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Robert Stirniman's
Antigravity Bibliography - 12
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Krech, Michael.
    The Casimir effect in critical systems / Michael Krech.  Singapore ; River
    Edge, NJ : World Scientific, c1994.  x, 253 p. : ill. ; 23 cm.
    LC CALL NUMBER: QC173.4.C74 K74 1994
    SUBJECTS: Critical phenomena. Casimir effect.
    ISBN:  9810218451

    Cavity quantum electrodynamics/edited by Paul R. Berman.  
    Boston : Academic Press, c1994.  xvi, 464 p. : ill. ; 24 cm.
    LC CALL NUMBER: QC446.2 .C38 1994
    SUBJECTS: Quantum optics. Quantum electrodynamics. Casimir effect.
    ISBN:  0120922452 (alk. paper)

    Long-range Casimir forces : theory and recent experiments on atomic systems 
    Edited by Frank S. Levin and David A. Micha.  New York : Plenum Press, c1993.
    LC CALL NUMBER: QC680 .L63 1993
    SUBJECTS: Casimir effect.
    ISBN:  0306443856

    Physics in the making : essays on developments in 20th century physics: 
    in honour of H.B.G. Casimir on the occasion of his 80th birthday/ 
    edited by A. Sarlemijn and M.J. Sparnaay.  Amsterdam : North-Holland; 
    New York, N.Y., U.S.A. : Sole distributors for the U.S.A. and Canada, 
    Elsevier Science Pub. Co., 1989.  xiv, 361 p. : ill. ; 23 cm.
    LC CALL NUMBER: QC7 .P48 1989
    SUBJECTS: Casimir, H. B. G. (Hendrik Brugt Gerhard), 1909-
      Casimir, H. B. G. (Hendrik Brugt Gerhard), 1909-
      Sarlemijn, Andries, 1936-
      Sparnaay, M. J. (Marcus Johannes)
    ISBN:  0444881212
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    Edwards-Casimir Quantum Vacuum Drive -- 
      A hypothetical drive exploiting the peculiarities of quantum
      mechanics by restricting allowed wavelengths of virtual photons
      on one side of the drive (the bow of the ship); the pressure
      generated from the unrestricted virtual photons toward the aft
      generates a net force and propels the drive.
    ----------------------------------------------------------------------

    CONDENSED MATTER, ABSTRACT COND-MAT/9505108
    From: moraes@guinness.ias.edu (Fernando Moraes)
    Date: Tue, 23 May 95 17:12:35 EDT
    Enhancement of the magnetic moment of the electron due to 
    a topological defect
    Author(s): Fernando Moraes (Institute for Advanced Study, Princeton)
      In the framework of the theory of defects/three-dimensional
      gravitation, it is obtained a positive correction to the magnetic
      moment of the electron bound to a disclination in a dielectric
      solid. With the disclination modelled as a parallel plate casimir 
      effect.

