Name: Theoretical Modeling of Large-Scale Structure of the Universe
Start: 2024-06-03T08:45:00+00:00
End: 2024-06-05T17:00:00+00:00
Location: No location set

Theoretical Modeling of Large-Scale Structure of the Universe

from Monday 3 June 2024 (08:45) to Wednesday 5 June 2024 (17:00)

Monday 3 June 2024

08:45 Registration and badge pick-up (Reception, Royal Observatory of Edinburgh)
Registration and badge pick-up (Reception, Royal Observatory of Edinburgh)
08:45 - 09:15

09:15

09:15 - 09:30
09:30
09:30 - 10:30
Contributions

09:30 EFT of LSS (D'Amico)

10:00 EFT of LSS (Zhang)
10:30 Break
Break
10:30 - 11:00
11:00
11:00 - 12:30
Contributions

11:00 Integrated perturbation theory for scalar and tensor fields (Matsubara)

11:30 Intrinsic alignments (Kokron)

12:00 The bispectrum in LPT (Chen)
12:30 Lunch
Lunch
12:30 - 13:30
13:30
13:30 - 14:00
Contributions

13:30 Galaxy bias renormalization group (Rubira)
14:00 Panel led discussion: New domains for Perturbation Theory
Panel led discussion: New domains for Perturbation Theory
14:00 - 14:30
Castorina (moderator): Akitsu, Chen, Ivanov, Matsubara
14:30
14:30 - 15:00
Contributions

14:30 Optimal Transport Reconstruction of Large Scale Structures (Nikakhtar)
15:00 Break
Break
15:00 - 15:30
15:30
15:30 - 16:30
Contributions

15:30 What makes a filament? (Feldbrugge)

16:00 The energy principle for the shape of protohaloes (Musso)
16:30 spotlights
spotlights
16:30 - 17:00

17:00 reception
reception
17:00 - 18:00
Tuesday 4 June 2024
09:00
09:00 - 10:34
Contributions

09:00 Fast numerical methods for cosmological inference from LSS (Hahn)

09:30 Hermes - Towards an Ultimate High-Performance Algorithm for Cosmic Statistics of Large Data Sets (Feng)

09:47 CLASS-OneLoop: Presentation and mock data analysis (Linde)

10:17 CLASS-OneLoop: Numerical Implementation and Outlook (Lesgourgues)
10:34 Break
Break
10:34 - 11:04
11:04
11:04 - 12:38
Contributions

11:04 Predicting non-linear effects in matter clustering from changes in cosmology and baryons using multi-fidelity simulations (Conley)

11:21 The “Missing baryons” in the cosmic web—what is it? Where is it? How much? (Ma)

11:38 Hybrid Lagrangian models (Zennaro)

12:08 HYMALAIA: A Hybrid Lagrangian Model for Intrinsic Alignments (Maion)
12:38 Lunch
Lunch
12:38 - 13:38
13:38
13:38 - 14:55
Contributions

13:38 Extending Hybrid Models of structure formation (Pellejero)

14:08 Field-level emulation of cosmic structure formation with styled neural networks (Jamieson)

14:25 Perturbative Forward-Modeling of Large-Scale Structure for Field-Level Analysis and Beyond (Stadler)
14:55 Break
Break
14:55 - 15:30
15:30
15:30 - 16:00
Contributions

15:30 How much information is left in galaxy clustering beyond the power spectrum? (Akitsu)
16:00 Panel led discussion: Simulations and theory
Panel led discussion: Simulations and theory
16:00 - 16:30
Peacock (moderator): Conley, Hall, Kokron, Pellejero, Stadler

16:30 Panel led discussion: Status of numerical implementations of PT – What’s “done”? What are their strengths? What’s missing?
Panel led discussion: Status of numerical implementations of PT – What’s “done”? What are their strengths? What’s missing?
16:30 - 17:00
Neveux (moderator): Aviles, D'Amico or Zhang, Lesgourgues, Philcox, Zennaro

20:00 Conference dinner
Conference dinner
20:00 - 21:30
Wednesday 5 June 2024
09:00
09:00 - 10:30
Contributions

09:00 Building the EFT of LSS beyond the standard model (Castorina)

09:30 Large scale structure formation in theories with scale dependent linear growth (Aviles)

10:00 Issues for perturbative methods at higher redshift (White)
10:30 Break
Break
10:30 - 11:00
11:00
11:00 - 12:30
Contributions

11:00 New tests of dark matter and inflation with BOSS using perturbation theory (Ivanov)

11:30 PNG in LSS modeling and analyses (Philcox)

12:00 Field level bias modeling, assembly bias, and primordial non-Gaussianity (Sullivan)
12:30 Lunch
Lunch
12:30 - 13:30

13:30 Panel led discussion: "Limits of pt, setting external priors, setting k_NL, how to squeeze info from LSS on small scales"
Panel led discussion: "Limits of pt, setting external priors, setting k_NL, how to squeeze info from LSS on small scales"
13:30 - 14:00
Carrilho (moderator), D'Amico or Zhang, Tsedrik, Sullivan
14:00
14:00 - 15:00
Contributions

14:00 Emission line galaxies: local PNG bias (Desjacques)

14:30 Tomographic analysis with the weak lensing convergence one-point statistics (Castiblanco, presented by Harnois-Deraps)
15:00 Break
Break
15:00 - 15:30
15:30
15:30 - 16:30
Contributions

15:30 The Effective Field Theory of Large-Scale Structure and Multi-tracer (Voivodic)

16:00 Going beyond redshift-space distortions with the streaming model (Dam)
16:30 Panel or moderated discussion: Status of perturbation theory and priorities for addressing challenges to come given the amount of survey data coming in the next decade
Panel or moderated discussion: Status of perturbation theory and priorities for addressing challenges to come given the amount of survey data coming in the next decade
16:30 - 17:00

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