Turning a Newtonian analogy for FLRW cosmology into a relativistic problem

2020 ◽  
Vol 102 (4) ◽  
Author(s):  
Valerio Faraoni ◽  
Farah Atieh
2020 ◽  
Vol 80 (11) ◽  
Author(s):  
Metin Gürses ◽  
Yaghoub Heydarzade

AbstractWe prove that for the Friedmann–Lemaitre–Robertson–Walker metric, the field equations of any generic gravity theory in arbitrary dimensions are of the perfect fluid type. The cases of general Lovelock and $${\mathcal {F}}(R, {\mathcal {G}})$$ F ( R , G ) theories are given as examples.


ChemInform ◽  
2003 ◽  
Vol 34 (22) ◽  
Author(s):  
Michael Filatov ◽  
Dieter Cremer
Keyword(s):  

1980 ◽  
Vol 56 (3) ◽  
pp. 263-288 ◽  
Author(s):  
D. Dominici ◽  
J. Gomis ◽  
G. Longhi
Keyword(s):  

2017 ◽  
Vol 376 ◽  
pp. 76-88 ◽  
Author(s):  
Jerónimo Cortez ◽  
Beatriz Elizaga Navascués ◽  
Mercedes Martín-Benito ◽  
Guillermo A. Mena Marugán ◽  
José M. Velhinho
Keyword(s):  

2007 ◽  
Vol 22 (14n15) ◽  
pp. 2609-2618 ◽  
Author(s):  
ANTONIO S. DE CASTRO

The intrinsically relativistic problem of spinless particles subject to a general mixing of vector and scalar kink-like potentials (~ tanh γx) is investigated. The problem is mapped into the exactly solvable Sturm–Liouville problem with the Rosen–Morse potential and exact bounded solutions for particles and antiparticles are found. The behavior of the spectrum is discussed in some detail. An apparent paradox concerning the uncertainty principle is solved by recurring to the concept of effective Compton wavelength.


2017 ◽  
Vol 95 (12) ◽  
pp. 1215-1218 ◽  
Author(s):  
Amir F. Bahrehbakhsh

We investigate the Friedmann–Lemaître–Robertson–Walker (FLRW) type cosmology of the induced dark energy model and illustrate that the extra terms emerging from the fifth dimension can play the role of dark energy. The model predicts the expansion with deceleration at early time and acceleration in late time for an open universe.


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