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Physics, Volume 4, Issue 1 (March 2022) – 24 articles

Cover Story (view full-size image): The National Center for Oncological Hadrontherapy (CNAO) is one of the few centers in the world able to provide hadrontherapy, an extremely advanced form of radiotherapy, making use of protons and carbon ions to treat complex tumors. The beating heart of the CNAO is the synchrotron, where physics meets oncology. The first particle accelerator built in Italy, in collaboration with CERN and INFN for the treatment of oncological patients, it has an 80-meter circumference ring, where ions and protons are directed with submillimeter precision to treatment rooms towards tumor cells. Research at CNAO never stops accelerating scientific progress, the basis for the success of every innovation in medicine. CNAO is a scientific, clinical and human facility, continuously striving for new treatment horizons in the treatment of complex tumors. View this paper
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19 pages, 2333 KiB  
Review
Trends in the Structure of Nuclei near 100Sn
by Magdalena Górska
Physics 2022, 4(1), 364-382; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010024 - 21 Mar 2022
Cited by 5 | Viewed by 3328
Abstract
Inevitable progress has been achieved in recent years regarding the available data on the structure of 100Sn and neighboring nuclei. Updated nuclear structure data in the region is presented using selected examples. State-of-the-art experimental techniques involving stable and radioactive beam facilities have [...] Read more.
Inevitable progress has been achieved in recent years regarding the available data on the structure of 100Sn and neighboring nuclei. Updated nuclear structure data in the region is presented using selected examples. State-of-the-art experimental techniques involving stable and radioactive beam facilities have enabled access to those exotic nuclei. The analysis of experimental data has established the shell structure and its evolution towards N = Z = 50 of the number of neutrons, N, and the atomic number, Z, seniority conservation and proton–neutron interaction in the g9/2 orbit, the super-allowed Gamow–Teller decay of 100Sn, masses and half-lives along the rapid neutron-capture process (r-process) path and super-allowed α decay beyond 100Sn. The status of theoretical approaches in shell model and mean-field investigations are discussed and their predictive power assessed. The calculated systematics of high-spin states for N = 50 isotopes including the 5 state and N = Z nuclei in the g9/2 orbit is presented for the first time. Full article
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35 pages, 419 KiB  
Article
(2 + 1)-Maxwell Equations in Split Quaternions
by Merab Gogberashvili
Physics 2022, 4(1), 329-363; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010023 - 17 Mar 2022
Cited by 3 | Viewed by 1874
Abstract
The properties of spinors and vectors in (2 + 2) space of split quaternions are studied. Quaternionic representation of rotations naturally separates two SO(2,1) subgroups of the full group of symmetry of the norms of split quaternions, [...] Read more.
The properties of spinors and vectors in (2 + 2) space of split quaternions are studied. Quaternionic representation of rotations naturally separates two SO(2,1) subgroups of the full group of symmetry of the norms of split quaternions, SO(2,2). One of them represents symmetries of three-dimensional Minkowski space-time. Then, the second SO(2,1) subgroup, generated by the additional time-like coordinate from the basis of split quaternions, can be viewed as the internal symmetry of the model. It is shown that the analyticity condition, applying to the invariant construction of split quaternions, is equivalent to some system of differential equations for quaternionic spinors and vectors. Assuming that the derivatives by extra time-like coordinate generate triality (supersymmetric) rotations, the analyticity equation is reduced to the exact Dirac–Maxwell system in three-dimensional Minkowski space-time. Full article
(This article belongs to the Section Classical Physics)
14 pages, 437 KiB  
Article
Jet Transport Coefficient at the Large Hadron Collider Energies in a Color String Percolation Approach
by Aditya Nath Mishra, Dushmanta Sahu and Raghunath Sahoo
Physics 2022, 4(1), 315-328; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010022 - 16 Mar 2022
Cited by 5 | Viewed by 2037
Abstract
Within the color string percolation model (CSPM), jet transport coefficient, q^, is calculated for various multiplicity classes in proton-proton and centrality classes in nucleus-nucleus collisions at the Large Hadron Collider energies for a better understanding of the matter formed in ultra-relativistic [...] Read more.