    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9212077
    From: milton@phyast.nhn.uoknor.edu (Kim Milton)
    Date: Fri, 11 Dec 92 16:13:13 CST
    MAXWELL-CHERN-SIMONS CASIMIR EFFECT, KIMBALL A. MILTON, 
    DEPARTMENT OF PHYSICS AND ASTRONOMY, UNIVERSITY OF OKLAHOMA
      In odd-dimensional spaces, gauge invariance permits a
      Chern-Simons mass term for the gauge fields in addition to the usual
      Maxwell-Yang-Mills kinetic energy term. We study the Casimir effect
      in such a (2+1)-dimensional Abelian theory. For the case of parallel
      conducting lines the result is the same as for a scalar field. For
      the case of circular boundary conditions the results are completely
      different, with even the sign of the effect being opposite for
      Maxwell-Chern-Simons fields and scalar fields. We further examine
      the effect of finite temperature. The Casimir stress is found to be
      attractive at both low and high temperature. Possibilities of
      observing this effect in the laboratory are discussed.
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC/9303038
    PHYS. REV. D 48, 776 (1993) 
    FROM: LFORD@PEARL.TUFTS.EDU
    Date: Wed, 31 Mar 1993 17:47 EDT
    MOTION OF INERTIAL OBSERVERS THROUGH NEGATIVE ENERGY, BY L.H. FORD AND 
    THOMAS A. ROMAN, 
      Recent research has indicated that negative energy fluxes due to
      quantum coherence effects obey uncertainty principle-type
      inequalities of the form $|\Delta E|\,{\Delta \tau} \lprox 1\,$.
      Here $|\Delta E|$ is the magnitude of the negative energy which is
      transmitted on a timescale $\Delta \tau$. Our main focus in this
      paper is on negative energy fluxes which are produced by the motion
      of observers through static negative energy regions. We find that
      although a quantum inequality appears to be satisfied for radially
      moving geodesic observers in two and four-dimensional black hole
      spacetimes, an observer orbiting close to a black hole will see a
      constant negative energy flux. In addition, we show that inertial
      observers moving slowly through the Casimir vacuum can achieve
      arbitrarily large violations of the inequality. It seems likely
      that, in general, these types of negative energy fluxes are not
      constrained by inequalities on the magnitude and duration of the
      flux. We construct a model of a non-gravitational stress-energy
      detector, which is rapidly switched on and off, and discuss the
      strengths and weaknesses of such a detector.
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC/9304008
    PHYS. REV. D 47, 4510 (1993).
    FROM: LFORD@PEARL.TUFTS.EDU
    Date: Tue, 6 Apr 1993 12:56 EDT
    SEMICLASSICAL GRAVITY THEORY AND QUANTUM FLUCTUATIONS, BY CHUNG-I KUO AND 
    L. H. FORD. 
      We discuss the limits of validity of the semiclassical theory of
      gravity in which a classical metric is coupled to the expectation
      value of the stress tensor. It is argued that this theory is a good
      approximation only when the fluctuations in the stress tensor are
      small. We calculate a dimensionless measure of these fluctuations
      for a scalar field on a flat background in particular cases,
      including squeezed states and the Casimir vacuum state. It is found
      that the fluctuations are small for states which are close to a
      coherent state, which describes classical behavior, but tend to be
      large otherwise. We find in all cases studied that the energy
      density fluctuations are large whenever the local energy density is
      negative. This is taken to mean that the gravitational field of a
      system with negative energy density, such as the Casimir vacuum, is
      not described by a fixed classical metric but is undergoing large
      metric fluctuations. We propose an operational scheme by which one
      can describe a fluctuating gravitational field in terms of the
      statistical behavior of test particles. For this purpose we obtain
      an equation of the form of the Langevin equation used to describe
      Brownian motion.
         
    HIGH ENERGY PHYSICS - PHENOMENOLOGY, ABSTRACT HEP-PH/9307258
    From: langfeld@ptsun1.tphys.physik.uni-tuebingen.de (Kurt Langfeld)
    Date: Tue, 13 Jul 93 08:04:30 +0200
    CASIMIR EFFECT OF STRONGLY INTERACTING SCALAR FIELDS, BY K. LANGFELD, 
    F. SCHMUSER, AND H. REINHARDT 
      Non-trivial $\phi ^{4}$-theory is studied in a renormalisation group
      invariant approach inside a box consisting of rectangular plates and
      where the scalar modes satisfy periodic boundary conditions at the
      plates. It is found that the Casimir energy exponentially approaches
      the infinite volume limit, the decay rate given by the scalar
      condensate. It therefore essentially differs from the power law of a
      free theory. This might provide experimental access to properties of
      the non-trivial vacuum. At small interplate distances the system can
      no longer tolerate a scalar condensate, and a first order phase
      transition to the perturbative phase occurs. The dependence of the
      vacuum energy density and the scalar condensate on the box
      dimensions are presented.
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC 9310007
    PHYSICA SCRIPTA 48, 649 (1993)
    FROM: harald@nordita.dk (Harald H. Soleng)
    Date: Mon, 4 Oct 93 
    INVERSE SQUARE LAW OF GRAVITATION IN (2+1)-DIMENSIONAL SPACE-TIME AS A
    CONSEQUENCE OF CASIMIR ENERGY, H. H. SOLENG, 
      The gravitational effect of vacuum polarization in space exterior to
      a particle in (2+1)-dimensional Einstein theory is investigated. In
      the weak field limit this gravitational field corresponds to an
      inverse square law of gravitational attraction, even though the
      gravitational mass of the quantum vacuum is negative. The paradox is
      resolved by considering a particle of finite extension and taking
      into account the vacuum polarization in its interior.
         
