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Volumn 2011, Issue 6, 2011, Pages

Next-to-leading resummations in cosmological perturbation theory

Author keywords

cosmological perturbation theory; cosmological simulations; dark matter simulations; power spectrum

Indexed keywords


EID: 79960020585     PISSN: None     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2011/06/015     Document Type: Article
Times cited : (44)

References (28)
  • 1
    • 33644934381 scopus 로고    scopus 로고
    • Memory of Initial Conditions in Gravitational Clustering
    • [astro-ph/0509419]
    • M. Crocce and R. Scoccimarro, 2006 Memory of Initial Conditions in Gravitational Clustering, Phys. Rev. D 73 063520 [astro-ph/0509419]
    • (2006) Phys. Rev. D , vol.73 , pp. 063520
    • Crocce, M.1    Scoccimarro, R.2
  • 2
    • 0036314605 scopus 로고    scopus 로고
    • Large-scale structure of the universe and cosmological perturbation theory
    • [astro-ph/0112551]
    • F. Bernardeau, S. Colombi, E. Gaztanaga and R. Scoccimarro, 2002 Large-scale structure of the universe and cosmological perturbation theory, Phys. Rept. 367 1 [astro-ph/0112551]
    • (2002) Phys. Rept. , vol.367 , pp. 1
    • Bernardeau, F.1    Colombi, S.2    Gaztanaga, E.3    Scoccimarro, R.4
  • 4
    • 33847061699 scopus 로고    scopus 로고
    • Dark matter clustering: A simple renormalization group approach
    • [astro-ph/0606028]
    • P. McDonald, 2007 Dark matter clustering: a simple renormalization group approach, Phys. Rev. D 75 043514 [astro-ph/0606028]
    • (2007) Phys. Rev. D , vol.75 , pp. 043514
    • McDonald, P.1
  • 5
    • 41549143542 scopus 로고    scopus 로고
    • Baryonic acoustic oscillations via the renormalization group
    • [astro-ph/0702653]
    • S. Matarrese and M. Pietroni, 2008 Baryonic acoustic oscillations via the renormalization group, Mod. Phys. Lett. A 23 25 [astro-ph/0702653]
    • (2008) Mod. Phys. Lett. A , vol.23 , pp. 25
    • Matarrese, S.1    Pietroni, M.2
  • 7
    • 38849119739 scopus 로고    scopus 로고
    • Nonlinear Evolution of Baryon Acoustic Oscillations
    • [0704.2783]
    • M. Crocce and R. Scoccimarro, 2008 Nonlinear Evolution of Baryon Acoustic Oscillations, Phys. Rev. D 77 023533 [0704.2783]
    • (2008) Phys. Rev. D , vol.77 , pp. 023533
    • Crocce, M.1    Scoccimarro, R.2
  • 8
    • 41549089575 scopus 로고    scopus 로고
    • Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
    • [0711.2521]
    • T. Matsubara, 2008 Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space, Phys. Rev. D 77 063530 [0711.2521]
    • (2008) Phys. Rev. D , vol.77 , pp. 063530
    • Matsubara, T.1
  • 9
    • 56449113876 scopus 로고    scopus 로고
    • Flowing with Time: A New Approach to Nonlinear Cosmological Perturbations
    • M. Pietroni, 2008 Flowing with Time: a New Approach to Nonlinear Cosmological Perturbations J. Cosmol. Astropart. Phys. JCAP10(2008)036 [0806.0971]
    • (2008) J. Cosmol. Astropart. Phys. JCAP , vol.10 , pp. 036
    • Pietroni, M.1
  • 10
    • 55149117504 scopus 로고    scopus 로고
    • Nonlinear perturbation theory with halo bias and redshift- space distortions via the Lagrangian picture
    • [0807.1733]
    • T. Matsubara, 2008 Nonlinear perturbation theory with halo bias and redshift- space distortions via the Lagrangian picture, Phys. Rev. D 78 083519 [0807.1733]
    • (2008) Phys. Rev. D , vol.78 , pp. 083519
    • Matsubara, T.1
  • 12
    • 73449108369 scopus 로고    scopus 로고
    • Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces
    • A. Taruya, T. Nishimichi, S. Saito and T. Hiramatsu, 2009 Non-linear Evolution of Baryon Acoustic Oscillations from Improved Perturbation Theory in Real and Redshift Spaces, Phys. Rev. D 80 123503 [0906.0507]
    • (2009) Phys. Rev. D , vol.80 , pp. 123503
    • Taruya, A.1    Nishimichi, T.2    Saito, S.3    Hiramatsu, T.4
  • 13
    • 67649400783 scopus 로고    scopus 로고
    • Chasing the non-linear evolution of matter power spectrum with numerical resummation method: Solution of closure equations
