2007
DOI: 10.1016/j.astropartphys.2006.10.003
|View full text |Cite
|
Sign up to set email alerts
|

Reissner–Nordström expansion

Help me understand this report
View preprint versions

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

0
24
0

Year Published

2008
2008
2011
2011

Publication Types

Select...
2
1

Relationship

2
1

Authors

Journals

citations
Cited by 3 publications
(24 citation statements)
references
References 19 publications
0
24
0
Order By: Relevance
“…Under minute density fluctuation in the volume density of one type of charges at some point, the domain of all other like charges within radius r − are trapped gravitationally into a cluster. We will call this domain a daemon (for dark electric matter objects, as introduced by [9], and in line with our previous work [5,6] on Reissner-Nordström expansion). There will be no charges of this type between r − and r + , while charges of this type on the outside of r + would be strongly repelled.…”
Section: U(r)mentioning
confidence: 96%
See 4 more Smart Citations
“…Under minute density fluctuation in the volume density of one type of charges at some point, the domain of all other like charges within radius r − are trapped gravitationally into a cluster. We will call this domain a daemon (for dark electric matter objects, as introduced by [9], and in line with our previous work [5,6] on Reissner-Nordström expansion). There will be no charges of this type between r − and r + , while charges of this type on the outside of r + would be strongly repelled.…”
Section: U(r)mentioning
confidence: 96%
“…However, in view of the parameters involved, q/m 1, thus A 1/4, and such situation cannot be achieved. To address the issue of bound states for equation (5) for the case A > 1/4, we will follow the steps of [10]. We introduce k 2 = √ −2mE/h.…”
Section: U(r)mentioning
confidence: 99%
See 3 more Smart Citations