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相关论文: Anthropic Estimates for Many Parameters of Physics…

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We present a lattice calculation of the mass difference between neutron and proton, for which we find $ M_n - M_p = 1.73(69) \, \text{MeV}$. This is obtained at 1st order in the $QED$ coupling $\alpha_{EM}$ and in the mass difference…

高能物理 - 格点 · 物理学 2022-07-12 Simone Romiti

Probabilistic models (developped by workers such as Boltzmann, on foundations due to pioneers such as Bayes) were commonly regarded merely as approximations to a deterministic reality before the roles were reversed by the quantum revolution…

量子物理 · 物理学 2007-05-23 Brandon Carter

Extremely weak new forces could lead to apparent violations of the Equivalence Principle. The MICROSCOPE experiment implies that the relative strength of a new long-range force, compared with gravity, is constrained to $|\bar\alpha_g|<3.2\…

高能物理 - 唯象学 · 物理学 2019-04-05 Pierre Fayet

The ratio between the proton and electron masses was shown to be close to the ratio between the shortest lifetimes of particles, decaying by the electromagnetic and strong interactions. The inherent property of each fundamental interaction…

综合物理 · 物理学 2015-12-31 Dimitar Valev

Selection effects in cosmology are often invoked to "explain" why some of the fundamental constant of Nature, and in particular the cosmological constant, take on the value they do in our Universe. We briefly review this probabilistic…

天体物理学 · 物理学 2009-11-11 Roberto Trotta , Glenn D. Starkman

We argue that the familiar gauge hierarchy between the fundamental Planck scale M_{Pl} and the electroweak scale M_{W}, can be naturally explained in higher dimensional theories with relatively large radii (R_c > 1/M_{Pl}) extra dimensions.…

高能物理 - 理论 · 物理学 2009-10-31 Masud Chaichian , Archil B. Kobakhidze

The Born approximation, based on $\bar\alpha \equiv\alpha (m_Z)$ instead of $\alpha$, reproduces all electroweak precision measurements within their $(1\sigma)$ accuracy. The low upper limits for the genuinely electroweak corrections…

高能物理 - 唯象学 · 物理学 2015-06-25 V. A. Novikov , L. B. Okun , M. I. Vysotsky

In the paper the Planck, Yukawa and Bohr forces were defined and calculated. It was shown that the Planck force mediates the universe acceleration. The Yukawa and Bohr forces describe the gradients of attractive strong and Coulomb forces.…

天体物理学 · 物理学 2007-05-23 Miroslaw Kozlowski , Janina Marciak-Kozlowska

The matching of our epoch of existence with the approximate equality of dark energy and dark matter energy densities is an apparent further fine-tuning, beyond the already troubling 120 orders of magnitude that separate dark energy from the…

宇宙学与河外天体物理 · 物理学 2013-04-17 Navin Sivanandam

We investigate possible systematic errors in the recent measurement of the matter power spectrum from the Lyman-alpha forest by Croft et al. (2001). We find that for a large set of prior cosmological models the Croft et al. result holds…

天体物理学 · 物理学 2009-11-07 Nickolay Y. Gnedin , Andrew J. S. Hamilton

A parameter method is introduced in order to estimate the relationship among the various variables of a system in equilibrium, where the potential energy functions are incompletely known or the quantum mechanical calculations very…

综合物理 · 物理学 2011-05-12 Walton R. Gutierrez

By either performing a Taylor expansion or making a polynomial approximation, the Bethe equation for charged particle stopping power in matter can be integrated analytically to obtain the range of charged particles in the continuous…

其他凝聚态物理 · 物理学 2009-02-11 Damian C. Swift , James M. McNaney

For a flat universe presently dominated by smooth energy, either cosmological constant (LCDM) or quintessence (QCDM), we calculate the asymptotic collapsed mass fraction as function of the present ratio of smooth energy to matter energy…

天体物理学 · 物理学 2009-10-31 Sidney Bludman , Matts Roos

We produce the simple formula for the radius R of a cold body of mass M, (4 pi rho/3)^{1/3} R = I.M^{1/3} / [1+ (M/Mp)^{2/3}], where I is one for white dwarfs with non-relativistic electrons, but depends on the ratio of the total mass to…

天体物理学 · 物理学 2007-05-23 D. Lynden-Bell , J. P. O'Dwyer

In a previous paper, I demonstrated the accuracy of simple, precessing, power ellipse (p-ellipse) approximations to orbits of low-to-moderate eccentricity in power-law potentials. Here I explore several extensions of these approximations to…

星系天体物理 · 物理学 2015-06-23 Curtis Struck

We point out that the long-standing strong CP problem may be resolved by an anthropic argument. The key ideas are: (i) to allow explicit breaking(s) of the Peccei-Quinn symmetry which reduces the strong CP problem to the cosmological…

高能物理 - 唯象学 · 物理学 2009-05-30 Fuminobu Takahashi

Using modified Richardson-Lucy algorithm we reconstruct the primordial power spectrum (PPS) from Planck Cosmic Microwave Background (CMB) temperature anisotropy data. In our analysis we use different combinations of angular power spectra…

宇宙学与河外天体物理 · 物理学 2014-12-19 Dhiraj Kumar Hazra , Arman Shafieloo , Tarun Souradeep

Probably not, because there are lots of manifestly unanthropic ways of producing entropy. We demonstrate that the Causal Entropic Principle (CEP), as a replacement for the anthropic principle to explain the properties of the observed…

高能物理 - 理论 · 物理学 2008-12-05 Irit Maor , Thomas W. Kephart , Lawrence M. Krauss , Y. Jack Ng , Glenn D. Starkman

Beginning from the standard Arnowitt-Deser-Misner (ADM) formulation of general relativity we construct a tentative model of quantum gravity from the point of view of an observer with constant proper acceleration, just outside of a horizon…

广义相对论与量子宇宙学 · 物理学 2024-05-30 Jarmo Mäkelä

The Dirac equation for an electron in two spatial dimensions in the Coulomb and homogeneous magnetic fields is discussed. For weak magnetic fields, the approximate energy values are obtained by semiclassical method. In the case with strong…

量子物理 · 物理学 2009-11-06 Choon-Lin Ho , V. R. Khalilov