Nonlinear evolution of baryon acoustic oscillations

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 77, Issue 2, 2008, Pages

  Crocce, Martín ^a,b   Scoccimarro, Román ^a  

^a NEW YORK UNIVERSITY   (United States)

^b INSTITUT DE CIÈNCIES DE L ESPAI CSIC IEEC   (Spain)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 38849119739     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.77.023533     Document Type: Article

References (77)

1. D.J. Eisenstein, W. Hu, and M. Tegmark, Astrophys. J. 504, L57 (1998); ASJOAB 0004-637X 10.1086/311582
2. A. Cooray, W. Hu, D. Huterer, and M. Joffre, Astrophys. J. 557, L7 (2001); ASJOAB 0004-637X 10.1086/323323
3. W. Hu and Z. Haiman, Phys. Rev. D 68, 063004 (2003); PRVDAQ 0556-2821 10.1103/PhysRevD.68.063004
4. C. Blake and K. Glazebrook, Astrophys. J. 594, 665 (2003); ASJOAB 0004-637X 10.1086/376983
5. H.-J. Seo and D.J. Eisenstein, Astrophys. J. 598, 720 (2003); ASJOAB 0004-637X 10.1086/379122
6. C. Blake and K. Glazebrook, Astrophys. J. 631, 1 (2005); ASJOAB 0004-637X 10.1086/432497
7. H. Zhan and L. Knox, Astrophys. J. 644, 663 (2006). ASJOAB 0004-637X 10.1086/503622
8. P.J.E. Peebles and J.T. Yu, Astrophys. J. 162, 815 (1970); ASJOAB 0004-637X 10.1086/150713
9. R. Sunyaev and Ya.-B. Zel'dovich, Astrophys. J. Suppl. Ser. 7, 3 (1970). APJSA2 0067-0049
10. D.J. Eisenstein, Astrophys. J. 633, 560 (2005). ASJOAB 0004-637X 10.1086/466512
11. S. Cole, Mon. Not. R. Astron. Soc. 362, 505 (2005); MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09318.x
12. M. Tegmark, Phys. Rev. D 74, 123507 (2006); PRVDAQ 0556-2821 10.1103/PhysRevD.74.123507
13. G. Hütsi, Astron. Astrophys. 449, 891 (2006); AAEJAF 0004-6361 10.1051/0004-6361:20053939
14. W. Percival, Astrophys. J. 657, 51 (2007); ASJOAB 0004-637X 10.1086/510772
15. N. Padmanabhan, Mon. Not. R. Astron. Soc. MNRAA4 0035-8711 378, 852 (2007). 10.1111/j.1365-2966.2007.11593.x
16. R. Angulo, C.M. Baugh, C.S. Frenk, and C.G. Lacey, arXiv:astro-ph/ 0702543.
17. A. Meiksin, M. White, and J.A. Peacock, Mon. Not. R. Astron. Soc. 304, 851 (1999); MNRAA4 0035-8711 10.1046/j.1365-8711.1999.02369.x
18. H.-J. Seo and D.J. Eisenstein, Astrophys. J. 598, 720 (2003); ASJOAB 0004-637X 10.1086/379122
19. M. White, Astropart. Phys. 24, 334 (2005); APHYEE 0927-6505 10.1016/j.astropartphys.2005.07.007
20. V. Springel, Nature (London) NATUAS 0028-0836 435, 629 (2005). 10.1038/nature03597
21. E. Huff, A.E. Schultz, M. White, D.J. Schlegel, and M.S. Warren, Astropart. Phys. APHYEE 0927-6505 26, 351 (2007). 10.1016/j.astropartphys.2006. 07.007
22. D.J. Eisenstein, H.-J. Seo, E. Sirko, and D.N.S. Spergel, arXiv:astro-ph/0604362.
23. Z. Ma, arXiv:astro-ph/0610213.
24. A.E. Schultz and M. White, Astropart. Phys. APHYEE 0927-6505 25, 172 (2006). 10.1016/j.astropartphys.2005.11.007
25. D. Jeong and E. Komatsu, Astrophys. J. 651, 619 (2006). ASJOAB 0004-637X 10.1086/507781
26. J. Guzik, G. Bernstein, and R.E. Smith, Mon. Not. R. Astron. Soc. MNRAA4 0035-8711 375, 1329 (2007). 10.1111/j.1365-2966.2006.11385.x
