Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp <p>The <strong>Journal of Atomic, Molecular, Condensed Matter and Nano Physics (JAMCNP)</strong> (ISSN 2582-8215) is an international journal being published since 2014. The main aim of this journal is to make available the most complete and reliable source of information on current developments, especially in the following fields (but are not limited to): <strong><em>Atomic Physics, Molecular Physics, Chemical Physics, Optical Physics, Condensed Matter, Nano Science including Nano-Photonics, Applied Physics</em> (<em>Environmental physics, Engineering physics, Biomedical physics, Astrophysics physics, Chemical physics, Computational physics, Quantum computing</em>)</strong>. </p> <p><strong>The Journal of Atomic, Molecular, Condensed Matter and Nano Physics<em> </em>is indexed in CAS Source Index (CASSI) of the American Chemical Society</strong></p> <p><img src="https://www.rgnpublications.com/journals/public/site/images/ganesh/cas.png" alt="" width="800" height="94" /></p> <p>To ensure speedy publication, only articles that are sufficiently well presented, contain significant results, and not required major revisions will be considered. <strong>Papers are accepted only after peer review</strong>.</p> <div> <p>Editorial decisions on the acceptance or otherwise are taken normally within 4 to 8 weeks (two months) of receipt of the paper.</p> <p><strong>Journal History:</strong> Formerly, <strong>Journal of Atomic, Molecular, Condensate and Nano Physics</strong> (eISSN 2349-2716; pISSN 2349-6088)</p> </div> en-US Authors who publish with this journal agree to the following terms:<br /><ul><li>Authors retain copyright and grant the journal right of first publication with the work simultaneously licensed under a CCAL that allows others to share the work with an acknowledgement of the work's authorship and initial publication in this journal.</li><li>Authors are able to enter into separate, additional contractual arrangements for the non-exclusive distribution of the journal's published version of the work (e.g., post it to an institutional repository or publish it in a book), with an acknowledgement of its initial publication in this journal.</li><li>Authors are permitted and encouraged to post their work online (e.g., in institutional repositories or on their website) prior to and during the submission process, as it can lead to productive exchanges, as well as earlier and greater citation of published work.</li></ul> manmohan@rgnpublications.com (Prof. (Dr.) Man Mohan) editorial@rgnpublications.com (The Head, Editorial Section) Sun, 26 Oct 2025 00:00:00 +0000 OJS 3.3.0.8 http://blogs.law.harvard.edu/tech/rss 60 Ionization of the \(1S\) and \(nS\) States of the Atomic Hydrogen by Positron and Electron Impacts https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3436 <p>The ionizations of the \(1S\) and \(nS\) states of the atomic hydrogen have been carried out using the hybrid theory, which is variationally correct and has been obtained by modifying the method of polarized orbitals. Earlier, we calculated cross sections of exciting the higher states from the ground state, and cross sections of photoabsorption. Now, we apply the same approach to the ionization of states. The distortion of the orbit is considered due to the incident positron or electron. The distortion takes place whether the incident particle is outside or inside the orbit. Temkin considered distortion of the target electron only when the incident particle is outside the orbit of the target. However, there is no simple way to consider distortion of \(nS\) states of atomic hydrogen. The cross sections are calculated by considering the distortion in the initial state as well as in the final state only in the \(1S\) state and are compared with the previous calculations and the experimental results. The present cross sections have a maximum at an energy which is the same as the incident energy in the experimental results.</p> A. K. Bhatia Copyright (c) 2025 Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3436 Sun, 26 Oct 2025 00:00:00 +0000 Variational Principles and Their Applications https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3018 <p><span class="fontstyle0">There are many variational calculations of energies of various systems which have </span><span class="fontstyle0">applications in Rydberg states and polarizabilities of these systems. There are variational calculations </span><span class="fontstyle0">of scattering functions which have applications in calculations of excitation, photoabsorption, and </span><span class="fontstyle0">radiative attachment cross sections. A few of these applications are mentioned.