27 citations · 48 across the 5 of their papers we have counts for
12 papers
A Brief Introduction to the Adomian Decomposition Method, with Applications in Astronomy and Astrophysics
Man Kwong Mak, Chun Sing Leung, Tiberiu Harko
The Adomian Decomposition Method (ADM) is a very effective approach for solving broad classes of nonlinear partial and ordinary differential equations, with important applications…
Analysing the radio flux density profile of the M31 galaxy: a possible dark matter interpretation
Man Ho Chan, Chu Fai Yeung, Lang Cui +1
Some recent studies have examined the gamma-ray flux profile of our Galaxy to determine the signal of dark matter annihilation. However, the results are controversial and no confir…
The effects of the dark energy on the static Schrödinger-Newton system -- an Adomian Decomposition Method and Padé approximants based approach
Man Kwong Mak, Chun Sing Leung, Tiberiu Harko
The Schrödinger-Newton system is a nonlinear system obtained by coupling together the linear Schrödinger equation of quantum mechanics with the Poisson equation of Newtonian mechan…
Constraining annihilating dark matter mass by the radio continuum spectral data of a high-redshift galaxy cluster
Man Ho Chan, Chak Man Lee, C. -Y. Ng +1
In the past decade, the properties of annihilating dark matter models were examined by various kinds of data, including the data of gamma rays, radio waves, X-ray, positrons, elect…
Vortex solutions in atomic Bose-Einstein condensates via the Adomian Decomposition Method
Tiberiu Harko, Man Kwong Mak, Chun Sing Leung
We study the dynamics of vortices with arbitrary topological charges in weakly interacting Bose-Einstein condensates using the Adomian Decomposition Method to solve the nonlinear G…
Ruling out GeV thermal relic annihilating dark matter by radio observation of the Andromeda galaxy
Man Ho Chan, Lang Cui, Jun Liu +1
In the past few years, some studies claimed that annihilating dark matter with mass GeV can explain the GeV gamma-ray excess in our Galaxy. However, recent analyses o…