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Nature of Reality

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Title: Nature of Reality


1
  • Nature of Reality
  • According to Einsteins
  • Statistical-Thermodynamic
  • and Geometrical ideas
  • Prof. O. Goloubjeva.
  • Prof. A.Soukhanov
  • Russia, Moscow ogol_at_oldi.ru

2
I. General introduction
  • At present time we have all the possibilities for
    the complete comprehension of Einsteins
    scientific legacy. The most important point here
    is to elucidate the role of Einsteins ideas in
    the creation of modern concepts about the nature
    of physical reality.
  • To evaluate Einsteins contribution in the world
    science and culture one must consider not only
    his papers on Physics but his achievements as a
    thinker and philosopher. He did not write pure
    philosophical works but in spite of it his
    comprehensive reflections about physics reality
    enriched humanity by new universal views on the
    Nature
  • Einstein always preferred in the Physics the
    most universal systems of views on the reality
    because he thought of as a picture of World
    must be entire. He was impressed by so-called
    Theories of Principle based on general
    features of phenomena. Such theories for him
    were the geometry and thermodynamics in the most
    wide sense of these notions ( according to
    Einstein, Physics Geometry Experience).

3
  • The concepts of geometry attracted him by the
    possibility of the invariant description of
    Nature without any specification of the
    coordinate system. These concepts were realized
    in Einsteins works on special and general
    relativity theories.
  • The concepts of thermodynamics are the most close
    to experience. They were also highly evaluated by
    Einstein due to their generalization , i.e.
    independence upon specific physical models. To
    develop and apply the thermodynamics were only
    needed the most general ideas about the
    interrelations between the material object and
    its environment, i.e. between the system and the
    thermal bath. At the same time the thermodynamics
    deals with macroscopic observables which may be
    obtained from experience

4
II. General Estimate of Einsteins Heritage
  • Philosophical and scientific ideas of Einstein
    were closely bound. But to understand his world
    outlook we start from estimating his scientific
    legacy. When one say about Einstein physicist
    the most often one refers to his world-famous
    relativistic theories. But according to well
    known scientist M. Born Einstein should be
    referred to as one of the greatest physicist of
    all times even in the case when he should write
    nothing on the relativity theory. We full agree
    upon this opinion (despite to the latest own
    Einsteins statements).
  • So let us make no mention of his relativity
    theories and concern Einsteins works on the
    statistical theories. They contain some pioneer
    basic ideas of modern essential part of Physics -
    the Statistical Thermodynamics which were
    developed by his nearest followers (Fuhrth, Laue,
    Szilard).

5
III. Short review of Einsteins statistical
theories
  • Chronologically the first of these statistical
    theories was the Statistical Mechanics in the
    phase space, which was worked out by Einstein
    simultaneously with and independent of Gibbs. As
    a byproduct of the statistical mechanics there
    appeared the fluctuations of some
    macro-parameters. But to these ones didnt
    belong intensive characteristics like a
    temperature and an entropy, having no
    mechanical analogues.
  • The second original and in fact most
    important statistical theory by Einstein, was
    the true statistical thermodynamics operating in
    the space of all macro-parameters in which he
    carried out a generalization of the zeroth law of
    thermodynamics. Einstein put forward the
    following fundamental statements
  • a temperature of any object in a thermal
    equilibrium state is only equal to a
    temperature of a thermal bath on the average and
    it has an ability to fluctuate alongside
    with other macro-parameters.

6
  • On this basis he established a fundamental sense
    and an universal formula for Boltzmann's constant
    that applied to macro-objects of any type
    calculated fluctuations of the internal energy
    and the inverse temperature of a macro-system
    that allows us to write a thermodynamic
    uncertainties relation between them depended on
    Boltzmann's constant formulated Boltzmann's
    principle and a developed the fluctuations
    theory of any macro parameters.
  • The third his statistical theory was the
    theory of Brownian motion, or the generalized
    diffusion theory, which includes the Einstein
    Fokker Planck equation. According to modern
    views, it is a fully independent from
    Statistical Mechanics theory, where coordinate
    and momentum obtain the sense of macro-
    parameters.
  • Finally, the fourth statistical theory was
    his Quantum Theory of radiation etc. Predicted
    by him a spontaneous radiation is an analogous to
    the spontaneous decay of the nucleus. This
    event opened the era of the development of
    stochastic notions on the microscopic level of
    the description of Nature.

