共查询到20条相似文献,搜索用时 0 毫秒
1.
Gordon McCabe 《Foundations of Physics》2010,40(6):629-637
The purpose of this paper is to elucidate, by means of concepts and theorems drawn from mathematical logic, the conditions under which the existence of a multiverse is a logical necessity in mathematical physics, and the implications of Gödel’s incompleteness theorem for theories of everything.Three conclusions are obtained in the final section: (i) the theory of the structure of our universe might be an undecidable theory, and this constitutes a potential epistemological limit for mathematical physics, but because such a theory must be complete, there is no ontological barrier to the existence of a final theory of everything; (ii) in terms of mathematical logic, there are two different types of multiverse: classes of non-isomorphic but elementarily equivalent models, and classes of model which are both non-isomorphic and elementarily inequivalent; (iii) for a hypothetical theory of everything to have only one possible model, and to thereby negate the possible existence of a multiverse, that theory must be such that it admits only a finite model. 相似文献
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B. G. Sidharth 《International Journal of Theoretical Physics》2015,54(6):2038-2041
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Abbé Georges Lemaître 《General Relativity and Gravitation》1997,29(5):641-680
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Russian Physics Journal - 相似文献
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References to energy of the universe have focussed upon the matter contribution, whereas the conservation laws must include a gravitational contribution as well. The conservation laws as applied to FRW cosmologies suggest a zero total energy irrespective of the spatial curvature when the value of the cosmological constant is taken to be zero. This result provides a useful constraint on models of the early universe and lends support to currently studied theories of the universe arising as a quantum fluctuation of the vacuum. 相似文献
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A rigorous solution of the field equations with a finite density of matter in the Universe is obtained in the context of classical gravitation theory. 相似文献
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Stan Gudder 《International Journal of Theoretical Physics》2011,50(12):3800-3811
It is first pointed out that there is a common mathematical model for the universe and the quantum computer. The former is
called the histories approach to quantum mechanics and the latter is called measurement-based quantum computation. Although
a rigorous concrete model for the universe has not been completed, a quantum measure and integration theory has been developed
which may be useful for future progress. In this work we show that the quantum integral is the unique functional satisfying
certain basic physical and mathematical principles. Since the set of paths (or trajectories) for a quantum computer is finite,
this theory is easier to treat and more developed. We observe that the sum of the quantum measures of the paths is unity and
the total interference vanishes. Thus, constructive interference is always balanced by an equal amount of destructive interference.
As an example we consider a simplified two-slit experiment. 相似文献
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Jean-Marc Bonnet-Bidaud 《Foundations of Physics》2017,47(6):851-869
In 1965, the discovery of a new type of uniform radiation, located between radiowaves and infrared light, was accidental. Known today as Cosmic Microwave background (CMB), this diffuse radiation is commonly interpreted as a fossil light released in an early hot and dense universe and constitutes today the main ’pilar’ of the big bang cosmology. Considerable efforts have been devoted to derive fundamental cosmological parameters from the characteristics of this radiation that led to a surprising universe that is shaped by at least three major unknown components: inflation, dark matter and dark energy. This is an important weakness of the present consensus cosmological model that justifies raising several questions on the CMB interpretation. Can we consider its cosmological nature as undisputable? Do other possible interpretations exist in the context of other cosmological theories or simply as a result of other physical mechanisms that could account for it? In an effort to questioning the validity of scientific hypotheses and the under-determination of theories compared to observations, we examine here the difficulties that still exist on the interpretation of this diffuse radiation and explore other proposed tracks to explain its origin. We discuss previous historical concepts of diffuse radiation before and after the CMB discovery and underline the limit of our present understanding. 相似文献