    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9312069
    From: segui@cc.unizar.es
    Date: Thu, 9 DEC 93 13:50 GMT
    A MODIFIED SCHWINGER'S FORMULA FOR THE CASIMIR EFFECT, M.V. COUGO-PINTO, C.
    FARINA AND ANTONIO J. SEGUI-SANTONJA
      After briefly reviewing how the (proper-time) Schwinger's formula
      works for computing the Casimir energy in the case of "scalar
      electrodynamics" where the boundary conditions are dictated by two
      perfectly conducting parallel plates with separation "a" in the
      Z-axis, we propose a slightly modification in the previous approach
      based on an analytical continuation method. As we will see, for the
      case at hand our formula does not need the use of Poisson summation
      to get a (renormalized) finite result.
         
    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9401123
    From: segui@cc.unizar.es
    Date: Tue, 25 JAN 94 21:47 GMT
    SCHWINGER'S METHOD FOR THE MASSIVE CASIMIR EFFECT, BY M.V. COUGO-PINTO, C.
    FARINA AND A.J. SEGUI-SANTONJA
      We apply to the massive scalar field a method recently proposed by
      Schwinger to calculate the Casimir effect. The method is applied
      with two different regularization schemes: the Schwinger original
      one by means of Poisson formula and another one by means of
      analytical continuation.
         
    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9405060
    From: Shtykov Nikolay 
    Date: Tue, 10 May 94 17:40:50 JST
    THE FINITE VACUUM ENERGY FOR SPINOR, SCALAR AND VECTOR FIELDS, N.SHTYKOV
      We compute the one-loop potential (the Casimir energy) for scalar,
      spinor and vectors fields on the spaces $\,R^{m+1}\, \times\,Y$ with
      $\,Y=\,S^N\,,CP^2$. As a physical model we consider spinor
      electrodynamics on four-dimensional product manifolds. We examine
      the cancelation of a divergent part of the Casimir energy on
      even-dimensional spaces by means of including the parameter $\,M$ in
      original action. For some models we compare our results with those
      found in the literature.
         
