Built on

T. Konstandin, R. A. Porto, and H. Rubira, JCAP 11
Original
1906
Earlier work this paper cites.
S. Floerchinger, M. Garny, A. Katsis, N. Tetradis, and U. A. Wiedemann, JCAP 09
Original
1907
Earlier work this paper cites.
A. Oddo, E. Sefusatti, C. Porciani, P. Monaco, and A. G. Sánchez, JCAP 03
Original
1908
Earlier work this paper cites.
C. Hahn, F. Villaescusa-Navarro, E. Castorina, and R. Scoccimarro, JCAP 03
Original
1909
Earlier work this paper cites.
G. Cabass and F. Schmidt, JCAP 04
Original
1909
Earlier work this paper cites.
N. Kaiser, Astrophys. J. Lett. 284
1984
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J. M. Bardeen, J. R. Bond, N. Kaiser, and A. S. Szalay, Astrophys. J. 304
1986
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M. H. Goroff, B. Grinstein, S. J. Rey, and M. B. Wise, Astrophys. J. 311
1986
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J. N. Fry and E. Gaztanaga, Astrophys. J. 413
1993
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R. J. Scherrer and D. H. Weinberg, Astrophys. J. 504
1998
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R. Scoccimarro, S. Colombi, J. N. Fry, J. A. Frieman, E. Hivon, and A. Melott, Astrophys. J. 496
1998
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T. Matsubara, Astrophys. J. 525
1999
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R. Scoccimarro, Astrophys. J. 544
2000
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C. W. Bauer, S. Fleming, D. Pirjol, and I. W. Stewart, Phys. Rev. D 63
2001
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F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, Phys. Rept. 367
2002
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M. Beneke, A. P. Chapovsky, M. Diehl, and T. Feldmann, Nucl. Phys. B 643
2002
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T. Eifler, H. Miyatake, E. Krause, C. Heinrich, V. Miranda, C. Hirata, J. Xu, S. Hemmati, M. Simet, P. Capak, A. Choi, O. Doré, C. Doux, X. Fang, R. Hounsell, E. Huff, H.-J. Huang, M. Jarvis, J. Kruk, D. Masters, E. Rozo, D. Scolnic, D. N. Spergel, M. Troxel, A. von der Linden, Y. Wang, D. H. Weinberg, L. Wenzl, and H.-Y. Wu, MNRAS (2021), 10.1093/mnras/stab1762 , arXiv:2004.05271 [astro-ph.CO]
Original
2004
Earlier work this paper cites.
Y. Donath and L. Senatore, JCAP 10
Original
2005
Earlier work this paper cites.
T. Hahn, Comput. Phys. Commun. 168
2005
Earlier work this paper cites.
E. Sefusatti, M. Crocce, S. Pueblas, and R. Scoccimarro, Phys. Rev. D 74
2006
Earlier work this paper cites.
A. Taruya, T. Nishimichi, and D. Jeong, Phys. Rev. D 103
Original
2007
Earlier work this paper cites.

Similar

R. Takahashi, Prog. Theor. Phys. 120
Original
2008
Cited alongside, same era.
M. Garny and P. Taule, JCAP 01
Original
2008
Cited alongside, same era.
S. Pueblas and R. Scoccimarro, Phys. Rev. D 80
Original
2009
Cited alongside, same era.
T. Steele and T. Baldauf, Phys. Rev. D 103
Original
2009
Cited alongside, same era.
D. Gualdi, S. Novell, H. Gil-Marín, and L. Verde, JCAP 01
Original
2009
Cited alongside, same era.

Then

G.-B. Zhao et al. , Mon. Not. Roy. Astron. Soc. 457
Original
2016
Later among the works it cites.
T. Abbott et al. (DES), Mon. Not. Roy. Astron. Soc. 460
Original
2016
Later among the works it cites.
A. Aghamousa et al. (DESI), (2016), arXiv:1611.00036 [astro-ph.IM]
Original
2016
Later among the works it cites.
A. A. Abolhasani, M. Mirbabayi, and E. Pajer, JCAP 05
Original
2016
Later among the works it cites.
T. Baldauf, M. Mirbabayi, M. Simonović, and M. Zaldarriaga, (2016), arXiv:1602.00674 [astro-ph.CO]
Original
2016

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2021

The two-loop bispectrum of large-scale structure

Baldauf, Tobias, Garny, Mathias, Taule, Petter et al.

