grgadget: an N-body TreePM relativistic code for cosmological simulations

被引:2
|
作者
Quintana-Miranda, Eduardo [1 ,2 ,3 ]
Monaco, Pierluigi [1 ,2 ,3 ,4 ]
Tornatore, Luca [1 ,2 ,3 ]
机构
[1] Sezionedi Astron, Dipartimento Fis, Via GB Tiepolo 11, I-34143 Trieste, Italy
[2] INAF Ist Nazl Astrofis, Osservatorio Astron Trieste, Via GB Tiepolo 11, I-34143 Trieste, Italy
[3] IFPU Inst Fundamental Phys Universe, Via Beirut 2, I-34100 Trieste, Italy
[4] INFN Ist Nazl Fis Nucleare, Via Valerio 2, I-34127 Trieste, Italy
关键词
large-scale structure of Universe; cosmology: theory; OBSERVABLES;
D O I
10.1093/mnras/stad1174
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present the merging of the Particle-Mesh (PM) relativistic gevolution code with the TreePM gadget-4 code, with the aim of studying general relativity effects in cosmology. Our code, called grgadget, is able to track the evolution of metric perturbations in the weak field limit by using gevolution's implementation of a relativistic PM in the Poisson gauge. To achieve this, starting from gevolution, we have written a c++ library called libgevolution, which allows a code to access and use the same abstractions and resources that gevolution uses for its PM-only N-body simulations. The code works under the assumption that particle interactions at short distances can be approximated as Newtonian, so that we can combine the forces computed with a Newtonian Tree with those computed with a relativistic PM. The result is a TreePM simulation code that represents metric perturbations at the scales where they are relevant while resolving non-linear structures. We validate our code by closely matching gadget-4 forces, computed with the Tree switched off, with those computed with libgevolution in the Newtonian limit. With grgadget, we obtain a matter power spectrum that is compatible with Newtonian gadget-4 at small scales and contains GR features at large scales that are consistent with results obtained with gevolution. We demonstrate that, due to the better resolution of the highly non-linear regime, the representation of the relativistic fields sampled on the mesh improves with respect to the PM-only simulations.
引用
下载
收藏
页码:5238 / 5253
页数:16
相关论文
共 50 条
  • [41] COSMOS:: A hybrid N-body/hydrodynamics code for cosmological problems
    Ricker, PM
    Dodelson, S
    Lamb, DQ
    ASTROPHYSICAL JOURNAL, 2000, 536 (01): : 122 - 143
  • [42] gevolution: a cosmological N-body code based on General Relativity
    Adamek, Julian
    Daverio, David
    Durrer, Ruth
    Kunz, Martin
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2016, (07):
  • [43] Initial conditions for cosmological N-body simulations of the scalar sector of theories of Newtonian, Relativistic and Modified Gravity
    Valkenburg, Wessel
    Hu, Bin
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2015, (09):
  • [44] A toy model to test the accuracy of cosmological N-body simulations
    Labini, F. Sylos
    ASTRONOMY & ASTROPHYSICS, 2013, 552
  • [45] Evolution of isolated overdensities as a control on cosmological N-body simulations
    Joyce, Michael
    Labini, Francesco Sylos
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2013, 429 (02) : 1088 - 1101
  • [46] The optimal gravitational softening length for cosmological N-body simulations
    Zhang, Tianchi
    Liao, Shihong
    Li, Ming
    Gao, Liang
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 487 (01) : 1227 - 1232
  • [47] Cosmological N-body simulations with generic hot dark matter
    Brandbyge, Jacob
    Hannestad, Steen
    JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS, 2017, (10):
  • [48] Stable clustering and the resolution of dissipationless cosmological N-body simulations
    Benhaiem, David
    Joyce, Michael
    Labini, Francesco Sylos
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2017, 470 (04) : 4099 - 4111
  • [49] Comments on the size of the simulation box in cosmological N-body simulations
    Bagla, JS
    Ray, S
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2005, 358 (03) : 1076 - 1082
  • [50] A method of generating initial conditions for cosmological N-body simulations
    Joyce, M
    Levesque, D
    Marcos, B
    PHYSICAL REVIEW D, 2005, 72 (10)