    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9408172
    From: LFORD@PEARL.TUFTS.EDU
    Date: Tue, 30 Aug 1994 16:45:05 -0400 (EDT)
    DECOHERENCE AND VACUUM FLUCTUATIONS, L.H. FORD, TUFTS UNIVERSITY
      The interference pattern of coherent electrons is effected by
      coupling to the quantized electromagnetic field. The amplitudes of
      the interference maxima are changed by a factor which depends upon a
      double line integral of the photon two-point function around the
      closed path of the electrons. The interference pattern is sensitive
      to shifts in the vacuum fluctuations in regions from which the
      electrons are excluded. Thus this effect combines aspects of both
      the Casimir and the Aharonov-Bohm effects. The coupling to the
      quantized electromagnetic field tends to decrease the amplitude of
      the interference oscillations, and hence is a form of decoherence.
      The contributions due to photon emission and to vacuum fluctuations
      may be separately identified. It is to be expected that photon
      emission leads to decoherence, as it can reveal which path an
      electron takes. It is less obvious that vacuum fluctuations also can
      cause decoherence. What is directly observable is a shift in the
      fluctuations due, for example, to the presence of a conducting
      plate. In the case of electrons moving parallel to conducting
      boundaries, the dominant decohering influence is that of the vacuum
      fluctuations. The shift in the interference amplitudes can be of the
      order of a few percent, so experimental verification of this effect
      may be possible. The possibility of using this effect to probe the
      interior of matter, e.g., to determine the electrical conductivity
      of a rod by means of electrons encircling it is discussed.
      (Presented at the Conference on Fundamental Problems in Quantum
      Theory, University of Maryland, Baltimore County, June 18-22, 1994.)
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC/9410043
    PHYS. REV. D 51, 4277(1995).
    FROM: FORD@TUHEP.PHY.TUFTS.EDU
    Date: Fri, 28 Oct 1994 20:33 EST
    AVERAGED ENERGY CONDITIONS AND QUANTUM INEQUALITIES, L.H. FORD AND 
    THOMAS A. ROMAN
      Connections are uncovered between the averaged weak (AWEC) and
      averaged null (ANEC) energy conditions, and quantum inequality
      restrictions on negative energy for free massless scalar fields. In
      a two-dimensional compactified Minkowski universe, we derive a
      covariant quantum inequality-type bound on the difference of the
      expectation values of the energy density in an arbitrary quantum
      state and in the Casimir vacuum state. From this bound, it is shown
      that the difference of expectation values also obeys AWEC and
      ANEC-type integral conditions. In contrast, it is well-known that
      the stress tensor in the Casimir vacuum state alone satisfies
      neither quantum inequalities nor averaged energy conditions. Such
      difference inequalities represent limits on the degree of energy
      condition violation that is allowed over and above any violation due
      to negative energy densities in a background vacuum state. In our
      simple two-dimensional model, they provide physically interesting
      examples of new constraints on negative energy which hold even when
      the usual AWEC, ANEC, and quantum inequality restrictions fail. In
      the limit when the size of the space is allowed to go to infinity,
      we derive quantum inequalities for timelike and null geodesics
      which, in appropriate limits, reduce to AWEC and ANEC in ordinary
      two-dimensional Minkowski spacetime. We also derive a quantum
      inequality bound on the energy density seen by an inertial observer
      in four-dimensional Minkowski spacetime. The bound implies that any
      inertial observer in flat spacetime cannot see an arbitrarily large
      negative energy density which lasts for an arbitrarily long period
      of time.
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC/9411053
    From: "Haret Rosu" 
    Date: 20 Nov 94 21:15:00 CST
    On the assignment of frequency spectra to quantum vacuum effects,
    Author: Haret C. Rosu,  Report: IFUG-25/94,
      I discuss in an introductory manner, i.e., in the form of comments
      on available references, the problem of assigning frequency spectra
      to such fundamental effects like Casimir, Hawking, Unruh, and
      squeezing effects. This may help to clarify their differences as
      well as their similarities.
         
    GENERAL RELATIVITY & QUANTUM COSMOLOGY, ABSTRACT GR-QC/9411056
    From: ulvi@tapir.Caltech.EDU (Ulvi Yurtsever)
    Date: Mon, 21 Nov 94 15:56:11 -0800
    The averaged null energy condition and difference inequalities in quantum 
    field theory, by: Ulvi Yurtsever
      Recently, Larry Ford and Tom Roman have discovered that in
      a flat cylindrical space, although the stress-energy tensor itself
      fails to satisfy the averaged null energy condition (ANEC) along the
      (non-achronal) null geodesics, when the ``Casimir-vacuum"
      contribution is subtracted from the stress-energy the resulting
      tensor does satisfy the ANEC inequality. Ford and Roman name this
      class of constraints on the quantum stress-energy tensor
      ``difference inequalities." Here I give a proof of the difference
      inequality for a minimally coupled massless scalar field in an
      arbitrary two-dimensional spacetime, using the same techniques as
      those we relied on to prove ANEC in an earlier paper with Robert
      Wald. I begin with an overview of averaged energy conditions in
      quantum field theory.
         
    QUANTUM PHYSICS, ABSTRACT QUANT-PH/9502024
    From: MANKO@napoli.infn.it
    Date: Mon, 27 Feb 1995 16:32:21 +0200 (CET)
    Deformation of Partical Distribution Functions due to Q-nonlinearity and
    Nonstationary Casimir Effect, Author: V. I. Man'ko
      The geometrical phase is shown to be integral of motion. Deformation
      of particle distribution function corresponding to nonstationary
      Casimir effect is expressed in terms of multivariable Hermite
      polynomials. Correction to Planck distribution due to
      q--nonlinearity is discussed.
         
