Fetching the paper…
Reading the bibliography…
We study the scale-dependence of halo bias in generic (non-local) primordial non-Gaussian (PNG) initial conditions of the type motivated by inflation, parametrized by an arbitrary quadratic kernel.
1903
Earlier work this paper cites.
B. Grinstein and M. B. Wise, “Non-Gaussian fluctuations and the correlations of galaxies or rich clusters of galaxies,” ApJ 310
1986
Earlier work this paper cites.
J. M. Bardeen, J. R. Bond, N. Kaiser, and A. S. Szalay, “The statistics of peaks of Gaussian random fields,” ApJ 304
1986
Earlier work this paper cites.
S. Matarrese, F. Lucchin, and S. A. Bonometto, “A path-integral approach to large-scale matter distribution originated by non-Gaussian fluctuations,” ApJ. Lett. 310
1986
Earlier work this paper cites.
S. Cole and N. Kaiser, “Biased clustering in the cold dark matter cosmogony,” MNRAS 237
1989
Earlier work this paper cites.
D. S. Salopek and J. R. Bond, “Nonlinear evolution of long-wavelength metric fluctuations in inflationary models,” Phys. Rev. D 42
1990
Earlier work this paper cites.
1990
Earlier work this paper cites.
J. A. Peacock and A. F. Heavens, “Alternatives to the Press-Schechter cosmological mass function,” MNRAS 243
1990
Earlier work this paper cites.
D. S. Salopek and J. R. Bond, “Stochastic inflation and nonlinear gravity,” Phys. Rev. D 43
1991
Earlier work this paper cites.
J. R. Bond, S. Cole, G. Efstathiou, and N. Kaiser, “Excursion set mass functions for hierarchical Gaussian fluctuations,” ApJ 379
1991
Earlier work this paper cites.
J. N. Fry and E. Gaztanaga, “Biasing and hierarchical statistics in large-scale structure,” ApJ 413
1993
Earlier work this paper cites.
C. Lacey and S. Cole, “Merger rates in hierarchical models of galaxy formation,” MNRAS 262
1993
Earlier work this paper cites.
A. Linde and V. Mukhanov, “Non-Gaussian isocurvature perturbations from inflation,” Phys. Rev. D 56
1997
Earlier work this paper cites.
H. J. Mo, Y. P. Jing, and S. D. M. White, “High-order correlations of peaks and haloes: a step towards understanding galaxy biasing,” MNRAS 284
1997
Earlier work this paper cites.
R. Scoccimarro, “Transients from initial conditions: a perturbative analysis,” MNRAS 299
1998
Earlier work this paper cites.
A. F. Heavens, S. Matarrese, and L. Verde, “The non-linear redshift-space power spectrum of galaxies,” MNRAS 301
1998
Earlier work this paper cites.
C. Armendáriz-Picón, T. Damour, and V. Mukhanov, “k-Inflation,” Physics Letters B 458
1999
Earlier work this paper cites.
R.K. Sheth and G. Lemson, “Biasing and the distribution of dark matter haloes,” MNRAS 304
1999
Earlier work this paper cites.
R. Scoccimarro, “Gravitational Clustering from χ 2 \chi^{2} Initial Conditions,” ApJ 542
2000
Earlier work this paper cites.
R. Scoccimarro, R.K. Sheth, L. Hui, and B. Jain, “How Many Galaxies Fit in a Halo? Constraints on Galaxy Formation Efficiency from Spatial Clustering,” ApJ 546
2001
Earlier work this paper cites.
D. H. Lyth and D. Wands, “Generating the curvature perturbation without an inflaton,” Physics Letters B 524
2002
Earlier work this paper cites.
K. Enqvist and M. S. Sloth, “Adiabatic CMB perturbations in pre-Big-Bang string cosmology,” Nuclear Physics B 626
2002
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, “Large-scale structure of the Universe and cosmological perturbation theory.” Phys. Rep. 367
2002
Earlier work this paper cites.
M. White, “The Mass Function,” ApJS 143
2002
Earlier work this paper cites.
J. Maldacena, “Non-gaussian features of primordial fluctuations in single field inflationary models,” Journal of High Energy Physics 5
2003
Earlier work this paper cites.
F. Bernardeau and J. Uzan, “Inflationary models inducing non-Gaussian metric fluctuations,” Phys. Rev. D 67
2003
Earlier work this paper cites.
