santiago; B Al-Suwaidan; John P. Turneaure; J Wade
The results of the Gravity Probe B relativity science mission published in Everitt et al (2011 Phys. Rev. Lett. 106 221101) required a rather sophisticated analysis of experimental data due to several unexpected complications discovered on-orbit. We give a detailed description of the Gravity Probe B data reduction. In the first paper (Silbergleit et al Class. Quantum Grav. 22 224018) we derived the measurement models, i.e., mathematical expressions for all the signals to analyze. In the third paper (Conklin et al Class. Quantum Grav. 22 224020) we explain the estimation algorithms and their program implementation, and discuss the experiment results obtained through data reduction. This paper deals with the science data preparation for the main analysis yielding the relativistic drift estimates.
Classical and Quantum Gravity | 2015
John Conklin; M I Heifetz; T. Holmes; M Al-Meshari; Bradford W. Parkinson; A S Silbergleit; C.W.F. Everitt; A Al-Jaadan; G. M. Keiser; Barry Muhlfelder; V G Solomonik; H Aljabreen
This paper provides detailed descriptions of the numerical estimation algorithms used to fit physics-based models to the data from the Gravity Probe B spacecraft, as well as the scientific results of the experiment, and the statistical and systematic uncertainties. The first paper in this series of three data analysis papers derives the mathematical expressions for the signals to be analyzed, and the second paper deals with science data acquisition and their preparation for the relativistic drift rate estimation. The data from each of the four gyroscopes are partitioned into six segments, each spanning several weeks to several months. These segments are first analyzed individually to check the validity of the mathematical models and the accuracy of the estimation routine by examining the consistency of the relativistic drift rate estimates from each of these 24 gyro-segments. Then, the drift rate estimates and uncertainties are calculated for each individual gyroscope and for the four gyroscopes combined. These results are presented and compared with each other and with the prediction of general relativity.
Classical and Quantum Gravity | 2015
A S Silbergleit; G. M. Keiser; John P. Turneaure; John Conklin; C.W.F. Everitt; M I Heifetz; T. Holmes; Paul Worden
Gravity Probe B (GP-B) was a cryogenic, space-based experiment testing the geodetic and frame-dragging predictions of Einsteins theory of general relativity (GR) by means of gyroscopes in Earth orbit. This first of three data analysis papers reviews the GR predictions and details the models that provide the framework for the relativity analysis. In the second paper we describe the flight data and their preprocessing. The third paper covers the algorithms and software tools that fit the preprocessed flight data to the models to give the experimental results published in Everitt et al (2011 Phys. Rev. Lett. 106 221101–4).
Cryogenic Optical Systems and Instruments II | 1986
C.W.F. Everitt; D.E. Davidson; R.A. Van Patten
This paper describes the design, development and preliminary testing of the cryogenic star-tracking telescope used as an optical reference for the gyroscopes in the Gravity Probe B Relativity Gyroscope experiment. The telescope is operated at 1.8 K; it is fabricated entirely from fused quartz components held together by optical contacting; it has a physical length of 14 in, a focal length of 150 in and an aperture of 5.6 in. Readout is by two photomultiplier chopper-detector assemblies at ambient satellite temperature. When fully operational the telescope may be expected to have a precision approaching 0.1 marc-s over a linear range of ±70 marc-s. Its projected noise performance corresponds to an angular resolution of 1 marc-s in 1 Hz bandwidth. The paper includes a theoretical analysis, a description of the design and fabrication of a laboratory version of the telescope, a discussion of techniques of optical contacting, an account of vibration tests on a separate mass model of the telescope, a description of the artificial star developed for optical tests, and an account of preliminary experimental results.