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Volumn 2011, Issue 4, 2011, Pages

Primordial non-Gaussianity in the bispectrum of the halo density field

Author keywords

galaxy clustering; inflation; non gaussianity; power spectrum

Indexed keywords


EID: 79955573409     PISSN: 14757516     EISSN: 14757516     Source Type: Journal    
DOI: 10.1088/1475-7516/2011/04/006     Document Type: Article
Times cited : (121)

References (63)
  • 1
    • 78349237006 scopus 로고    scopus 로고
    • Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure
    • M. Liguori, E. Sefusatti, J.R. Fergusson and E.P.S. Shellard, 2010 Primordial non-Gaussianity and Bispectrum Measurements in the Cosmic Microwave Background and Large-Scale Structure Adv. Astron. 2010 980523 [1001.4707]
    • (2010) Adv. Astron. , vol.2010 , pp. 980523
    • Liguori, M.1    Sefusatti, E.2    Fergusson, J.R.3    Shellard, E.P.S.4
  • 2
    • 85017228910 scopus 로고    scopus 로고
    • Primordial non-Gaussianity from the large scale structure
    • V. Desjacques and U. Seljak, 2010 Primordial non-Gaussianity from the large scale structure, Class. Quant. Grav. 27 124011 [1003.5020]
    • (2010) Class. Quant. Grav. , vol.27 , Issue.12 , pp. 124011
    • Desjacques, V.1    Seljak, U.2
  • 3
    • 33744732338 scopus 로고
    • The Inflationary Universe: A Possible Solution to the Horizon and Flatness Problems
    • A.H. Guth, 1981 The Inflationary Universe: A Possible Solution To The Horizon And Flatness Problems, Phys. Rev. D 23 347
    • (1981) Phys. Rev. , vol.23 , pp. 347
    • Guth, A.H.1
  • 4
    • 0000511848 scopus 로고
    • A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems
    • A.D. Linde, 1982 A New Inflationary Universe Scenario: A Possible Solution of the Horizon, Flatness, Homogeneity, Isotropy and Primordial Monopole Problems, Phys. Lett. B 108 389
    • (1982) Phys. Lett. , vol.108 , pp. 389
    • Linde, A.D.1
  • 5
    • 33744766749 scopus 로고
    • Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking
    • A. Albrecht and P.J. Steinhardt, 1982 Cosmology for Grand Unified Theories with Radiatively Induced Symmetry Breaking, Phys. Rev. Lett. 48 1220
    • (1982) Phys. Rev. Lett. , vol.48 , pp. 1220
    • Albrecht, A.1    Steinhardt, P.J.2
  • 7
    • 79551521249 scopus 로고    scopus 로고
    • Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
    • WMAP collaboration
    • WMAP collaboration, E. Komatsu et al., 2011 Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation, Astrophys. J. Suppl. 192 18 [1001.4538]
    • (2011) Astrophys. J. Suppl. , vol.192 , Issue.2 , pp. 18
    • Komatsu, E.1
  • 8
    • 18444383344 scopus 로고    scopus 로고
    • Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering
    • [astro-ph/0412626]
    • E. Sefusatti and R. Scoccimarro, 2005 Galaxy Bias and Halo-Occupation Numbers from Large-Scale Clustering, Phys. Rev. D 71 063001 [astro-ph/0412626]
    • (2005) Phys. Rev. , vol.71 , pp. 063001
    • Sefusatti, E.1    Scoccimarro, R.2
  • 9
    • 0000514184 scopus 로고
    • Nonlinear evolution of long wavelength metric fluctuations in inflationary models
    • D.S. Salopek and J.R. Bond, 1990 Nonlinear evolution of long wavelength metric fluctuations in inflationary models, Phys. Rev. D 42 3936
    • (1990) Phys. Rev. , vol.42 , pp. 3936