27. D.J. Eisenstein, H.-J. Seo, and M. White, arXiv:astro-ph/064361.
28. R.E. Smith, R. Scoccimarro, and R.K. Sheth, Phys. Rev. D 75, 063512 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.75.063512
29. S. Matarrese and M. Pietroni, arXiv:astro-ph/0702653;
30. S. Matarrese M. Pietroni J. Cosmol. Astropart. Phys. 1475-7516 06 (2007) 026. 10.1088/1475-7516/2007/06/026
31. R.E. Smith, R. Scoccimarro, and R.K. Sheth, arXiv:astro-ph/0703620.
32. R.E. Smith, Mon. Not. R. Astron. Soc. 341, 1311 (2003). MNRAA4 0035-8711 10.1046/j.1365-8711.2003.06503.x
33. M. Crocce and R. Scoccimarro, Phys. Rev. D 73, 063519 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.063519
34. M. Crocce and R. Scoccimarro, Phys. Rev. D 73, 063520 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.73.063520
35. For other, related, recent approaches to understanding nonlinear clustering see. In particular, the description of BAO in the power spectrum is also addressed in.
36. S. Bharadwaj, Astrophys. J. 472, 1 (1996). ASJOAB 0004-637X 10.1086/178036
37. M. Crocce and R. Scoccimarro (unpublished).
38. F. Bernardeau, S. Colombi, E. Gaztañaga, and R. Scoccimarro, Phys. Rep. 367, 1 (2002). PRPLCM 0370-1573 10.1016/S0370-1573(02)00135-7
39. For ease of presentation, we ignore here that the propagator is a matrix; what we call G here is the density propagator for growing mode initial conditions described in. Also, we implicitly assume Gaussian initial conditions, from which the identification of the propagator with the cross correlation follows. The propagator G has two types of contributions: growing mode and decaying mode. In loop diagrams the latter also become important, as after nonlinear interactions perturbations do not remain in the growing mode. See also the Appendix.
40. R. Scoccimarro, Mon. Not. R. Astron. Soc. 299, 1097 (1998). MNRAA4 0035-8711 10.1046/j.1365-8711.1998.01845.x
41. M. Crocce, S. Pueblas, and R. Scoccimarro, Mon. Not. R. Astron. Soc. 373, 369 (2006). MNRAA4 0035-8711 10.1111/j.1365-2966.2006.11040.x
42. V. Springel, Mon. Not. R. Astron. Soc. 364, 1105 (2005). MNRAA4 0035-8711 10.1111/j.1365-2966.2005.09655.x
43. F. Bernardeau, M. Crocce, and R. Scoccimarro (unpublished).
44. N. Makino, M. Sasaki, and Y. Suto, Phys. Rev. D 46, 585 (1992); PRVDAQ 0556-2821 10.1103/PhysRevD.46.585
45. B. Jain and E. Bertschinger, Astrophys. J. 431, 495 (1994); ASJOAB 0004-637X 10.1086/174502
46. C.M. Baugh and G. Efstathiou, Mon. Not. R. Astron. Soc. 270, 183 (1994); MNRAA4 0035-8711
47. E.L. Łokas, R. Juszkiewicz, F.R. Bouchet, and E. Hivon, Astrophys. J. 467, 1 (1996); ASJOAB 0004-637X 10.1086/177580
48. R. Scoccimarro and J.A. Frieman, Astrophys. J. 473, 620 (1996). ASJOAB 0004-637X 10.1086/178177
49. J.M. Bardeen, J.R. Bond, N. Kaiser, and A.S. Szalay, Astrophys. J. 304, 15 (1986). ASJOAB 0004-637X 10.1086/164143
50. K. Heitmann, P.M. Ricker, M.S. Warren, and S. Habib, Astrophys. J. Suppl. Ser. 160, 28 (2005). APJSA2 0067-0049 10.1086/432646