    QUANTUM PHYSICS, ABSTRACT QUANT-PH/9503001
    From: onofrio%38619.hepnet@Csa4.LBL.Gov
    Date: Wed, 1 Mar 95 08:23:43 PST
    Detecting Casimir Forces through a Tunneling Electromechanical Transducer
    Authors: Roberto Onofrio , Giovanni Carugno
      We propose the use of a tunneling electromechanical transducer to
      dinamically detect Casimir forces between two conducting surfaces.
      The maximum distance for which Casimir forces should be detectable
      with our method is around $1 \mu$m, while the lower limit is given
      by the ability to approach the surfaces. This technique should
      permit to study gravitational forces on the same range of distances,
      as well as the vacuum friction provided that very low dissipation
      mechanical resonators are used.

    CONDENSED MATTER THEORY, ABSTRACT COND-MAT/9505023
    From: moraes@guinness.ias.edu (Fernando Moraes)
    Date: Fri, 5 May 95 09:35:57 EDT
    Casimir effect around disclinations
    Author: Fernando Moraes (Institute for Advanced Study, Princeton)
      This communication concerns the structure of the electromagnetic
      quantum vacuum in a disclinated insulator. It is shown that a
      nonzero vacuum energy density appears when the rotational symmetry
      of a continuous insulating elastic medium is broken by a
      disclination. An explicit expression is given for this Casimir
      energy density in terms of the parameter describing the
      disclination.

    CONDENSED MATTER THEORY, ABSTRACT COND-MAT/9505108
    From: moraes@guinness.ias.edu (Fernando Moraes)
    Date: Tue, 23 May 95 17:12:35 EDT
    Enhancement of the magnetic moment of the electron due to a topological defect
    Author: Fernando Moraes (Institute for Advanced Study, Princeton)
      In the framework of the theory of defects/three-dimensional
      gravitation, it is obtained a positive correction to the magnetic
      moment of the electron bound to a disclination in a dielectric
      solid.
         
    QUANTUM PHYSICS, ABSTRACT QUANT-PH/9506005
    From: JAEKEL Marc 
    Date: Wed, 7 Jun 1995 16:30:40 +0200
    Mechanical Effects of Radiation Pressure Quantum Fluctuations
    Authors: Marc-Thierry Jaekel (Laboratoire de Physique Th\'eorique de
    l'Ecole Normale Sup\'erieure) , Serge Reynaud (Laboratoire Kastler-Brossel)
      As revealed by space-time probing, mechanics and field theory come
      out as complementary descriptions for motions in space-time. In
      particular, quantum fields exert a radiation pressure on scatterers
      which results in mechanical effects that persist in vacuum. They
      include mean forces due to quantum field fluctuations, like Casimir
      forces, but also fluctuations of these forces and additional forces
      linked to motion. As in classical electron theory, a moving
      scatterer is submitted to a radiation reaction force which modifies
      its motional response to an applied force. We briefly survey the
      mechanical effects of quantum field fluctuations and discuss the
      consequences for stability of motion in vacuum and for position
      fluctuations.
         
    QUANTUM PHYSICS, ABSTRACT QUANT-PH/9506006
    From: JAEKEL Marc 
    Date: Wed, 7 Jun 1995 16:58:17 +0200
    Quantum Fluctuations and Inertia
    Authors: Marc-Thierry Jaekel (Laboratoire de Physique Th\'eorique de
    l'Ecole Normale Sup\'erieure) , Serge Reynaud (Laboratoire Kastler-Brossel)
      Vacuum field fluctuations exert a radiation pressure which induces
      mechanical effects on scatterers. The question naturally arises
      whether the energy of vacuum fluctuations gives rise to inertia and
      gravitation in agreement with the general principles of mechanics.
      As a new approach to this question, we discuss the mechanical
      effects of quantum field fluctuations on two mirrors building a
      Fabry-Perot cavity. We first put into evidence that the energy
      related to Casimir forces is an energy stored on field fluctuations
      as a result of scattering time delays. We then discuss the forces
      felt by the mirrors when they move within vacuum field fluctuations,
      and show that energy stored on vacuum fluctuations contributes to
      inertia in conformity with the law of inertia of energy. As a
      further consequence, inertial masses exhibit quantum fluctuations
      with characteristic spectra in vacuum.
         