    • Salopek, D.S.1    Bond, J.R.2
  • 10
    • 23544453617 scopus 로고
    • Stochastic inflation and nonlinear gravity
    • D.S. Salopek and J.R. Bond, 1991 Stochastic inflation and nonlinear gravity, Phys. Rev. D 43 1005
    • (1991) Phys. Rev. , vol.43 , pp. 1005
    • Salopek, D.S.1    Bond, J.R.2
  • 12
    • 45249115446 scopus 로고    scopus 로고
    • The imprints of primordial non-Gaussianities on large-scale structure: Scale dependent bias and abundance of virialized objects
    • [0710.4560]
    • N. Dalal, O. Dore, D. Huterer and A. Shirokov, 2008 The imprints of primordial non-Gaussianities on large-scale structure: scale dependent bias and abundance of virialized objects, Phys. Rev. D 77 123514 [0710.4560]
    • (2008) Phys. Rev. , vol.77 , pp. 123514
    • Dalal, N.1    Dore, O.2    Huterer, D.3    Shirokov, A.4
  • 13
    • 52949154422 scopus 로고    scopus 로고
    • The effect of primordial non-Gaussianity on halo bias
    • S. Matarrese and L. Verde, 2008 The effect of primordial non-Gaussianity on halo bias, Astrophys. J. 677 L77 [0801.4826]
    • (2008) Astrophys. J. , vol.677 , Issue.2 , pp. 77
    • Matarrese, S.1    Verde, L.2
  • 14
    • 56349161653 scopus 로고    scopus 로고
    • Constraints on local primordial non-Gaussianity from large scale structure
    • [0805.3580]
    • A. Slosar, C. Hirata, U. Seljak, S. Ho and N. Padmanabhan, 2008 Constraints on local primordial non-Gaussianity from large scale structure J. Cosmol. Astropart. Phys. JCAP08(2008)031 [0805.3580]
    • (2008) J. Cosmol. Astropart. Phys. , vol.2008 , Issue.8 , pp. 031
    • Slosar, A.1    Hirata, C.2    Seljak, U.3    Ho, S.4    Padmanabhan, N.5
  • 16
    • 77649198888 scopus 로고    scopus 로고
    • Signature of primordial non-Gaussianity of φ3-type in the mass function and bias of dark matter haloes
    • 3-type in the mass function and bias of dark matter haloes, Phys. Rev. D 81 023006 [0907.2257]
    • (2010) Phys. Rev. , vol.81 , pp. 023006
    • Desjacques, V.1    Seljak, U.2
  • 21
    • 70350681281 scopus 로고    scopus 로고
    • Primordial non-Gaussianity, scale-dependent bias and the bispectrum of galaxies
    • [0904.0497]
    • D. Jeong and E. Komatsu, 2009 Primordial non-Gaussianity, scale-dependent bias and the bispectrum of galaxies, Astrophys. J. 703 1230 [0904.0497]
    • (2009) Astrophys. J. , vol.703 , Issue.2 , pp. 1230
    • Jeong, D.1    Komatsu, E.2
  • 22
    • 73349112861 scopus 로고    scopus 로고
    • 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions
    • [0905.0717]
    • E. Sefusatti, 2009 1-loop Perturbative Corrections to the Matter and Galaxy Bispectrum with non-Gaussian Initial Conditions, Phys. Rev. D 80 123002 [0905.0717]
    • (2009) Phys. Rev. , vol.80 , pp. 123002
    • Sefusatti, E.1
  • 24
    • 0039929391 scopus 로고
    • A Path Integral Approach to Large Scale Matter Distribution Originated by Nongaussian Fluctuations
    • S. Matarrese, F. Lucchin and S. A. Bonometto, 1986 A Path Integral Approach To Large Scale Matter Distribution Originated By Nongaussian Fluctuations Astrophys. J. 310 L21
    • (1986) Astrophys. J. , vol.310 , pp. 21
    • Matarrese, S.1    Lucchin, F.2    Bonometto, S.A.3
  • 25
    • 0037437973 scopus 로고    scopus 로고
    • The primordial density perturbation in the curvaton scenario
    • [astro-ph/0208055]