Within the color string percolation model (CSPM), jet transport coefficient, q^, is calculated for various multiplicity classes in proton-proton and centrality classes in nucleus-nucleus collisions at the Large Hadron Collider energies for a better understanding of the matter formed in ultra-relativistic collisions. q^ is studied as a function of final state charged particle multiplicity (pseudorapidity density at midrapidity), initial state percolation temperature and energy density. The CSPM results are then compared with different theoretical calculations from the JET Collaboration those incorporate particle energy loss in the medium. Full article
(This article belongs to the Special Issue Jean Cleymans: A Life for Physics)
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14 pages, 3531 KiB  
Review
Numerical Relativity as a New Tool for Fundamental Cosmology
by Anna Ijjas
Physics 2022, 4(1), 301-314; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010021 - 04 Mar 2022
Cited by 4 | Viewed by 2370
Abstract
Advances in our understanding of the origin, evolution, and structure of the universe have long been driven by cosmological perturbation theory, model building, and effective field theory. In this review, numerical relativity is introduced as a powerful new complementary tool for fundamental cosmology. [...] Read more.
Advances in our understanding of the origin, evolution, and structure of the universe have long been driven by cosmological perturbation theory, model building, and effective field theory. In this review, numerical relativity is introduced as a powerful new complementary tool for fundamental cosmology. To illustrate its power, applications of numerical relativity are discussed to studying the robustness of slow contraction and inflation in homogenizing, isotropizing, and flattening the universe beginning from generic unsmooth initial conditions. In particular, it is described how recent numerical relativity studies of slow contraction have revealed a novel, non-linear smoothing mechanism based on ultralocality that challenges the conventional view on what is required to explain the large-scale homogeneity and isotropy of the observable universe. Full article
(This article belongs to the Section High Energy Physics)
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7 pages, 375 KiB  
Article
Color Transparency in p¯A Reactions
by Alexei B. Larionov
Physics 2022, 4(1), 294-300; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010020 - 25 Feb 2022
Viewed by 1888
Abstract
Exclusive channels of antiproton annihilation on the bound nucleon are sensitive to mesonic interactions with the target residue. If the hard scale is present, then such interactions should be reduced due to color transparency (CT). In this paper, the [...] Read more.
Exclusive channels of antiproton annihilation on the bound nucleon are sensitive to mesonic interactions with the target residue. If the hard scale is present, then such interactions should be reduced due to color transparency (CT). In this paper, the d(p¯,ππ0)p reaction is discussed at a large center-of-mass angle. Predictions for the future PANDA (antiProton ANnihilations at DArmstadt) experiment at FAIR (Facility for Antiproton and Ion Research, Darmstadt, Germany) are given for nuclear transparency ratios calculated within the generalized eikonal approximation and the quantum diffusion model of CT. Full article
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8 pages, 599 KiB  
Opinion
Distinctive Features of Charge Exchange Involving the Second Flavor of Hydrogen Atoms—The Candidates for Dark Matter
by Eugene Oks
Physics 2022, 4(1), 286-293; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010019 - 23 Feb 2022
Viewed by 1687
Abstract
The second flavor of hydrogen atoms (SFHA) refers to the kind of hydrogen atoms that have only the states of the zero orbital angular momentum (the S-states), both in the discrete and continuous spectra. They were first discovered theoretically in one of my [...] Read more.
The second flavor of hydrogen atoms (SFHA) refers to the kind of hydrogen atoms that have only the states of the zero orbital angular momentum (the S-states), both in the discrete and continuous spectra. They were first discovered theoretically in one of my earlier papers, where a proof of their existence was also provided by analyzing atomic experiments concerning the high-energy tail of the linear momentum distribution in the ground state of hydrogen atoms. From a theoretical point of view, the discovery was based on the standard Dirac equation for hydrogen atoms without changing the existing physical laws. Recently, the existence of the SFHA was seemingly also confirmed by two types of astrophysical observations: the allowance for the SFHA explained the puzzling results concerning both the anomalous absorption of the redshifted 21 cm spectral line from the early Universe, and the observations by the Dark Energy Survey (DES) team where it was found that the distribution of dark matter in the Universe is noticeably smoother than predictions employing Einstein’s relativity. In the present review, we exhibit results from two recent papers where attention was brought to a visible difference in the cross-sections of the resonant charge exchange for collisions of the SFHA with incoming protons, compared to collisions of the usual hydrogen atoms with incoming protons. It was shown that, after taking into account the SFHA, there is a better agreement with the corresponding experimental cross-section. Coupled with the previous evidence of the existence of the SFHA, deduced from the analysis of the other kind of atomic experiments, and evidenced by two different kinds of astrophysical observations, this strengthens the standing of the SFHA as the most probable candidate for all or a part of dark matter. Full article
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28 pages, 3498 KiB  
Review
Emerging Concepts in Nuclear Structure Based on the Shell Model
by Takaharu Otsuka
Physics 2022, 4(1), 258-285; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010018 - 22 Feb 2022
Cited by 8 | Viewed by 3677
Abstract
Some emerging concepts of nuclear structure are overviewed. (i) Background: the many-body quantum structure of atomic nucleus, a complex system comprising protons and neutrons (called nucleons collectively), has been studied largely based on the idea of the quantum liquid (à la Landau), where [...] Read more.
