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Examination of equilibrium radiation in plasma media shows that the spectral the energy distribution of such radiation is different from the Planck equilibrium radiation. Using the previously obtained general relations for the spectral…

统计力学 · 物理学 2019-09-04 Alexander M. Ignatov , Sergey A. Trigger

We present two possible physical explanations of the nonextensive parameter in a self-gravitating system. One is related to the detailed balance in such system. With the detailed balance, the statistical balance of molecular energy is…

统计力学 · 物理学 2015-08-10 Yahui Zheng , Jiulin Du

We argue that the Maxwellian approximation can essentially underestimate the rates of some nuclear reactions in hot plasma under conditions very close to thermal equilibrium. This phenomenon is demonstrated explicitly on the example of…

等离子体物理 · 物理学 2009-11-13 Makoto Nakamura , Victor T. Voronchev , Yasuyuki Nakao

The current standard solar models can be improved by substituting the relativistic equilibrium velocity distribution for the Maxwellian velocity distribution. The relativistic equilibrium velocity distribution is close- fitting to the…

统计力学 · 物理学 2007-05-23 Jian-Miin Liu

The equilibrium of dense plasma in a self-gravitation is considered. The obtained results radically distinguish from the point of view which is commonly accepted in the astrophysical society. It is important that all these results were…

天体物理学 · 物理学 2007-05-23 B. V. Vasiliev

Nuclear reactions in stars occur between nuclei in the high-energy tail of the energy distribution and are sensitive to possible deviations from the standard equilibrium thermal-energy distribution. We are able to derive strong constraints…

天体物理学 · 物理学 2008-11-26 S. Degl'Innocenti , G. Fiorentini , M. Lissia , P. Quarati , B. Ricci

We present an overview of possible imprints of non-extensitivity in particle and nucler physics. Special emphasis is put on the intrinsic fluctuations present in the system under consideration as the possible source of nonextensivity. The…

高能物理 - 唯象学 · 物理学 2009-04-15 G. Wilk , Z. Wlodarczyk

This article illustrates how very small deviations from the Maxwellian exponential tail, while leaving unchanged bulk quantities, can yield dramatic effects on fusion reaction rates and discuss several mechanisms that can cause such…

天体物理学 · 物理学 2009-11-13 Marcello Lissia , Piero Quarati

In a solar flare, a large fraction of the magnetic energy released is converted rapidly to the kinetic energy of non-thermal particles and bulk plasma motion. This will likely result in non-equilibrium particle distributions and turbulent…

太阳与恒星天体物理 · 物理学 2017-02-15 Natasha L. S. Jeffrey , Lyndsay Fletcher , Nicolas Labrosse

This study concerns a situation when measurements of the nonresonant cross-section of nuclear reactions appear highly dependent on the environment in which the particles interact. An appealing example discussed in the paper is the…

等离子体物理 · 物理学 2015-05-30 N. J. Fisch , M. G. Gladush , Yu. V. Petrushevich , Piero Quarati , A. N. Starostin

The problem of determining the effects of the surrounding plasma on nuclear reaction rates in stars is formulated ab initio, using the techniques of quantum statistical mechanics. We derive a result that expresses the complete effects of…

天体物理学 · 物理学 2008-11-26 Lowell S. Brown , R. F. Sawyer

We compute the hard photon production rate of a chemically non-equilibrated quark-gluon plasma. We assume that the plasma is already thermally equilibrated, i.~e. describable by a temperature, but with a phase-space distribution that…

高能物理 - 唯象学 · 物理学 2008-11-26 Christoph T. Traxler , Markus H. Thoma

In the hot, dense plasma of solar and stellar interiors, Coulomb potentials are screened, resulting in increased nuclear reaction rates. Although Salpeter's approximation for static screening is widely accepted and used in stellar modeling,…

太阳与恒星天体物理 · 物理学 2011-02-11 Dan Mao , Katie Mussack , Werner Däppen

The relativistic corrections to the Maxwellian velocity distribution are needed for standard solar models. Relativistic equilibrium velocity distribution, if adopted in standard solar models, will lower solar neutrino fluxes and change…

综合物理 · 物理学 2007-05-23 Jian-Miin Liu

The equation of state of symmetric nuclear matter is addressed starting both from a realistic interaction derived from nucleon-nucleon scattering processes and from a low-momentum effective potential. The approach is based on finite…

核理论 · 物理学 2008-12-18 V. Soma

Negative ions have been detected in abundance in recent years by spacecraft across the solar system. These detections were, however, made by instruments not designed for this purpose and, as such, significant uncertainties remain regarding…

空间物理 · 物理学 2021-06-17 Ravindra T. Desai , Zeqi Zhang , Xinni Wu , Charles Lue

A specific linear combination of the total solar neutrino fluxes must equal the measured solar photon luminosity if nuclear fusion reactions among light elements are responsible for solar energy generation. This luminosity constraint,…

高能物理 - 唯象学 · 物理学 2009-11-07 John N. Bahcall

The fluctuation-dissipation theorem is used to evaluate the screening factor of nuclear reactions due to the electromagnetic fluctuations in a plasma. We show that the commonly used Saltpeter factor is obtained if only fluctuations near the…

天体物理学 · 物理学 2007-05-23 Merav Opher , Reuven Opher

The instability of current-driven ion-acoustic waves in the collisionless magnetic-field-free space plasma is investigated by using a nonextensive approach. The ions and the electrons are thought of in the power-law distributions that can…

等离子体物理 · 物理学 2015-08-10 Zhipeng Liu , Liyan Liu , Jiulin Du

Non-Maxwellian distributions are commonly observed across a wide range of systems and scales. While direct observations provide the strongest evidence for these distributions, they also manifest indirectly through their influence on…

统计力学 · 物理学 2024-12-17 Kamel Ourabah