L. Kofman, “Probing String Theory with Modulated Cosmological Fluctuations,” ArXiv Astrophysics e-prints (2003), arXiv:astro-ph/0303614
2003
Earlier work this paper cites.
F. Bernardeau, L. Kofman, and J.-P. Uzan, “Modulated fluctuations from hybrid inflation,” Phys. Rev. D 70
2004
Earlier work this paper cites.
M. Zaldarriaga, “Non-Gaussianities in models with a varying inflaton decay rate,” Phys. Rev. D 69
2004
Earlier work this paper cites.
M. Alishahiha, E. Silverstein, and D. Tong, “DBI in the sky: Non-Gaussianity from inflation with a speed limit,” Phys. Rev. D 70
2004
Earlier work this paper cites.
E. Silverstein and D. Tong, “Scalar speed limits and cosmology: Acceleration from D-cceleration,” Phys. Rev. D 70
2004
Earlier work this paper cites.
K. Enqvist, A. Jokinen, A. Mazumdar, T. Multamäki, and A. Väihkönen, “Non-Gaussianity from preheating,” Physical Review Letters 94
2005
Earlier work this paper cites.
E. Sirko, “Initial Conditions to Cosmological N-Body Simulations, or, How to Run an Ensemble of Simulations,” ApJ 634
2005
Earlier work this paper cites.
V. Springel, “The cosmological simulation code GADGET-2,” MNRAS 364
2005
Earlier work this paper cites.
N. Barnaby and J. M. Cline, “Non-Gaussian and nonscale-invariant perturbations from tachyonic preheating in hybrid inflation,” Phys. Rev. D 73
2006
Cited alongside, same era.
C. T. Byrnes, M. Sasaki, and D. Wands, “Primordial trispectrum from inflation,” Phys. Rev. D 74
2006
Cited alongside, same era.
K. M. Smith and M. Zaldarriaga, “Algorithms for bispectra: forecasting, optimal analysis, and simulation,” ArXiv Astrophysics e-prints (2006), astro-ph/0612571
2006
Cited alongside, same era.
M. Crocce, S. Pueblas, and R. Scoccimarro, “Transients from initial conditions in cosmological simulations,” MNRAS 373
2006
Cited alongside, same era.
P. McDonald, “Clustering of dark matter tracers: Renormalizing the bias parameters,” Phys. Rev. D 74
2006
Cited alongside, same era.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
Q.-G. Huang, “Scale dependence of f NL
2010
Later among the works it cites.
F. Schmidt and M. Kamionkowski, “Halo clustering with nonlocal non-Gaussianity,” Phys. Rev. D 82
alphaXiv searches the wider corpus for related work and actual follow-ups.
alphaXiv is searching for related work…
X. Chen, M.-x. Huang, S. Kachru, and G. Shiu, “Observational signatures and non-Gaussianities of general single-field inflation,” JCAP 1
2007
Cited alongside, same era.
N. Barnaby and J. M. Cline, “Non-Gaussianity from tachyonic preheating in hybrid inflation,” Phys. Rev. D 75
2007
Cited alongside, same era.
2007
Cited alongside, same era.
R. E. Smith, R. Scoccimarro, and R. K. Sheth, “Scale dependence of halo and galaxy bias: Effects in real space,” Phys. Rev. D 75
2007
Cited alongside, same era.
D. S. Reed, R. Bower, C. S. Frenk, A. Jenkins, and T. Theuns, “The halo mass function from the dark ages through the present day,” MNRAS 374
2007
Cited alongside, same era.
2008
Cited alongside, same era.
2008
Cited alongside, same era.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2010
Later among the works it cites.
2011
Closest in time.
A. Ashoorioon and G. Shiu, “A note on calm excited states of inflation,” JCAP 3
2011
Closest in time.
2011
Closest in time.
E. Sefusatti, M. Crocce, and V. Desjacques, “The halo bispectrum in N-body simulations with non-Gaussian initial conditions,” In preparation (2011)
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.
C. McBride et al, In preparation (2011)
2011
Closest in time.
Q. Mao, A.A. Berlind, C. McBride, R. Scherrer, R. Scoccimarro, and M. Manera, “Constraining primordial non-gaussianity with skewness and kurtosis measurements of large-scale structure,” In preparation (2011)
2011
Closest in time.
M. Manera and E. Gaztanaga, “The Local Bias Model in the Large Scale Halo Distribution,” MNRAS 415
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.
2011
Closest in time.