Some emerging concepts of nuclear structure are overviewed. (i) Background: the many-body quantum structure of atomic nucleus, a complex system comprising protons and neutrons (called nucleons collectively), has been studied largely based on the idea of the quantum liquid (à la Landau), where nucleons are quasiparticles moving in a (mean) potential well, with weak “residual” interactions between nucleons. The potential is rigid in general, although it can be anisotropic. While this view was a good starting point, it is time to look into kaleidoscopic aspects of the nuclear structure brought in by underlying dynamics and nuclear forces. (ii) Methods: exotic features as well as classical issues are investigated from fresh viewpoints based on the shell model and nucleon–nucleon interactions. The 70-year progress of the shell–model approach, including effective nucleon–nucleon interactions, enables us to do this. (iii) Results: we go beyond the picture of the solid potential well by activating the monopole interactions of the nuclear forces. This produces notable consequences in key features such as the shell/magic structure, the shape deformation, the dripline, etc. These consequences are understood with emerging concepts such as shell evolution (including type-II), T-plot, self-organization (for collective bands), triaxial-shape dominance, new dripline mechanism, etc. The resulting predictions and analyses agree with experiment. (iv) Conclusion: atomic nuclei are surprisingly richer objects than initially thought. Full article
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29 pages, 48229 KiB  
Review
Hadron Therapy Achievements and Challenges: The CNAO Experience
by Sandro Rossi
Physics 2022, 4(1), 229-257; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010017 - 22 Feb 2022
Cited by 7 | Viewed by 5778
Abstract
Protons and carbon ions (hadrons) have useful properties for the treatments of patients affected by oncological pathologies. They are more precise than conventional X-rays and possess radiobiological characteristics suited for treating radio-resistant or inoperable tumours. This paper gives an overview of the status [...] Read more.
Protons and carbon ions (hadrons) have useful properties for the treatments of patients affected by oncological pathologies. They are more precise than conventional X-rays and possess radiobiological characteristics suited for treating radio-resistant or inoperable tumours. This paper gives an overview of the status of hadron therapy around the world. It focusses on the Italian National Centre for Oncological Hadron therapy (CNAO), introducing operation procedures, system performance, expansion projects, methodologies and modelling to build individualized treatments. There is growing evidence that supports safety and effectiveness of hadron therapy for a variety of clinical situations. However, there is still a lack of high-level evidence directly comparing hadron therapy with modern conventional radiotherapy techniques. The results give an overview of pre-clinical and clinical research studies and of the treatments of 3700 patients performed at CNAO. The success and development of hadron therapy is strongly associated with the creation of networks among hadron therapy facilities, clinics, universities and research institutions. These networks guarantee the growth of cultural knowledge on hadron therapy, favour the efficient recruitment of patients and present available competences for R&D (Research and Development) programmes. Full article
(This article belongs to the Special Issue Selected Papers from Applied Nuclear Physics Conference 2021)
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12 pages, 278 KiB  
Article
Tachyon Behavior Due to Mass-State Transitions at Scattering Vertices
by John R. Fanchi
Physics 2022, 4(1), 217-228; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010016 - 18 Feb 2022
Cited by 5 | Viewed by 1805
Abstract
A particle beam-thin foil scattering model is updated within the context of parametrized relativistic quantum theory (pRQT). This paper focuses on the creation, annihilation, and detection of tachyons when a beam of particles scatters off a thin foil. Improved calculation procedures and recent [...] Read more.
