The Newtonian limit at intermediate energies

被引：137

作者：

Cembranos, JAR ^{[1
]}

机构：

[1] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA

来源：

PHYSICAL REVIEW D | 2006年 / 73卷 / 06期

基金：

美国国家科学基金会;

关键词：

D O I：

10.1103/PhysRevD.73.064029

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We study the metric solutions for the gravitational equations in Modified Gravity Models (MGMs). In models with negative powers of the scalar curvature, we show that the Newtonian Limit (NL) is well defined as a limit at intermediate energies, in contrast with the usual low energy interpretation. Indeed, we show that the gravitational interaction is modified at low densities or low curvatures.

引用

页数：5

共 60 条

[1] Limits on the brane fluctuations mass and on the brane tension scale from electron-positron colliders [J].

Alcaraz, J ;

Cembranos, JAR ;

Dobado, A ;

Maroto, AL .

PHYSICAL REVIEW D, 2003, 67 (07)

[2] Dark energy dominance and cosmic acceleration in first-order formalism [J].

Allemandi, G ;

Borowiec, A ;

Francaviglia, M ;

Odintsov, SD .

PHYSICAL REVIEW D, 2005, 72 (06)

[3] Post-newtonian parameters from alternative theories of gravity [J].

Allemandi, G ;

Francaviglia, M ;

Ruggiero, ML ;

Tartaglia, A .

GENERAL RELATIVITY AND GRAVITATION, 2005, 37 (11) :1891-1904

[4] Accelerated cosmological models in first-order nonlinear gravity [J].

Allemandi, G ;

Borowiec, A ;

Francaviglia, M .

PHYSICAL REVIEW D, 2004, 70 (04)

[5] Reconciling dark energy models with f(R) theories -: art. no. 043503 [J].

Capozziello, S ;

Cardone, VF ;

Troisi, A .

PHYSICAL REVIEW D, 2005, 71 (04) :043503-1

[6] Can higher order curvature theories explain rotation curves of galaxies? [J].

Capozziello, S ;

Cardone, VF ;

Carloni, S ;

Troisi, A .

PHYSICS LETTERS A, 2004, 326 (5-6) :292-296

[7] Curvature quintessence matched with observational data [J].

Capozziello, S ;

Cardone, VF ;

Carloni, S ;

Troisi, A .

INTERNATIONAL JOURNAL OF MODERN PHYSICS D, 2003, 12 (10) :1969-1982

[8]

CAPOZZIELLO S, ASTROPH0303041

[9] Cosmological dynamics of Rn gravity [J].

Carloni, S ;

Dunsby, PKS ;

Capozziello, S ;

Troisi, A .

CLASSICAL AND QUANTUM GRAVITY, 2005, 22 (22) :4839-4868

[10] Is cosmic speed-up due to new gravitational physics? [J].

Carroll, SM ;

Duvvuri, V ;

Trodden, M ;

Turner, MS .

PHYSICAL REVIEW D, 2004, 70 (04)

← 1 2 3 4 5 6 →