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相关论文: NASA's astonishing evidence that c is not constant…

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The fine structure constant $\alpha $ includes the speed of light as given by $\alpha =\frac{e^{2}}{4\pi \epsilon_{0}c\hbar}$. It is shown here that, following a $TH\epsilon \mu $ formalism, interpreting the permittivity $\epsilon_{0}$ and…

广义相对论与量子宇宙学 · 物理学 2009-08-25 Antonio Alfonso-Faus

We investigate how the universal constants, including the fine structure constant, have varied since the early universe close to the Planck energy scale ($E_P\sim 10^{19}$GeV) and, thus, how they have evoluted over the cosmological time…

广义相对论与量子宇宙学 · 物理学 2021-02-11 Cláudio Nassif , A. C. Amaro de Faria

The present work describes the investigation of the navigation anomaly of Pioneer 10 and 11 probes which became known as the Pioneer Anomaly. It appeared as a linear drift in the Doppler data received by the spacecraft, which has been…

广义相对论与量子宇宙学 · 物理学 2014-07-30 Dario Modenini , Paolo Tortora

In this paper, we implement a new method to test the invariance of the speed of light ($c$) as a function of redshift, by combining the measurements of galaxy cluster gas mass fraction, $H(z)$ from cosmic chronometers, and Type-Ia…

宇宙学与河外天体物理 · 物理学 2021-11-18 I. E. C. R. Mendonça , Kamal Bora , R. F. L. Holanda , Shantanu Desai , S. H. Pereira

We illustrate the energy transfer during planetary flybys as a function of time using a number of flight mission examples. The energy transfer process is rather more complicated than a monotonic increase (or decrease) of energy with time.…

天体物理学 · 物理学 2008-11-26 John D. Anderson , James K. Campbell , Michael Martin Nieto

The universe appears to be accelerating, but the reason why is a complete mystery. The simplest explanation, a small vacuum energy (cosmological constant), raises three difficult issues: why the vacuum energy is so small, why it is not…

天体物理学 · 物理学 2009-07-09 Sean M. Carroll

An additional variation of the Einstein-Hilbert action with respect to the Planck mass provides a constraint on the average Ricci scalar that prevents vacuum energy from gravitating. Consideration of the evolution of the inhomogeneous…

广义相对论与量子宇宙学 · 物理学 2019-09-18 Lucas Lombriser

No. It is simply not plausible that cosmic acceleration could arise within the context of general relativity from a back-reaction effect of inhomogeneities in our universe, without the presence of a cosmological constant or ``dark energy.''…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Akihiro Ishibashi , Robert M. Wald

The result of the OPERA experiment revealed that the velocity of muon-neutrinos was larger than the speed of light. We argue that this apparent superluminal velocity can be interpreted as a weak value, which is a new concept recently…

高能物理 - 唯象学 · 物理学 2011-10-11 Shogo Tanimura

In a recent paper (Vigoureux et al. Int. J. Theor. Phys. 47:928, 2007) it has been suggested that the velocity of light and the expansion of the universe are two aspects of one single concept connecting space and time in the expanding…

宇宙学与河外天体物理 · 物理学 2011-03-22 David Viennot , Jean-Marie Vigoureux

The Cosmic Neutrinos Background (\textbf{CNB}) are Primordial Neutrinos decoupled when the Universe was very young. Its detection is complicated, especially if we take into account neutrino mass and a possible breaking of Lorentz Invariance…

天体物理学 · 物理学 2009-02-11 Jorge Alfaro , Pablo González

Recent papers by Samuel declared that the linearized post-Newtonian v/c effects are too small to have been measured in the recent experiment involving Jupiter and quasar J0842+1845 that was used to measure the ultimate speed of gravity…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Sergei M. Kopeikin , Edward B. Fomalont

Many of the general-relativity-tests such as bending of light near a star and gravitational red/blue shift are explained without general-relativity and without Newtonian-approach. The author first casts doubts on both, the Newtonian and the…

综合物理 · 物理学 2007-05-23 Dr. R. C. Gupta

The group velocity of light in material around the AGN jet is acquiescently one (c as a unit), but this is only a hypothesis. Here, we re-derive apparent superluminal and Doppler formulas for the general case (it is assumed that the group…

高能天体物理现象 · 物理学 2015-02-25 Wen-Po Liu , Li-Yan Liu , Chun-Cheng Wang

Recent precise measurements of cosmic ray (CR) spectra show that the energy distribution of protons is softer than those of heavier nuclei, and there are spectral hardenings for all nuclear compositions above $\sim$200 GV. Models proposed…

高能天体物理现象 · 物理学 2017-08-02 Yiran Zhang , Siming Liu , Qiang Yuan

The often quoted equ. (15) in (Anderson_ea:2002) defines the observed Pioneer anomaly $a_P$ such that literal reading suggests $\nu_{obs} < \nu_{mod$ ($\nu _{obs}$ the observed (Doppler) frequency, $\nu_{mod}$ the one expected from a…

天体物理学 · 物理学 2007-08-14 Erhard Scholz

Type 1a supernovae, SNeIa, are used as standard candles in cosmology for determining the distances of the galaxies harboring them. We show that the luminosity of an SNIa depends on its distance from us when physical constants (the speed of…

广义相对论与量子宇宙学 · 物理学 2022-02-09 Rajendra P. Gupta

A possible explanation of the results of the OPERA experiment is presented. Assuming that the usual value of c should be interpreted as the velocity of light in dark matter, we call the "true" velocity of light in vacuum, $c_t$. Then the…

高能物理 - 唯象学 · 物理学 2013-05-30 Joseph Schechter , M. Naeem Shahid

According to the cosmological principle, the Universe should appear isotropic, without any preferred directions, to an observer whom we may consider to be fixed in the co-moving co-ordinate system of the expanding Universe. Such an observer…

宇宙学与河外天体物理 · 物理学 2013-06-11 Ashok K. Singal

Standard cosmology has long been plagued by a number of persistent problems. The origin of the apparent acceleration of the cosmic expansion remains enigmatic. The cosmological constant has been reintroduced as a free parameter with a value…

综合物理 · 物理学 2023-02-28 Jan O. Stenflo