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Exact solutions of the Lagrange equations in the Logunov metric are found in the context of classical gravitation theory. 相似文献
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Paul Halpern 《General Relativity and Gravitation》2003,35(2):251-261
We consider a five dimensional vacuum cosmology with Bianchi type-IX spatial geometry and an extra non-compact coordinate. Finding a new class of solutions, we examine and rule out the possibility of deterministic chaos. We interpret this result within the context of induced matter theory. 相似文献
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B. G. Sidharth 《Foundations of Physics Letters》2004,17(5):503-506
Extending the result of a previous paper, wherein elementary particles were considered to be an array of Planck scale oscillators, we show that the universe itself is the normal mode of a set of Planck scale oscillators. 相似文献
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O. K. Davtyan 《Annalen der Physik》1979,491(3):227-237
On basis of principle of discreteness of the space and time the following relations are obtained ΛoMoc = 2π?, τoEo = 2π? and c2 = 2GMo/Λo giving the values of fundamental elements of length Λo ≈ (?G/c3)1/2, mass Mo ≈ (?c/G)1/2, time τo ≈ (?G/c5)1/2 and energy Eo ≈ (?c5/G)1/2. The geon crown of any critical system and the crown of the Universe must have a thickness equal to the fundamental length Λo = 2(π?G/c3)1/2 = 5.74. 10?33 cm. Each critical system has its specific (most probable) quantum with an average invariant mass which in the case of the Universe is equal to (2π2?Hu/Gc)1/3 ≈ 300 me where Hu is Hubble's constant. There are all reasons to consider the universal virtual quanta of an invariant mass mu ≈ 300 me as carriers of gravitational, electromagnetic and nuclear fields in the Universe. 相似文献
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D.J. Schwarz 《Annalen der Physik》2003,12(4):220-270
The history of the Universe after its first second is now tested by high quality observations of light element abundances and temperature anisotropies of the cosmic microwave background. The epoch of the first second itself has not been tested directly yet; however, it is constrained by experiments at particle and heavy ion accelerators. Here I attempt to describe the epoch between the electroweak transition and the primordial nucleosynthesis. The most dramatic event in that era is the quark‐hadron transition at 10 μs. Quarks and gluons condense to form a gas of nucleons and light mesons, the latter decay subsequently. At the end of the first second, neutrinos and neutrons decouple from the radiation fluid. The quark‐hadron transition and dissipative processes during the first second prepare the initial conditions for the synthesis of the first nuclei. As for the cold dark matter (CDM), WIMPs (weakly interacting massive particles) – the most popular candidates for the CDM – decouple from the presently known forms of matter, chemically (freeze‐out) at 10 ns and kinetically at 1 ms. The chemical decoupling fixes their present abundances and dissipative processes during and after thermal decoupling set the scale for the very first WIMP clouds. 相似文献
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B S Sathyaprakash 《Pramana》2001,56(4):457-475
The new millennium will see the upcoming of several ground-based interferometric gravitational wave antennas. Within the next
decade a space-based antenna may also begin to observe the distant Universe. These gravitational wave detectors will together
operate as a network taking data continuously for several years, watching the transient and continuous phenomena occurring
in the deep cores of astronomical objects and dense environs of the early Universe where gravity was extremely strong and
highly nonlinear. The network will listen to the waves from rapidly spinning non-axisymmetric neutron stars, normal modes
of black holes, binary black hole inspiral and merger, phase transitions in the early Universe, quantum fluctuations resulting
in a characteristic background in the early Universe. The gravitational wave antennas will open a new window to observe the
dark Universe unreachable via other channels of astronomical observations. 相似文献
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天体神秘而奇妙,为探索其奥秘,天文学家和物理学家建立了一系列关于天体运动的理论,以此为素材的问题孕育而生.以下例析此类问题,让我们共同领略自然界的神奇魅力. 相似文献
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The most striking observable feature of our indeterministic quantum universe is the wide range of time, place, and scale on
which the deterministic laws of classical physics hold to an excellent approximation. This essay describes how this domain
of classical predictability of every day experience emerges from a quantum theory of the universe’s state and dynamics. 相似文献
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Russian Physics Journal - 相似文献