.png){kind=icon}
.png){kind=icon}
Return
Spectral function for 4He using the Chebyshev expansion in coupled-cluster theory
.png){kind=icon}
OA
AI
DOI：10.1103/PhysRevC.106.034310.png)
.png){kind=icon}
Original request for help.png){kind=icon}
Share.png){kind=icon}
Save
Abstract
En 中文
We compute spectral function for 4He by combining coupled-cluster theory with an expansion of integral transforms into Chebyshev polynomials. Our method allows us to estimate the uncertainty of spectral reconstruction. The properties of the Chebyshev polynomials make the procedure numerically stable and considerably lower in memory usage than the typically employed Lanczos algorithm. We benchmark our predictions with other calculations in the literature and with electron-scattering data in the quasi-elastic peak. The spectral function formalism allows one to extend ab initio lepton-nucleus cross sections into the relativistic regime. This makes it a promising tool for modeling this process at higher-energy transfers. The results we present open the door for studies of heavier nuclei, important for the neutrino oscillation programs.
Keywords:
SCATTERING
Journal
IF:
3.4
Papers:
2.9W
Citations:
5.7W