    • D.H. Lyth, C. Ungarelli and D. Wands, 2003 The primordial density perturbation in the curvaton scenario, Phys. Rev. D 67 023503 [astro-ph/0208055]
    • (2003) Phys. Rev. , vol.67 , pp. 023503
    • Lyth, D.H.1    Ungarelli, C.2    Wands, D.3
  • 26
    • 1642389072 scopus 로고    scopus 로고
    • On non-Gaussianity in the curvaton scenario
    • N. Bartolo, S. Matarrese and A. Riotto, 2004 On non-Gaussianity in the curvaton scenario, Phys. Rev. D 69 043503 [hep-ph/0309033]
    • (2004) Phys. Rev. , vol.69 , pp. 043503
    • Bartolo, N.1    Matarrese, S.2    Riotto, A.3
  • 27
    • 1642393860 scopus 로고    scopus 로고
    • Non-Gaussianities in models with a varying inflaton decay rate
    • M. Zaldarriaga, 2004 Non-Gaussianities in models with a varying inflaton decay rate, Phys. Rev. D 69 043508 [astro-ph/0306006]
    • (2004) Phys. Rev. , vol.69 , pp. 043508
    • Zaldarriaga, M.1
  • 28
    • 36749033321 scopus 로고    scopus 로고
    • A smooth bouncing cosmology with scale invariant spectrum
    • P. Creminelli and L. Senatore, 2007 A smooth bouncing cosmology with scale invariant spectrum J. Cosmol. Astropart. Phys. JCAP11(2007)010 [hep-th/0702165]
    • (2007) J. Cosmol. Astropart. Phys. , vol.2007 , Issue.11 , pp. 010
    • Creminelli, P.1    Senatore, L.2
  • 29
    • 77951612521 scopus 로고    scopus 로고
    • Structure formation from non-Gaussian initial conditions: Multivariate biasing, statistics and comparison with N-body simulations
    • T. Giannantonio and C. Porciani, 2010 Structure formation from non-Gaussian initial conditions: multivariate biasing, statistics and comparison with N-body simulations, Phys. Rev. D 81 063530 [0911.0017]
    • (2010) Phys. Rev. , vol.81 , pp. 063530
    • Giannantonio, T.1    Porciani, C.2
  • 30
    • 23044478124 scopus 로고    scopus 로고
    • Non-Gaussian features of primordial fluctuations in single field inflationary models
    • J.M. Maldacena, 2003 Non-Gaussian features of primordial fluctuations in single field inflationary models J. High Energy Phys. JHEP05(2003)013 [astro-ph/0210603]
    • (2003) J. High Energy Phys. , vol.2003 , Issue.5 , pp. 013
    • Maldacena, J.M.1
  • 31
    • 77955871606 scopus 로고    scopus 로고
    • Local non-Gaussianity from inflation
    • D. Wands, 2010 Local non-Gaussianity from inflation, Class. Quant. Grav. 27 124002 [1004.0818]
    • (2010) Class. Quant. Grav. , vol.27 , Issue.12 , pp. 124002
    • Wands, D.1
  • 32
    • 67649871529 scopus 로고    scopus 로고
    • Scale-dependent bias from primordial non-Gaussianity in general relativity
    • D. Wands and A. Slosar, 2009 Scale-dependent bias from primordial non-Gaussianity in general relativity, Phys. Rev. D 79 123507 [0902.1084]
    • (2009) Phys. Rev. , vol.79 , pp. 123507
    • Wands, D.1    Slosar, A.2
  • 33
    • 70449629088 scopus 로고    scopus 로고
    • A New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects
    • J. Yoo, A.L. Fitzpatrick and M. Zaldarriaga, 2009 A New Perspective on Galaxy Clustering as a Cosmological Probe: General Relativistic Effects, Phys. Rev. D 80 083514 [0907.0707]
    • (2009) Phys. Rev. , vol.80 , pp. 083514
    • Yoo, J.1    Fitzpatrick, A.L.2    Zaldarriaga, M.3
  • 34
    • 78651070202 scopus 로고    scopus 로고
    • General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?