    • T. Hiramatsu and A. Taruya, 2009 Chasing the non-linear evolution of matter power spectrum with numerical resummation method: solution of closure equations, Phys. Rev. D 79 103526 [0902.3772]
    • (2009) Phys. Rev. , vol.79 , pp. 103526
    • Hiramatsu, T.1    Taruya, A.2
  • 14
    • 78650994729 scopus 로고    scopus 로고
    • Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory
    • A. Taruya, T. Nishimichi and S. Saito, 2010 Baryon Acoustic Oscillations in 2D: Modeling Redshift-space Power Spectrum from Perturbation Theory, Phys. Rev. D 82 063522 [1006.0699]
    • (2010) Phys. Rev. D , vol.82 , pp. 063522
    • Taruya, A.1    Nishimichi, T.2    Saito, S.3
  • 18
    • 77950225540 scopus 로고    scopus 로고
    • Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: The Time-RG Approach
    • N. Bartolo, J.P.B. Almeida, S. Matarrese, M. Pietroni and A. Riotto, 2010 Signatures of Primordial non-Gaussianities in the Matter Power-Spectrum and Bispectrum: the Time-RG Approach J. Cosmol. Astropart. Phys. JCAP03(2010)011 [0912.4276]
    • (2010) J. Cosmol. Astropart. Phys. , vol.2010 , pp. 011
    • Bartolo, N.1    Almeida, J.P.B.2    Matarrese, S.3    Pietroni, M.4    Riotto, A.5
  • 19
    • 33644932646 scopus 로고    scopus 로고
    • Renormalized Cosmological Perturbation Theory
    • M. Crocce and R. Scoccimarro, 2006 Renormalized Cosmological Perturbation Theory, Phys. Rev. D 73 063519 [astro-ph/0509418]
    • (2006) Phys. Rev. D , vol.73 , pp. 063519
    • Crocce, M.1    Scoccimarro, R.2
  • 20
    • 57149146310 scopus 로고    scopus 로고
    • Multi-Point Propagators in Cosmological Gravitational Instability
    • F. Bernardeau, M. Crocce and R. Scoccimarro, 2008 Multi-Point Propagators in Cosmological Gravitational Instability, Phys. Rev. D 78 103521 [0806.2334]
    • (2008) Phys. Rev. D , vol.78 , pp. 103521
    • Bernardeau, F.1    Crocce, M.2    Scoccimarro, R.3
  • 21
    • 78651069622 scopus 로고    scopus 로고
    • Multi-Point Propagators for Non-Gaussian Initial Conditions
    • F. Bernardeau, M. Crocce and E. Sefusatti, 2010 Multi-Point Propagators for Non-Gaussian Initial Conditions, Phys. Rev. D 82 083507 [1006.4656]
    • (2010) Phys. Rev. D , vol.82 , pp. 083507
    • Bernardeau, F.1    Crocce, M.2    Sefusatti, E.3
  • 22
    • 0012749240 scopus 로고
    • Formulation of the theory of turbulence in an incompressible fluid
    • H.W. Wyld Jr., 1961 Formulation of the theory of turbulence in an incompressible fluid Annals Phys. 14 143
    • (1961) Annals Phys. , vol.14 , pp. 143
    • Wyld Jr., H.W.1
  • 24
    • 69949171651 scopus 로고    scopus 로고
    • A critical look at cosmological perturbation theory techniques
    • J. Carlson, M. White and N. Padmanabhan, 2009 A critical look at cosmological perturbation theory techniques, Phys. Rev. D 80 043531 [0905.0479]
    • (2009) Phys. Rev. D , vol.80 , pp. 043531
    • Carlson, J.1    White, M.2    Padmanabhan, N.3
  • 25
    • 0034239591 scopus 로고    scopus 로고
    • Efficient Computation of CMB anisotropies in closed FRW models
    • [astro-ph/9911177]
    • A. Lewis, A. Challinor and A. Lasenby, 2000 Efficient Computation of CMB anisotropies in closed FRW models, Astrophys. J. 538 473 [astro-ph/9911177]
    • (2000) Astrophys. J. , vol.538 , pp. 473
    • Lewis, A.1    Challinor, A.2    Lasenby, A.3
  • 26
    • 12044253591 scopus 로고
    • Statistics of primordial density perturbations from discrete seed masses
    • R.J. Scherrer and E. Bertschinger, 1991 Statistics of primordial density perturbations from discrete seed masses Astrophys. J. 381 349
    • (1991) Astrophys. J. , vol.381 , pp. 349
    • Scherrer, R.J.1    Bertschinger, E.2
  • 27
    • 0036888096 scopus 로고    scopus 로고
    • Halo models of large scale structure
    • [astro-ph/0206508]
    • A. Cooray and R.K. Sheth, 2002 Halo models of large scale structure, Phys. Rept. 372 1 [astro-ph/0206508]
    • (2002) Phys. Rept. , vol.372 , pp. 1
    • Cooray, A.1    Sheth, R.K.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.