    QUANTUM PHYSICS, ABSTRACT QUANT-PH/9506023
    From: claudia@cromwell.physics.uiuc.edu (Claudia C Eberlein)
    Date: Thu, 15 Jun 95 11:13:57 -0500
    Sonoluminescence as quantum vacuum radiation
    Author: Claudia Eberlein (Dept of Physics, UIUC, Urbana, IL)
      Sonoluminescence is explained in terms of quantum radiation by
      moving interfaces between media of different polarizability. It can
      be considered as a dynamic Casimir effect, in the sense that it is a
      consequence of the imbalance of the zero-point fluctuations of the
      electromagnetic field during the non-inertial motion of a boundary.
      The transition amplitude from the vacuum into a two-photon state is
      calculated in a Hamiltonian formalism and turns out to be governed
      by the transition matrix-element of the radiation pressure.
      Expressions for the spectral density and the total radiated energy
      are given.

    HIGH ENERGY PHYSICS - THEORY, ABSTRACT HEP-TH/9508086
    From: eli@ecm.ub.es (Emili Elizalde)
    Date: Fri, 18 Aug 1995 10:14:50 +0200
    A precise definition of the Casimir energy, Authors: K. Kirsten ,
                                                         E. Elizalde
      The somehow arbitrary definition of the Casimir energy corresponding
      to a quantum system in a $d$-dimensional ultrastatic spacetime
      ---profusely used in the last years--- which has been critized
      sometimes for adopting without a sound argument the minimal
      subtraction scheme, is shown to be completely equivalent to the
      definition steming naturally from the concept of functional
      determinant through the zeta-function prescription. This is done by
      considering the theory at finite temperature and by defining then
      the Casimir energy as its energy in the limit $T\to 0$. The
      ambiguity in the coefficient $C_{d/2}$ is understood to be a result
      of the necessary renormalization of the free energy of the system.
      As an example, the Casimir energy corresponding to a general
      $(1+2)$-dimensional toroidal spacetime with flat spatial geometry,
      parametrized by the corresponding Teichm\"uller parameters, and its
      precise dependence on these parameters is obtained under the form of
      an analytic function.
    ------------------------------------------------------------------------    

    Ernest G. Cullwick. In his book "Electromagnetism and Relativity", 
    published in 1957, was one of the first to provide an analysis of 
    the probable coupling between EM and inertial fields. Cullwick 
    realized that Maxwell's equations and most existing theories of 
    electrodynamics assume that the mass of an electron is zero. At 
    Maxwell's time this was a reasonable assumption. But it is well 
    known today that electrons have mass, and therefore an inertial 
    momemtum is always associated with an electric current. Cullwick 
    suggested in his analysis that coupling terms between EM and inertia 
    may be very small, but would likely appear sometime in the future 
    as we go to higher current densities. And he was one of the first 
    scientists to predict some of the odd effects which can now seen 
    with superconductors. Cullwick was also one of the first to identify 
    and attempt an analysis of the relativistic paradoxes and unusual 
    effects which occur in a rotating EM field. His work still stands 
    today as one of the only existing efforts to consider the problem 
    of a rotating EM field.

        AUTHOR:     Cullwick, E. G. (Ernest Geoffrey), 1903-
        TITLE:      Electromagnetism and relativity : with particular reference
                    to moving media and electromagnetic induction / by E. G.
                    Cullwick.
        EDITION     2d ed.
        PUBL.:      New York : J. Wiley,
        DATE:       1959 (2nd Edition)
        SUBJECT:    Electromagnetic theory, Relativity (Physics)

        AUTHOR:     Cullwick, E. G. (Ernest Geoffrey), 1903-
        TITLE:      The fundamentals of electro-magnetism by E.G. Cullwick.   
        EDITION     3rd ed. 
        PUBL.:      London, Cambridge U.P.,
        DATE:       1966 (3rd Edition)
        SUBJECT:    Electromagnetism
                   
        AUTHOR:     Cullwick, E. G. (Ernest Geoffrey), 1903-
        TITLE:      The fundamentals of electro-magnetism; a restatement for  
                    engineering students and others of physical and theoretical
                    principles in accordance with modern scientific thought,
                    by E. Geoffrey Cullwick ... With an appendix and numerous
                    examples on the recently adopted M.K.S. system of practical
                    units ...
        PUBL.:      New York, The Macmillan company; Cambridge, Eng., The
                    University press,
        DATE:       1939
        SUBJECT:    Electromagnetism
    
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