Quintessence and supergravity

被引:376
作者
Brax, P [1 ]
Martin, J
机构
[1] CEA Saclay, Serv Phys Theor, F-91191 Gif Sur Yvette, France
[2] Observ Paris Meudon, DARC, UMR 8629, F-92195 Meudon, France
关键词
D O I
10.1016/S0370-2693(99)01209-5
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In the context of quintessence, the concept of tracking solutions allows to address the fine-tuning and coincidence problems. When the field is on tracks today, one has Q = m(P1) demonstrating that, generically, any realistic model of quintessence must be based on supergravity. We construct the most simple model for which the scalar potential is positive. The scalar potential deduced from the supergravity model has the form V(Q) = Lambda(4 + alpha)/Q(alpha)e(mu/2Q2). We show that despite the appearance of positive powers of the field, the coincidence problem is still solved. If alpha greater than or equal to 11, the fine-tuning problem can be overcome. Moreover, due to the presence of the exponential term, the value of the equation of state, omega(Q), is pushed towards the value -1 in contrast to the usual case for which it is difficult to go beyond omega(Q) approximate to -0.7. For Omega(m) approximate to 0.3, the model presented here predicts omega(Q) approximate to -0.82. Finally, we establish the Omega(m) - omega(Q) relation for this model. (C) 1999 Published by Elsevier Science B.V. All rights reserved.
引用
收藏
页码:40 / 45
页数:6
相关论文
共 22 条
  • [11] DUALITY-ANOMALY CANCELLATION, MINIMAL STRING UNIFICATION AND THE EFFECTIVE LOW-ENERGY LAGRANGIAN OF 4D STRINGS
    IBANEZ, LE
    LUST, D
    [J]. NUCLEAR PHYSICS B, 1992, 382 (02) : 305 - 361
  • [12] Anomalous U(1)'s in Type I and Type IIB D = 4, N = 1 string vacua
    Ibáñez, LE
    Rabadán, R
    Uranga, AM
    [J]. NUCLEAR PHYSICS B, 1999, 542 (1-2) : 112 - 138
  • [13] THE COSMOLOGICAL CONSTANT IS BACK
    KRAUSS, LM
    TURNER, MS
    [J]. GENERAL RELATIVITY AND GRAVITATION, 1995, 27 (11) : 1137 - 1144
  • [14] MASIERO A, HEPPH9905346
  • [15] PERLMUTTER S, ASTROPH9901052
  • [16] PERROTTA F, ASTROPH9906066
  • [17] COSMOLOGICAL CONSEQUENCES OF A ROLLING HOMOGENEOUS SCALAR FIELD
    RATRA, B
    PEEBLES, PJE
    [J]. PHYSICAL REVIEW D, 1988, 37 (12): : 3406 - 3427
  • [18] Observational evidence from supernovae for an accelerating universe and a cosmological constant
    Riess, AG
    Filippenko, AV
    Challis, P
    Clocchiatti, A
    Diercks, A
    Garnavich, PM
    Gilliland, RL
    Hogan, CJ
    Jha, S
    Kirshner, RP
    Leibundgut, B
    Phillips, MM
    Reiss, D
    Schmidt, BP
    Schommer, RA
    Smith, RC
    Spyromilio, J
    Stubbs, C
    Suntzeff, NB
    Tonry, J
    [J]. ASTRONOMICAL JOURNAL, 1998, 116 (03) : 1009 - 1038
  • [19] ROSATI F, HEPPH9908518
  • [20] STEINHARDT PJ, ASTROPH9812313