Energetics of the aligned pulsar magnetosphere

Martin, R.

doi:10.1007/bf00651088

Search citation statements

Order By: Relevance

Paper Sections

Select...

Introduction1

Citation Types

Supporting

Mentioning

Contrasting

Year Published

2017

Publication Types

Select...

Article1

Relationship

Self Cite0

Independent1

Authors

Journals

Cited by 1 publication

(1 citation statement)

References 11 publications

Supporting

Mentioning

Contrasting

Order By: Relevance

“…On the other hand, inflation can also be driven by a scalar field to describe the accelerated expansion of the early universe (Liddle & Lyth 2000;Bassett et al 2006;Linde 2008Linde , 2014Baumann & McAllister 2015;Chernoff & Tye 2015;Martin 2016). Recently, increasing attention has been paid to the possibility of whether a homogeneous and isotropic universe can be obtained through inflation with relatively arbitrary initial conditions (note that the initial conditions are mainly related to the initial value of the scalar field and its velocity; see Brandenberger 2017, for a short review).…”

Section: Introductionmentioning

confidence: 99%

The Dynamics of Inhomogeneous Dark Energy

Tian

Cao

Zhu

2017

ApJ

View full text Add to dashboard Cite

In this paper, by analyzing the dynamics of the inhomogeneous quintessence dark energy, we find that the gradient energy of dark energy will oscillate and gradually vanish, which indicates the gradient energy of the scalar field present in the early universe does not affect the current dynamics of the universe. Moreover, with the decaying of gradient energy, there exists a possible mutual transformation between kinetic energy and gradient energy. In the framework of interacting dark energy models, we argue that inhomogeneous dark energy may have a significant effect on the evolution of the cosmic background, the investigation of which still requires fully relativistic N -body numerical simulations in the future.

show abstract