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Representing Massive Gravitons, as a Way to Quantify Early Universe Magnetic Field Contributions to Space-Time, Created by non Linear Electrodynamics

机译:代表巨大的格格,作为量化早期宇宙磁场对时空的贡献的一种方式,由非线性电动力产生

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We review a relationship between cosmological vacuum energy and massive gravitons as given by Garattini and also the nonlinear electrodynamics of Camara et.al (2004) for a non singular universe and NLED. In evaluating the Garattini result, we find that having the scale factor close to zero due to a given magnetic field value in, an early universe magnetic field affects how we would interpret Garattini's linkage of the 'cosmological constant' value and non zero graviton mass. We close as to how these initial conditions affect the issue of an early universe initial pressure and its experimental similarities and differences with results by Corda and Questa as to negative pressure at the surface of a star. Note, that in theDupays et.al. article, the star in question is rapidly spinning, which is not. assumed in the Camara et.al article, for an early universe. Also, Corda and Questa do not assume a spinning star. We conclude with a comparison between the Lagrangian Dupays and other authors bring up for non linear electrodynamics which is for rapidly spinning neutron stars, and a linkage between the Goldstone theorem and NLED. Our conclusion is for generalizing results seen in the Dupays neutron star Lagrangian with conditions which may confirm C. A. Escobar and L. F. Urrutia's work on the Goldstone theorem and non linear electrodynamics, for some future projects we have in mind. If the universe does not spin, then we will stick with the density analogy given by adapting density as proportional to one over the fourth power of the minimum value of the scale factor as computed by adaptation of the Camara et.al.(2004) theory for non spinning universes. What may happen is that the Camara (2004) density and Quintessential density are both simultaneously satisfied, which would put additional restrictions on the magnetic field, which is one of our considerations, regardless if a universe spins, akin to spinning neutron stars. The spinning universe though may allow for easier reconciliation of the 'Goldstone' behavior of gravity and NLED though.
机译:我们审查了Garattini给出的宇宙学真空能量和大规模格子之间的关系,也是非单数宇宙的Camara et.al(2004)的非线性电动力学。在评估Garattini结果时,我们发现由于给定的磁场值而具有较好的比例因子,早期宇宙磁场会影响我们将如何解释Garattini的“宇宙学常数”值和非零墓穴的联系。我们接近这些初始条件如何影响早期宇宙初始压力的问题及其实验相似性,以及Corda和Questa的结果,以及明星表面的负压。注意,在Thedupays et.al中。文章,有问题的恒星正在迅速旋转,这不是。假设在Camara et.al文章中,为早期宇宙。此外,Corda和Questa不承担旋转星。我们在拉格朗日DPOPAY和其他作者之间进行了比较,即将出现非线性电动电动,这是用于快速旋转中子恒星的旋转中子恒星,以及金石定理与NLED之间的连锁。我们的结论是在Dupays中子星拉格朗安中看到的概括结果,条件可以确认C. A. Escobar和L.F.Frurutia对Goldstone定理和非线性电动电动的工作,我们考虑的一些未来的项目。如果宇宙没有旋转,那么我们将通过调整密度,以通过适应Camara et.al的适应计算的比例因子的最小值的第四个电量成比例的密度类比。(2004)理论对于非旋转宇宙。可能发生的是Camara(2004)密度和典型密度都同时满足,这将对磁场提出额外的限制,这是我们考虑的额外限制,无论宇宙旋转,类似于纺纱中子恒星。旋转宇宙可能允许更容易地对和解重力的“金石”行为。

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