Bhatt, Jitesh R.Jitesh R.BhattNatwariya, Pravin KumarPravin KumarNatwariyaNayak, Alekha C.Alekha C.NayakPandey, Arun KumarArun KumarPandey2025-08-312025-08-312020-04-0110.1140/epjc/s10052-020-7886-x2-s2.0-85083656687http://repository.iitgn.ac.in/handle/IITG2025/24187We have shown that in presence of a cosmic magnetic field the bounds on baryon dark matter cross-section (σ^), dark-matter mass (m<inf>d</inf>) and values of the magnetic field (B) can strongly influence each other. This requires to rework the bounds on σ^, m<inf>d</inf> and B which can explain the observed absorption signal by EDGES collaboration. The upper limit on the magnetic field strength can modify in presence of baryon-dark matter interaction cross-section. In the presence of a strong magnetic field, a large baryon-dark matter interaction cross-section is required to balance magnetic heating of gas to explain the EDGES signal as compared to a weak magnetic field. Subsequently, the strong magnetic-fields can even erase the 21 cm signal–this gives an upper bound on the strength of magnetic-fields, dark-matter mass and baryon-dark matter cross-section. In the special case when σ^ = 0, one can recover the bound on magnetic field strength calculated in [1]. In this work we find that the allowed range of the primordial magnetic field can increase by three orders of magnitude in comparison with [1]. We get upper bound on the magnetic field strength: 3.48 × 10 ^{- 6} G for the dark matter mass ≲ 10 ^{- 2} GeV.trueArticlehttps://link.springer.com/content/pdf/10.1140/epjc/s10052-020-7886-x.pdf143460521 April 202016334arJournal16