7
IV. Entering of fundamental constants
  • Einstein's ideas have begun an independent
    description of the Nature at the macro level. He
    provided the stochastic description of Nature as
    on the microscopic as well macroscopic levels.
    Nevertheless, Einstein appeared to be the
    ancestor of qualitatively new non-classical
    views of the Nature, where the central point is
    the concept of the stochasticity of all natural
    processes.
  • Note that each of his theories (as relativistic
    as statistical) is connected with one (or more
    than one) of world constants. In particular
    constant c (velocity of light) is in
    corresponding to SRT, G (constant of
    gravitation)- to GRT, ? (Plancks constant)
    appeared due to photon hypotheses and at last kB
    (Boltzmanns constant) has an direct relationship
    to fluctuations theory. Moreover Einsteins
    radiation theory joins three constants ?, c and
    kB. . So it must be admitted that they all them
    had got the status of universal constants due to
    Einstein!

8
V. The goal of Physics
  • Let us recall that just the formation of the
    Physics Picture of World as a whole
    description is the uttermost goal of physics
    such was the opinion of many outstanding
    physicists and thinkers like Leibnitz, Mach,
    Planck and Einstein himself. That is another
    matter how entire this PPW might be in the
    final. Before Einstein Physics looked like a
    mosaic of theories sometimes even contradicting
    each other. All the work of Einstein in
    relativity theory as well as in thermodynamics
    was intended on the overcoming of this
    disconnection of various views on the Nature. He
    was sure that PPW must be entire.

9
  • The main methodological achievement of Einstein
    was demonstrating the fundamental role of two
    universal views on the Nature i.e., geometry
    and thermodynamics in the most wide sense of
    these concepts. The geometrical way of
    Einsteins thinking allowed him to realize the
    concept of integrity in the classical version of
    PPW, in which fluctuations are absent. In turn,
    the thermodynamic way of Einsteins thinking
    created the possibilities for the realization of
    the integrity concept in the non-classical
    version of PPW in which there are the
    fluctuations as extensive as intensive
    characteristics.

10
VI. Zellmanovs cube
  • The results of Einsteins studies continue to
    play the outstanding role in the acknowledgment
    of the integrity of contemporary PPW. First of
    all the question is in the discovery of
    conceptual structure of Physics. Many scientists
    were interested in this problem and suggested
    its different versions. Several of them were
    grounded on the basis composed of fundamental
    constants and connected with them theories.
  • In the thirties of XX century was realized the
    three- parametrical model of Zellmanov. The
    model was formulated in terms of only
    three fundamental constants - c, G, h. It gave
    some possibility for analysis of the
    interrelations between existing physical theories
    and stimulated the searching of the missing
    elements of the model. The model was referred to
    as Zellmanovs cube because it had got an
    obvious geometrical image in the form of cube.

11
  • In our opinion, the main shortcoming of this
    model consists in abandonment from
    consideration the fundamental Boltzmanns
    constant kB which status according Plancks
    mention (1899) is not lower than of preceding
    three constants. It means that in this model
    Physics was only reduced to the microscopic
    description.
  • In this way, from the very beginning was excluded
    the thermodynamics as an independent fundamental
    and universal physical theory. Up to
    now the all intellectual efforts to
    construct a full model didnt bring the
    expected results.

12
  • Now to construction a PPW we suggest starting
    from admitting on equal rights of all four
    fundamental physical constants. The main
    bulk of physical knowledge in our opinion may
    be classified according to two foundations the
    first are versions of PPW, while the second the
    levels of the Nature description.

13
  • Starting from the first foundation we obtain two
    versions of PPW the classical and non-classical
    ones.
  • Starting from the second foundation we suggest
    that there are two levels of the description of
    Nature the microscopic and macroscopic ones.