    • J. Yoo, 2010 General Relativistic Description of the Observed Galaxy Power Spectrum: Do We Understand What We Measure?, Phys. Rev. D 82 083508 [1009.3021]
    • (2010) Phys. Rev. , vol.82 , pp. 083508
    • Yoo, J.1
  • 35
    • 0001429631 scopus 로고
    • Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation
    • W.H. Press and P. Schechter, 1974 Formation of galaxies and clusters of galaxies by selfsimilar gravitational condensation, Astrophys. J. 187 425
    • (1974) Astrophys. J. , vol.187 , pp. 425
    • Press, W.H.1    Schechter, P.2
  • 36
    • 0043124932 scopus 로고    scopus 로고
    • Large scale bias and the peak background split
    • R.K. Sheth and G. Tormen, 1999 Large scale bias and the peak background split, Mon. Not. Roy. Astron. Soc. 308 119 [astro-ph/9901122]
    • (1999) Mon. Not. Roy. Astron. Soc. , vol.308 , pp. 119
    • Sheth, R.K.1    Tormen, G.2
  • 37
    • 84879052549 scopus 로고    scopus 로고
    • Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures
    • M. LoVerde, A. Miller, S. Shandera and L. Verde, 2008 Effects of Scale-Dependent Non-Gaussianity on Cosmological Structures J. Cosmol. Astropart. Phys. JCAP04(2008)014 [0711.4126]
    • (2008) J. Cosmol. Astropart. Phys. , vol.2008 , Issue.4 , pp. 014
    • Loverde, M.1    Miller, A.2    Shandera, S.3    Verde, L.4
  • 38
    • 77953770901 scopus 로고    scopus 로고
    • The halo mass function from the excursion set method. III. First principle derivation for non-Gaussian theories
    • M. Maggiore and A. Riotto, 2010 The halo mass function from the excursion set method. III. First principle derivation for non-Gaussian theories, Astrophys. J. 717 526 [0903.1251]
    • (2010) Astrophys. J. , vol.717 , Issue.1 , pp. 526
    • Maggiore, M.1    Riotto, A.2
  • 39
    • 0034692203 scopus 로고    scopus 로고
    • The abundance of high-redshift objects as a probe of non-Gaussian initial conditions
    • S. Matarrese, L. Verde and R. Jimenez, 2000 The abundance of high-redshift objects as a probe of non-Gaussian initial conditions, Astrophys. J. 541 10 [astro-ph/0001366]
    • (2000) Astrophys. J. , vol.541 , Issue.1 , pp. 10
    • Matarrese, S.1    Verde, L.2    Jimenez, R.3
  • 40
    • 79952610499 scopus 로고    scopus 로고
    • An Improved Calculation of the Non-Gaussian Halo Mass Function
    • G. D'Amico, M. Musso, J. Norẽa and A. Paranjape, 2011 An Improved Calculation of the Non-Gaussian Halo Mass Function J. Cosmol. Astropart. Phys. JCAP02(2011)001 [1005.1203]
    • (2011) J. Cosmol. Astropart. Phys. , vol.2011 , Issue.2 , pp. 001
    • G. D'Amico1
  • 41
    • 58149161542 scopus 로고    scopus 로고
    • Primordial non-Gaussianity: Large-scale structure signature in the perturbative bias model
    • P. McDonald, 2008 Primordial non-Gaussianity: large-scale structure signature in the perturbative bias model, Phys. Rev. D 78 123519 [0806.1061]
    • (2008) Phys. Rev. , vol.78 , pp. 123519
    • McDonald, P.1
  • 42
    • 33750920086 scopus 로고    scopus 로고
    • Clustering of dark matter tracers: Renormalizing the bias parameters
