PIRSA:13110088

Video URL

https://pirsa.org/13110088

N-body lensed CMB maps: lensing extraction and characterization

Antolini, C. (2013). N-body lensed CMB maps: lensing extraction and characterization. Perimeter Institute for Theoretical Physics. https://pirsa.org/13110088

Antolini, Claudia. N-body lensed CMB maps: lensing extraction and characterization. Perimeter Institute for Theoretical Physics, Nov. 15, 2013, https://pirsa.org/13110088 

          @misc{ scivideos_PIRSA:13110088,
            doi = {10.48660/13110088},
            url = {https://pirsa.org/13110088},
            author = {Antolini, Claudia},
            keywords = {Cosmology},
            language = {en},
            title = {N-body lensed CMB maps: lensing extraction and characterization},
            publisher = {Perimeter Institute for Theoretical Physics},
            year = {2013},
            month = {nov},
            note = {PIRSA:13110088 see, \url{https://scivideos.org/pirsa/13110088}}
          }

Claudia Antolini SISSA International School for Advanced Studies

Talk numberPIRSA:13110088
DOI10.48660/13110088
Source RepositoryPIRSA
Collection
Talk Type Scientific Series
Subject

Abstract

After multiple high precision detections (ACT, SPT, Planck) gravitational lensing has become a new source of relevant cosmological information: combining it with other probes (e.g. the large scale structure) can give significant insight on the evolution of the Dark Energy component. Developing new algorithms of estimate of this signal will allow the community to exploit this observable as a new and independent probe in cosmology. In my talk I will present the reconstruction of the lensing shear pattern and its angular power spectrum from total intensity and polarised CMB maps obtained using Born approximated ray-tracing through N-body simulated structures.The recovered spectra are in agreement with predictions of the underlying ΛCDM with no visible bias, on a scale interval which extends from the arcminute to several degrees over the sky. This demonstrates the feasibility of CMB lensing studies based on large scale simulations of cosmological structure formation in the context of the upcoming large observational campaigns.