14
  • On this basis the special and general relativity
    theories are classical ones, whereas statistical
    thermodynamics and quantum dynamics are the
    non-classical ones.
  • On this way we take into account Einsteins
    viewpoint on fluctuations as an important
    property of Nature objects. So these versions
    differ in the following respect do or do not
    play the significant role the fluctuations of all
    the physical quantities (as well as correlations
    between them) in these theories.
  • Noticed, Micro- and macro- levels are equally
    fundamental and independent. By macroscopic
    description the outstanding role are played by
    such quantities as temperature and entropy.

15
VII. The tetrahedron
  • The main difficulty on this way looking for
    adequate geometrical image for this structure.
    As the first step it may be schematically shown
    by the aid of planar table, consisting of four
    cells. Accordingly we have four sets of
    fundamental physical theories, which are
    qualitatively different. The constants c and G
    correspond to classical theories but constants ?
    and kB correspond to non-classical ones.
  • But much more informative will be obtained by
    means of some obvious spatial image. For all
    this construction it should be the tetrahedron
    the minimal Platos body.

16
  • Every face of this body corresponds to one of the
    cells of the planar table and, consequently, to
    one of fundamental constants.

17
  • The tetrahedron suggested is the image of some
    integral physical picture of the world (IPPW).
    All the faces of the body, unifying sets of
    physical theories, together describe the Nature
    as a whole. It may be well admissible that the
    future development of physics will come towards
    the deepening of the interrelations between the
    theories on every face as well as between the
    different faces. This prognosis in our opinion
    is adequate to entire Nature.

18
VIII. Elaboration of Einsteins ideas
  • Einsteins creative heritage suggests the
    possibility also for the next step toward the
    integrity of PPW. In fact, the question is to
    generalize and to give a real content to the
    Machs principle which was highly rated by
    Einstein. In our opinion, the generalized Machs
    principle is equivalent to the following
    statement
  • any physical object besides the local
    characteristics possess also the global ones, and
    just these last ones reflect in some generalized
    way the influence of the environment on the
    object.
  • Striking examples of the global characteristics
    are the temperature in statistical thermodynamics
    (non-classical version of PPW) and the
    energy-momentum tensor in general relativity
    theory (classical version of PPW). Einstein
    explained us their physical sense and role in
    Natures description.

19
  • In this connection, grows the significance of
    another Einsteins favorite method - the
    Geometry in the wide sense. Nowadays
    geometrical ideas are wide used for
    generalization of thermodynamics.
  • Finally, one more tradition laid down by
    Einstein consists in the use of so-called
    thermodynamic envelope when developing the
    quantum views. This may be considered as the
    prologue to the creation of modern quantum field
    theory (QFT) with belonging to this theory
    universal concept of vacuum.

20
  • At the same time successfully developing are some
    versions of QFT at finite temperatures in the
    first place the thermo-field dynamics (TFD),
    which allows to combine in harmonic way the
    significant features of standard QFT and
    statistical thermodynamics. This version of QFT
    relies on the universal notion of the
    thermo-field vacuum, which combines the usual
    notions of cold vacuum and the thermal bath.
  • As a result, one may foresee the following
    possible development of theoretical physics in
    the current post-Einstein century. In our
    opinion, there should happen the combination and
    unification of the ideas originally inherent in
    Einsteins creative and seminal work i.e., his
    ideas in geometry, quantum field theory and
    statistical thermodynamics.

21
IX. Conclusion
  • As a conclusion let us present some formula,
    which symbolizes the future integrated theory of
    physics. This formula is well known about thirty
    years, but it was not yet analyzed in such a
    context we mean the Beckenstein Hawking
    formula for the entropy S of the black hole.
  • Assume for simplicity the hole as being not
    charged and not rotating then the standard form
    of this formula is the following
  • S kB(A/4L 2PL), A4pR2
  • here kB is the Boltzmanns constant LPL -
    is the Planck length
  • R is the radius of the black hole.

22
  • If one rewrites this formula, expressing Rbh
    through M the mass of the black hole and using
    further only the fundamental constants, one
    obtains S4p M2 (
    ).
  • It is not difficult to see in this formula on
    quite equal rights enter all the four fundamental
    constants. It seems us this is a very beautiful
    expression!
  • Following to Einstein, such fact hardly may be
    considered as simply accidental one!
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