    • P. McDonald, 2006 Clustering of dark matter tracers: renormalizing the bias parameters, Phys. Rev. D 74 103512 [astro-ph/0609413]
    • (2006) Phys. Rev. , vol.74 , pp. 103512
    • McDonald, P.1
  • 43
    • 70349883877 scopus 로고    scopus 로고
    • Calibrating the Baryon Oscillation Ruler for Matter and Halos
    • N. Padmanabhan and M. White, 2009 Calibrating the Baryon Oscillation Ruler for Matter and Halos, Phys. Rev. D 80 063508 [0906.1198]
    • (2009) Phys. Rev. , vol.80 , pp. 063508
    • Padmanabhan, N.1    White, M.2
  • 45
    • 1542712787 scopus 로고    scopus 로고
    • An Analytic model for the spatial clustering of dark matter halos
    • H.J. Mo and S.D.M. White, 1996 An Analytic model for the spatial clustering of dark matter halos Mon. Not. Roy. Astron. Soc. 282 347 [astro-ph/9512127]
    • (1996) Mon. Not. Roy. Astron. Soc. , vol.282 , Issue.2 , pp. 347
    • Mo, H.J.1    White, S.D.M.2
  • 46
    • 1542501820 scopus 로고    scopus 로고
    • The Correlation Function of Clusters of Galaxies and the Amplitude of Mass Fluctuations in the Universe
    • H.J. Mo, Y.P. Jing and S.D.M. White, 1996 The Correlation Function of Clusters of Galaxies and the Amplitude of Mass Fluctuations in the Universe Mon. Not. Roy. Astron. Soc. 282 1096 [astro-ph/9602052]
    • (1996) Mon. Not. Roy. Astron. Soc. , vol.282 , Issue.3 , pp. 1096
    • Mo, H.J.1    Jing, Y.P.2    White, S.D.M.3
  • 47
    • 0036314605 scopus 로고    scopus 로고
    • Large-scale structure of the universe and cosmological perturbation theory
    • F. Bernardeau, S. Colombi, E. Gaztãaga 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
    • F. Bernardeau1
  • 48
    • 58149161542 scopus 로고    scopus 로고
    • Primordial non-Gaussianity: Large-scale structure signature in the perturbative bias model
    • P. McDonald, 2008 Primordial non-Gaussianity: large-scale structure signature in the perturbative bias model, Phys. Rev. D 78 123519 [0806.1061]
    • (2008) Phys. Rev. , vol.78 , pp. 123519
    • McDonald, P.1
  • 49
    • 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. , vol.73 , pp. 063519
    • Crocce, M.1    Scoccimarro, R.2
  • 51
    • 0003145068 scopus 로고
    • Coupling of Modes of Cosmological Mass Density Fluctuations
    • M.H. Goroff, B. Grinstein, S.J. Rey and M.B. Wise, 1986 Coupling of Modes of Cosmological Mass Density Fluctuations, Astrophys. J. 311 6
    • (1986) Astrophys. J. , vol.311 , pp. 6
    • Goroff, M.H.1    Grinstein, B.2    Rey, S.J.3    Wise, M.B.4
  • 52
    • 4243678307 scopus 로고    scopus 로고
    • Loop Corrections in Non-Linear Cosmological Perturbation Theory
    • R. Scoccimarro and J. Frieman, 1996 Loop Corrections in Non-Linear Cosmological Perturbation Theory, Astrophys. J. Suppl. 105 37 [astro-ph/9509047]
    • (1996) Astrophys. J. Suppl. , vol.105 , pp. 37
    • Scoccimarro, R.1    Frieman, J.2
  • 53
    • 41549089575 scopus 로고    scopus 로고
    • Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
    • 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. , vol.77 , pp. 063530
    • Matsubara, T.1