</span> <br /><br /></p> A. K. Bhatia Copyright (c) 2025 Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3018 Sun, 26 Oct 2025 00:00:00 +0000 New \(Q\)-\(\beta\)-Decay Theory Applied to the Calculations of the Rest Mass Energy \(m_0c^2\) of the Electron and of the \(Q\)-Value for \(\beta^+\)-Decay Transitions in Mirrors Nuclei \(A = 2Z - 1\) https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3173 <p>A new nuclear approach named \(Q\)-\(\beta\)-decay theory \((Q\beta T)\) is presented. This method is applied to express theoretically the \(\beta^+\)-\(Q\)-value for mirrors nuclei \(A = 2Z-1\). An important parameter named nuclear charge distribution coefficient (NCDC) noted \(\alpha (Z)\) is presented. In the framework of the liquid drop nuclear model where the nuclear charge is uniformly distributed in the nuclear volume, \(\alpha (Z) = 3/5\). It this work, it is demonstrated that the protons are not rigorously uniformly distributed within the nucleus. A slight correction is obtained with \(\alpha (Z) \approx \alpha_0 = 3/5 + 0.0557\). For \({}^{37}\)K and \({}^{65}\)As, we find for the electron rest mass energy \(m_0c^2=0.510\) 996 MeV agreeing excellently with the recommended value 0.510 998 950 MeV (CODATA, 2022). In addition, the \(Q\)-value calculated for \(A\) ranging between 11 and 99 agree very well with the recent Atomic Mass Evaluation -- AME2020 (Wang et al. [15]). New accurate $Q$-values are tabulated for nuclei mirrors with \(A\) ranging between 101 and 199. The present \(Q\)-\(\beta\)-DT make it possible to understand many nuclear properties and phenomena depending on the \(Q\)-value such as comparison between experimental and theoretical predictions of atomic masses, the understanding of the weak force and of the competitive processes between electron capture and \(\beta^+\)-decay.</p> I. Sakho Copyright (c) 2025 Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3173 Sun, 26 Oct 2025 00:00:00 +0000 Dilaton Detection in Radio Regions https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3490 <p>Structure formation is a very important phenomena to follow the cosmological evolution of our universe. The role of ultra-light dark matter in this whole process is substantial.\ Keeping this point in view, one anticipates that the extremely light dilatons can be expected play it's part in this crucial process.\ The detection of the light dilatons is however not very easy, their cosmological signal may be detected in large radio telescopes.\ Using radiometer equation we ealborate on the possibility of detecting dilaton signal coming from the dark matter halo of nearby galaxies.\ Our analysis shows that in some parameter range the possibility of their detection is non-negligible.</p> Ankur Chaubey, Avijit K. Ganguly Copyright (c) 2025 https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3490 Sun, 26 Oct 2025 00:00:00 +0000 4F and 5F Excitations of Atomic Hydrogen by Electron Impact https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3137 <p><span class="fontstyle0">The excitation cross-sections of the 4F and 5F states of atomic hydrogen by electron </span><span class="fontstyle0">impact have been calculated at incident energies 1.00 to 42.25 Ry, using the hybrid theory, which </span><span class="fontstyle0">is variationally correct. The present calculation is a single-channel or a distorted wave calculation. </span><span class="fontstyle0">Partial waves ranged from \(</span><span class="fontstyle2">L</span><span class="fontstyle3">=</span><span class="fontstyle0">3\) to 14 to obtain converged results. Excitations of higher states are </span><span class="fontstyle0">needed for diagnostics of the solar and astrophysical plasmas. They are also needed to model plasma </span><span class="fontstyle0">in fusion research, because they indicate the possibility that a state will be excited to a higher state </span><span class="fontstyle0">when colliding with another state. Transition rates to the lower states can be measured by observing </span><span class="fontstyle0">decays of the excited states.</span></p> A. K. Bhatia Copyright (c) 2025 Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3137 Sun, 26 Oct 2025 00:00:00 +0000 Excitation of \((1s2s)\) \(^{1}S\), the Singlet State of Helium Atoms by Positron Impact https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3180 <p>The excitation of the \((1s2s)\) \({}^{1}S\) state of a helium atom has been calculated using scattering functions obtained by the method of polarized orbitals. In this method, the distortion of each orbital is considered due to the presence of the incident particle. The distortion takes place only when the incident particle is outside the target orbital. This method has been widely used in the scattering of electrons and positrons from various targets. Plane-wave normalization of the continuum function is considered, while it has been neglected in calculations carried out by Mandal <em>et al</em>. [1], and Willis and McDowell [3]. Consequently, the present results are higher than those obtained by them.</p> A. K. Bhatia Copyright (c) 2025 Journal of Atomic, Molecular, Condensed Matter and Nano Physics https://www.rgnpublications.com/journals/index.php/jamcnp/article/view/3180 Sun, 26 Oct 2025 00:00:00 +0000