Dark Energy and Baryon Isocurvature Perturbation

  • Quintessence is a possible candidate for dark energy. In this paper we study the possibility of Quintessence interacting with the ordinary matter and its implications in baryogenesis. With a specific coupling of the Quintessence to the baryon fields, we will show that the baryon number asymmetry of the universe can be explained naturally. We will also in this paper study the isocur-vature perturbation of the baryon number in our model.
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  • [1] Bennett C L et al. astro–ph/0302207; Spergel D Net al. astro–ph/0302209 2 For a review, see Weinberg S. Rev. Mod. Phys., 1989,61:1–233 Ratra B, Peebles P J E. Phys. Rev., 1988,D37:3406–3427; Wetterich C. Nucl. Phys., 1988, B302:302–306;Frieman J A, Hill C T, Stebbins A et al. Phys. Rev. Lett., 1995, 75:2077–20804 Uzan J P. Phys. Rev., 1999, D59: 123510(1–10) ;Chiba T. Phys. Rev., 1999, D60:083508 (1–14) ; CHEN X, Kamionkouski M. Phys. Rev., 1999,D60: 104036(1–11) ;Perrotta F, Baccigalupi C, Matarrese S. Phys. Rev., 2000, D61:023507(1–12) 5 Peccei R D. hep–ph/00090306 Kolda C, Lyth D H. Phys. Lett., 1999, B458:197–201 7 Carroll S M. Phys. Rev. Lett., 1998,81:3067–3070 8 LI Ming–Zhe, WANG Xiu–Lian, FENG Bo et al. Phys. Rev., 2001, D65:103511 (1–5)9 Trodden Mark. hep–ph/0302151; De Felice Antonio, Nasri Salah, Trodden Mark. Phys. Rev., 2003, D67:043509(1–9)10 Brandenberger Robert H, Yamaguchi Masahide. hep–ph/0301270; Chiba T et al. hep–ph/0304102 ; Yamaguchi Masahide. hep–ph/0211163 ; LI Ming–Zhe, ZHANG Xin–Min. hep–ph/0209093 11 Kolb, Turner E W. The Early Universe, 1990. 47–86 12 Steinhardt P J, WANG L, Zlatev I. Phys. Rev., 1999,D59:123504 (1–13)13 Brax P, Martin J, Riazuelo A. Phys. Rev., 2000, D62:103505(1–11)14 Abramo L R, Finelli F. Phys. Rev., 2001, D64:083513(1–10)15 Kawasaki M, Moroi T, Takahashi T. astro–ph/0108081 16 Turner M S, Cohen A, Kaplan D. Phys. Lett., 1989, B216:20–30
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WANG Xiu-Lian and ZHANG Xin-Min. Dark Energy and Baryon Isocurvature Perturbation[J]. Chinese Physics C, 2003, 27(10): 874-878.
WANG Xiu-Lian and ZHANG Xin-Min. Dark Energy and Baryon Isocurvature Perturbation[J]. Chinese Physics C, 2003, 27(10): 874-878. shu
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Received: 2003-04-11
Revised: 1900-01-01
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Dark Energy and Baryon Isocurvature Perturbation

    Corresponding author: WANG Xiu-Lian,
  • Institute of High Energy Physics,CAS,Beijing 100039,China

Abstract: Quintessence is a possible candidate for dark energy. In this paper we study the possibility of Quintessence interacting with the ordinary matter and its implications in baryogenesis. With a specific coupling of the Quintessence to the baryon fields, we will show that the baryon number asymmetry of the universe can be explained naturally. We will also in this paper study the isocur-vature perturbation of the baryon number in our model.

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