  • 54
    • 58649111949 scopus 로고    scopus 로고
    • Signature of Primordial Non-Gaussianity on Matter Power Spectrum
    • A. Taruya, K. Koyama and T. Matsubara, 2008 Signature of Primordial Non-Gaussianity on Matter Power Spectrum, Phys. Rev. D 78 123534 [0808.4085]
    • (2008) Phys. Rev. , vol.78 , pp. 123534
    • Taruya, A.1    Koyama, K.2    Matsubara, T.3
  • 55
    • 85174220674 scopus 로고    scopus 로고
    • The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions
    • E. Sefusatti, M. Crocce and V. Desjacques, 2010 The Matter Bispectrum in N-body Simulations with non-Gaussian Initial Conditions Mon. Not. Roy. Astron. Soc. 406 1014 [1003.0007]
    • (2010) Mon. Not. Roy. Astron. Soc. , vol.406 , pp. 1014
    • Sefusatti, E.1    Crocce, M.2    Desjacques, V.3
  • 56
    • 35649001011 scopus 로고    scopus 로고
    • The bispectrum of galaxies from high-redshift galaxy surveys: Primordial non-Gaussianity and non-linear galaxy bias
    • E. Sefusatti and E. Komatsu, 2007 The bispectrum of galaxies from high-redshift galaxy surveys: Primordial non-Gaussianity and non-linear galaxy bias, Phys. Rev. D 76 083004 [0705.0343]
    • (2007) Phys. Rev. , vol.76 , pp. 083004
    • Sefusatti, E.1    Komatsu, E.2
  • 57
    • 77954283947 scopus 로고    scopus 로고
    • Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations
    • T. Nishimichi, A. Taruya, K. Koyama and C. Sabiu, 2010 Scale Dependence of Halo Bispectrum from Non-Gaussian Initial Conditions in Cosmological N-body Simulations J. Cosmol. Astropart. Phys. JCAP07(2010)002 [0911.4768]
    • (2010) J. Cosmol. Astropart. Phys. , vol.2010 , Issue.7 , pp. 002
    • Nishimichi, T.1    Taruya, A.2    Koyama, K.3    Sabiu, C.4
  • 58
    • 79955627927 scopus 로고    scopus 로고
    • private communication
    • T. Nishimichi, private communication
    • Nishimichi, T.1
  • 59
    • 3042740884 scopus 로고    scopus 로고
    • Probing Primordial Non-Gaussianity with Large-Scale Structure
    • R. Scoccimarro, E. Sefusatti and M. Zaldarriaga, 2004 Probing Primordial Non-Gaussianity with Large-Scale Structure, Phys. Rev. D 69 103513 [astro-ph/0312286]
    • (2004) Phys. Rev. , vol.69 , pp. 103513
    • Scoccimarro, R.1    Sefusatti, E.2    Zaldarriaga, M.3
  • 62
    • 48349098532 scopus 로고    scopus 로고
    • An analytic model for the bispectrum of galaxies in redshift space
    • R.E. Smith, R.K. Sheth and R. Scoccimarro, 2008 An analytic model for the bispectrum of galaxies in redshift space, Phys. Rev. D 78 023523 [0712.0017]
    • (2008) Phys. Rev. , vol.78 , pp. 023523
    • Smith, R.E.1    Sheth, R.K.2    Scoccimarro, R.3
  • 63
    • 33947397649 scopus 로고    scopus 로고
    • The Scale Dependence of Halo and Galaxy Bias: Effects in Real Space
    • R.E. Smith, R. Scoccimarro and R.K. Sheth, 2007 The Scale Dependence of Halo and Galaxy Bias: Effects in Real Space, Phys. Rev. D 75 063512 [astro-ph/0609547]
    • (2007) Phys. Rev. , vol.75 , pp. 063512
    • Smith, R.E.1    Scoccimarro, R.2    Sheth, R.K.3


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