About Me

I am currently as a Full Professor at Astronomy Department, Beijing Normal University. I work on CMB physics, Large-scale Struture formation and astrophysical gravitational waves. In details, it covers Dark Energy/Modified Gravity, Weak Lensing, Strong Lensing, parameter estimation, non-gaussianity and higher-order statistics etc. I am memeber of the Euclid Consortium, AliCPT project, COrE Collaboration.

Contact Details

Dr. Prof. Bin Hu
Astronomy Department, Beijing Normal University
XinJieKou WaiDaJie, 19 100875 Beijing



MS + PhD

MS + PhD in Theoretical Physics / 2006 - 2011/ Advisor: Rong-Gen Cai

Institute of Theoretical Physics, Chinese Academy of Sciences


BS in Material Physics / 2002 - 2006

Shandong University



INSTITUTE OF COSMOS SCIENCES, University of Barcelona/ 2015 - 2016/
Adivsor: Licia Verde

Lorentz Institute for theoretical physics, Leiden University/ 2013 - 2015/
Adivsor: Ana Achucarro

Istituto Nazionale di Fisica Nucleare, Sezione di Padova / 2011 - 2013/
Adivsor: Sabino Matarrese/ Nicola Bartolo


Dark Energy/Modified Gravity On the linear regime of the density perturbation, we use the Effective Field Theory approach; on the mildly non-linear regime, we are interested in the extension of Lagrangian Perturbation Theory; on the extremely non-linear regime, we are interested in the N-body simulation algorithm and corresponding halo model.

Gravitational Lensing We are interested in CMB Lensing, galaxy Weak Lensing, Strong Lensing. In particular, delensing operation for the measurement of CMB B-mode polarization.

Gravitational Waves We are interested in several aspects of the astrophysical sources of the gravitational wave, such as gravity test in the strong field regime; Strong lensing; galaxy-black hole co-evolution; precision cosmology w. standard sires, etc.

Besides these, we are also interested in, Higher order statistics, Cosmic inflation mechanism, etc.


Master course ``Dark Energy: theory and observations''. You can find the materials HERE: lecture1, lecture2, lecture3, lecture4, lecture5, lecture6, lecture7.

Supplement materials: Visulaization of Cosmic density field (This document is done by Shu-Xun Tian, open with Adobe Reader to see the animation).

Bachelor course ``Electrodyanmics B''. You can find the materials HERE: lecture1.


Based on INSPIRE database, up to 2017/05, my publication record reaches: 30+ papers, and 1000+ citations.


EFTCAMB is a linear Einstein-Boltzmann solver for
Dark Energy/Modified Gravity models.
This package has been selected by the Planck and Euclid consortium as one of the main science case. You can follow the EFTCAMB developer version via github.

FalconIC is an initial conditions generator for the cosmology of arbitrary metric theories of gravity. The missing link between Boltzmann codes and N-body simulations. This code is developed by Wessel VALKENBURG and Bin HU.

CHAM is sCreened HAlo Model solver for the non-linear matter spectra for the altenative models to LCDM. This code is developed by Bin HU and Xue-Wen LIU.


Effective Field Theory with CAMB
Early Universe, Cosmology and Fundamental Physics, KITPC/Beijing, Sept.2015

Searching for primordial features from CMB and LSS surveys
Early Universe, Cosmology and Fundamental Physics, KITPC/Beijing, Sept.2015

Initial Condition of N-body simulation in Modified Gravity from EFT point of view
From Inflation to Galaxies: a workshop in honor of Sabino Matarrese, Castiglioncello, Sep.2015

EFTCAMB poster
Theoretical and Observational Progress on Large-scale Structure of the Universe, ESO, Garching, Jul.2015

Computation of CMB-LSS XC spectra in EFT Cosmologies-II
Euclid Consortium Meeting 2015, Lausanne, Jun.2015

EFTCAMB: Effective field theory for DE/MG
Theoretical cosmology Seminar, Padova, May.2015

Searching for the primordial features with CMB and LSS surveys