51. A. Cooray and R.K. Sheth, Phys. Rep. 372, 1 (2002). PRPLCM 0370-1573 10.1016/S0370-1573(02)00276-4
52. X. Yang, H.J. Mo, and F.C. van den Bosch, Mon. Not. R. Astron. Soc. 339, 1057 (2003). MNRAA4 0035-8711 10.1046/j.1365-8711.2003.06254.x
53. Z. Zheng, Astrophys. J. 610, 61 (2004). ASJOAB 0004-637X 10.1086/421542
54. J.L. Tinker, D.H. Weinberg, Z. Zheng, and I. Zehavi, Astrophys. J. 631, 41 (2005). ASJOAB 0004-637X 10.1086/432084
55. P. McDonald, Phys. Rev. D 74, 103512 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.103512
56. R.K. Sheth and G. Tormen, Mon. Not. R. Astron. Soc. 308, 119 (1999). MNRAA4 0035-8711 10.1046/j.1365-8711.1999.02692.x
57. Ya.B. Zel'dovich, Adv. Astron. Astrophys. 3, 241 (1965). AAYAAK 0065-2180
58. P.J.E. Peebles, The Large-Scale Structure of the Universe (Princeton University Press, Princeton, NJ, 1980), Sec. II-28.
59. M.H. Goroff, B. Grinstein, S.-J. Rey, and M.B. Wise, Astrophys. J. 311, 6 (1986). ASJOAB 0004-637X 10.1086/164749
60. T. Nishimichi, H. Ohmuro, M. Nakamichi, A. Taruya, K. Yahata, A. Shirata, S. Saito, H. Nomura, K. Yamamoto, and Y. Suto, arXiv:astro-ph/07051589.
61. W.J. Percival, S. Cole, D.J. Eisenstein, R.C. Nichol, J.A. Peacock, A.C. Pope, and A.S. Szalay, arXiv:astro-ph/07053323.
62. C. Blake and K. Glazebrook, Astrophys. J. 594, 665 (2003). ASJOAB 0004-637X 10.1086/376983
63. R. Scoccimarro and J.A. Frieman, Astrophys. J. 473, 620 (1996). ASJOAB 0004-637X 10.1086/178177
64. For another way of seeing how shifts arise naturally, see. The v• terms in the equations of motion we highlight here lead to the flow of characteristics and the erasure of the acoustic peak in the divergence of the pairwise infall velocities Θ discussed in.
65. For a similar effect in the covariance matrix of the power spectrum, see.
66. A.F. Heavens, S. Matarrese, and L. Verde, Mon. Not. R. Astron. Soc. 301, 797 (1998). MNRAA4 0035-8711 10.1046/j.1365-8711.1998.02052.x
67. E. Hivon, F.R. Bouchet, S. Colombi, and R. Juszkiewicz, Astron. Astrophys. 298, 643 (1995); AAEJAF 0004-6361
68. L. Verde, A.F. Heavens, S. Matarrese, and L. Moscardini, Mon. Not. R. Astron. Soc. 300, 747 (1998); MNRAA4 0035-8711 10.1046/j.1365-8711.1998.01937.x
69. R. Scoccimarro, H.M.P. Couchman, and J.A. Frieman, Astrophys. J. 517, 531 (1999). ASJOAB 0004-637X 10.1086/307220
70. R. Scoccimarro, R.K. Sheth, L. Hui, and B. Jain, Astrophys. J. 546, 20 (2001). ASJOAB 0004-637X 10.1086/318261
71. E. Sefusatti, M. Crocce, S. Pueblas, and R. Scoccimarro, Phys. Rev. D 74, 023522 (2006). PRVDAQ 0556-2821 10.1103/PhysRevD.74.023522
72. H.A. Feldman, J.A. Frieman, J.N. Fry, and R. Scoccimarro, Phys. Rev. Lett. 86, 1434 (2001). PRLTAO 0031-9007 10.1103/PhysRevLett.86.1434
73. R. Scoccimarro, Ann. N.Y. Acad. Sci. ANYAA9 0077-8923 927, 13 (2001).
74. N. Afshordi, Phys. Rev. D 75, 021302(R) (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.75.021302
75. P. Valageas, arXiv:astro-ph/0611849.
76. P. McDonald, Phys. Rev. D 75, 043514 (2007). PRVDAQ 0556-2821 10.1103/PhysRevD.75.043514
77. M.C. Neyrinck and I. Szapudi, arXiv:0710.3586.