Understand

The bispectrum is the leading non-Gaussian statistic in large-scale structure, carrying valuable information on cosmology that is complementary to the power spectrum.

To access this information, we need to model the bispectrum in the weakly non-linear regime.
In this work we present the first two-loop, i.e., next-to-next-to-leading order perturbative description of the bispectrum within an effective field theory (EFT) framework.
Using an analytic expansion of the perturbative kernels up to $F_6$ we derive a renormalized bispectrum that is demonstrated to be independent of the UV cutoff.

Built on

T. Konstandin, R. A. Porto, and H. Rubira, JCAP 11
Original
1906
Earlier work this paper cites.
S. Floerchinger, M. Garny, A. Katsis, N. Tetradis, and U. A. Wiedemann, JCAP 09
Original
1907
Earlier work this paper cites.
A. Oddo, E. Sefusatti, C. Porciani, P. Monaco, and A. G. Sánchez, JCAP 03
Original
1908
Earlier work this paper cites.
C. Hahn, F. Villaescusa-Navarro, E. Castorina, and R. Scoccimarro, JCAP 03
Original
1909
Earlier work this paper cites.
G. Cabass and F. Schmidt, JCAP 04
Original
1909
Earlier work this paper cites.
N. Kaiser, Astrophys. J. Lett. 284
1984
Earlier work this paper cites.
J. M. Bardeen, J. R. Bond, N. Kaiser, and A. S. Szalay, Astrophys. J. 304
1986
Earlier work this paper cites.
M. H. Goroff, B. Grinstein, S. J. Rey, and M. B. Wise, Astrophys. J. 311
1986
Earlier work this paper cites.
J. N. Fry and E. Gaztanaga, Astrophys. J. 413
1993
Earlier work this paper cites.
R. J. Scherrer and D. H. Weinberg, Astrophys. J. 504
1998
Earlier work this paper cites.
R. Scoccimarro, S. Colombi, J. N. Fry, J. A. Frieman, E. Hivon, and A. Melott, Astrophys. J. 496
1998
Earlier work this paper cites.
T. Matsubara, Astrophys. J. 525
1999
Earlier work this paper cites.
R. Scoccimarro, Astrophys. J. 544
2000
Earlier work this paper cites.
C. W. Bauer, S. Fleming, D. Pirjol, and I. W. Stewart, Phys. Rev. D 63
2001
Earlier work this paper cites.
F. Bernardeau, S. Colombi, E. Gaztanaga, and R. Scoccimarro, Phys. Rept. 367
2002
Earlier work this paper cites.
M. Beneke, A. P. Chapovsky, M. Diehl, and T. Feldmann, Nucl. Phys. B 643
2002
Earlier work this paper cites.
T. Eifler, H. Miyatake, E. Krause, C. Heinrich, V. Miranda, C. Hirata, J. Xu, S. Hemmati, M. Simet, P. Capak, A. Choi, O. Doré, C. Doux, X. Fang, R. Hounsell, E. Huff, H.-J. Huang, M. Jarvis, J. Kruk, D. Masters, E. Rozo, D. Scolnic, D. N. Spergel, M. Troxel, A. von der Linden, Y. Wang, D. H. Weinberg, L. Wenzl, and H.-Y. Wu, MNRAS (2021), 10.1093/mnras/stab1762 , arXiv:2004.05271 [astro-ph.CO]
Original
2004
Earlier work this paper cites.
Y. Donath and L. Senatore, JCAP 10
Original
2005
Earlier work this paper cites.
T. Hahn, Comput. Phys. Commun. 168
2005
Earlier work this paper cites.
E. Sefusatti, M. Crocce, S. Pueblas, and R. Scoccimarro, Phys. Rev. D 74
2006
Earlier work this paper cites.
A. Taruya, T. Nishimichi, and D. Jeong, Phys. Rev. D 103
Original
2007
Earlier work this paper cites.