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It is usually assumed that the angular momentum (AM) of dark matter halos arises during the linear stages of structure formation, as a consequence of the coupling between the proto-haloes' shape and the tidal field produced by their…

宇宙学与河外天体物理 · 物理学 2024-04-08 Pablo López

The alignment between halo spins and the cosmic web is still poorly understood despite being a widely studied topic. Here, we study this alignment within the context of tidal torque theory (TTT) and deviations from it. To this end, we…

星系天体物理 · 物理学 2021-02-19 Pablo López , Marius Cautun , Dante Paz , Manuel Merchán , Rien van de Weygaert

The standard explanation for galaxy spin starts with the tidal-torque theory (TTT), in which an ellipsoidal dark-matter protohalo, which comes to host the galaxy, is torqued up by the tidal gravitational field around it. We discuss a…

宇宙学与河外天体物理 · 物理学 2020-03-26 Mark C. Neyrinck , Miguel A. Aragon-Calvo , Bridget Falck , Alexander S. Szalay , Jie Wang

The peak model of structure formation was built more than fifty years ago with the aim to address the origin of dark matter halo rotation in the tidal torque theory (TTT). Paradoxically, it has allowed one to explain and reproduce all halo…

宇宙学与河外天体物理 · 物理学 2025-12-01 Eduard Salvador-Solé , Alberto Manrique

The tidal torque theory (TTT) relates the origin and evolution of angular momentum with the environment in which dark matter (DM) haloes form. The deviations introduced by late non-linearities are commonly thought as noise in the model. In…

宇宙学与河外天体物理 · 物理学 2019-03-14 Pablo López , Manuel E. Merchán , Dante J. Paz

In the tidal-torque theory, the angular momentum (AM) of dark matter halos arises from the tidal torque suffered by aspherical collapsing patches due to surrounding mass fluctuations. This theory was implemented in the peak model where…

宇宙学与河外天体物理 · 物理学 2025-04-01 Eduard Salvador-Solé , Alberto Manrique

We investigate the spin alignment of the dark matter halos by considering a mechanism somewhat similar to tidal locking. We dubbed it Tidal Locking Theory (TLT). While Tidal Torque Theory is responsible for the initial angular momentum of…

宇宙学与河外天体物理 · 物理学 2024-03-05 E. Ebrahimian , A. A. Abolhasani

Large scale tidal field estimated directly from the distribution of dark matter halos is used to investigate how halo shapes and spin vectors are aligned with the cosmic web. The major, intermediate and minor axes of halos are aligned with…

宇宙学与河外天体物理 · 物理学 2016-07-06 Sijie Chen , Huiyuan Wang , H. J. Mo , Jingjing Shi

We evaluate the success of linear tidal-torque theory (TTT) in predicting galactic-halo spin using a cosmological N-body simulation with thousands of well-resolved haloes. The proto-haloes are identified by tracing today's haloes back to…

天体物理学 · 物理学 2009-11-06 Cristiano Porciani , Avishai Dekel , Yehuda Hoffman

We present a numerical evidence supporting the primordial origin of secondary halo bias even on the galactic mass scale. Analyzing the data from the IllustrisTNG 300-1 simulations, we investigate the dependence of halo bias on the degree of…

宇宙学与河外天体物理 · 物理学 2024-11-01 Jounghun Lee , Jun-Sung Moon

We study how halo intrinsic dynamical properties are linked to their formation processes for halos in two mass ranges, $10^{12}-10^{12.5}h^{-1}{\rm M_\odot}$ and $\ge 10^{13}h^{-1}{\rm M_\odot}$, and how both are correlated with the large…

宇宙学与河外天体物理 · 物理学 2015-05-07 Jingjing Shi , Huiyuan Wang , Houjun Mo

We present direct $N$-body simulations of tidally filling 30,000 ${\rm M}_\odot$ star clusters orbiting between 10 kpc and 100 kpc in galaxies with a range of dark matter substructure properties. The time-dependent tidal force is determined…

星系天体物理 · 物理学 2019-08-21 Jeremy J. Webb , Jo Bovy , Raymond G. Carlberg , Mark Gieles

Galaxy angular momentum directions (spins) are observable, well described by the Lagrangian tidal torque theory, and proposed to probe the primordial universe. They trace the spins of dark matter halos, and are indicators of protohalos…

宇宙学与河外天体物理 · 物理学 2021-03-24 Qiaoya Wu , Hao-Ran Yu , Shihong Liao , Min Du

The tidal torque theory (TTT) predicts that galaxy spins are correlated with the surrounding tidal field, reflecting how angular momentum is acquired during structure formation. We present a new observational test of this prediction using…

星系天体物理 · 物理学 2025-12-05 Jun-Sung Moon , Teppei Okumura

We investigate the cross-talk between the two key components of tidal-torque theory, the inertia (I) and shear (T) tensors, using a cosmological N-body simulation with thousands of well-resolved haloes. We find that the principal axes of I…

天体物理学 · 物理学 2009-11-06 Cristiano Porciani , Avishai Dekel , Yehuda Hoffman

We develop a new model within which the radius-dependent transition of the subhalo inner spins with respect to the cosmic web and the variation of the transition threshold radius ($r_{\rm th}$) with subhalo mass ($M_{\rm vir}$), smoothing…

宇宙学与河外天体物理 · 物理学 2023-07-26 Jun-Sung Moon , Jounghun Lee

We present a numerical evidence supporting the claim that the mass-dependent transitions of the halo spin orientations from the intermediate to the minor principal directions of the local tidal fields can in principle be a useful…

宇宙学与河外天体物理 · 物理学 2020-10-20 Jounghun Lee , Noam I Libeskind

Tidal torque theory (TTT) predicts that galaxy angular momenta are imprinted by the early tidal field acting on their proto-structures, which are preserved through cosmic evolution and provide the potentially most precise measurement of the…

宇宙学与河外天体物理 · 物理学 2025-12-15 Ming-Jie Sheng , Hao-Ran Yu , Min Bao , Bing-Hang Chen , Fang-Na Shao , Qi Guo , Yanmei Chen , Huiyuan Wang , Ue-Li Pen , Jie Wang , Xiaohu Yang

In the standard model of cosmology, structure emerges out of non-rotational flow and the angular momentum of collapsing halos is induced by tidal torques. The growth of halo angular momentum in the linear and quasi-linear phases is…

宇宙学与河外天体物理 · 物理学 2015-06-12 Noam I Libeskind , Yehuda Hoffman , Matthias Steinmetz , Stefan Gottloeber , Alexander Knebe , Steffen Hess

The correlation between the spins of dark matter halos and the large-scale structure (LSS) has been studied in great detail over a large redshift range, while investigations of galaxies are still incomplete. Motivated by this point, we use…

星系天体物理 · 物理学 2018-10-31 Peng Wang , Quan Guo , Xi Kang , Noam I. Libeskind
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