A particle beam-thin foil scattering model is updated within the context of parametrized relativistic quantum theory (pRQT). This paper focuses on the creation, annihilation, and detection of tachyons when a beam of particles scatters off a thin foil. Improved calculation procedures and recent data are used to update model calculations for a pion-proton system. Full article
(This article belongs to the Section High Energy Physics)
15 pages, 2833 KiB  
Article
Free Convection of a Bingham Fluid in a Differentially-Heated Porous Cavity: The Effect of a Square Grid Microstructure
by D. Andrew S. Rees
Physics 2022, 4(1), 202-216; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010015 - 10 Feb 2022
Cited by 2 | Viewed by 1777
Abstract
We examine how a square-grid microstructure affects the manner in which a Bingham fluid is convected in a sidewall-heated rectangular porous cavity. When the porous microstructure is isotropic, flow arises only when the Darcy–Rayleigh number is higher than a critical value, and this [...] Read more.
We examine how a square-grid microstructure affects the manner in which a Bingham fluid is convected in a sidewall-heated rectangular porous cavity. When the porous microstructure is isotropic, flow arises only when the Darcy–Rayleigh number is higher than a critical value, and this corresponds to when buoyancy forces are sufficient to overcome the yield threshold of the Bingham fluid. In such cases, the flow domain consists of a flowing region and stagnant regions within which there is no flow. Here, we consider a special case where the constituent pores form a square grid pattern. First, we use a network model to write down the appropriate macroscopic momentum equations as a Darcy–Bingham law for this microstructure. Then detailed computations are used to determine strongly nonlinear states. It is found that the flow splits naturally into four different regions: (i) full flow, (ii) no-flow, (iii) flow solely in the horizontal direction and (iv) flow solely in the vertical direction. The variations in the rate of heat transfer and the strength of the flow with the three governing parameters, the Darcy–Rayleigh number, Ra, the Rees–Bingham number, Rb, and the aspect ratio, A, are obtained. Full article
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17 pages, 504 KiB  
Article
Probing Different Characteristics of Shell Evolution Driven by Central, Spin-Orbit, and Tensor Forces
by Yutaka Utsuno
Physics 2022, 4(1), 185-201; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010014 - 09 Feb 2022
Cited by 1 | Viewed by 2113
Abstract
In this paper, the validity of the shell-evolution picture is investigated on the basis of shell-model calculations for the atomic mass number 25A55 neutron-rich nuclei. For this purpose, the so-called SDPF-MU interaction is used. Its central, two-body spin–orbit, and [...] Read more.
In this paper, the validity of the shell-evolution picture is investigated on the basis of shell-model calculations for the atomic mass number 25A55 neutron-rich nuclei. For this purpose, the so-called SDPF-MU interaction is used. Its central, two-body spin–orbit, and tensor forces are taken from a simple Gaussian force, the M3Y (Michigan 3-range Yukawa) interaction, and a π+ρ meson exchange force, respectively. Carrying out almost a complete survey of the predicted effective single-particle energies, it is confirmed here that the present scheme is quite effective for describing shell evolution in exotic nuclei. Full article
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13 pages, 2545 KiB  
Review
Dose Limits and Countermeasures for Mitigating Radiation Risk in Moon and Mars Exploration
by Daria Boscolo and Marco Durante
Physics 2022, 4(1), 172-184; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010013 - 09 Feb 2022
Cited by 7 | Viewed by 3761
Abstract
After decades of research on low-Earth orbit, national space agencies and private entrepreneurs are investing in exploration of the Solar system. The main health risk for human space exploration is late toxicity caused by exposure to cosmic rays. On Earth, the exposure of [...] Read more.
After decades of research on low-Earth orbit, national space agencies and private entrepreneurs are investing in exploration of the Solar system. The main health risk for human space exploration is late toxicity caused by exposure to cosmic rays. On Earth, the exposure of radiation workers is regulated by dose limits and mitigated by shielding and reducing exposure times. For space travel, different international space agencies adopt different limits, recently modified as reviewed in this paper. Shielding and reduced transit time are currently the only practical solutions to maintain acceptable risks in deep space missions. Full article
(This article belongs to the Special Issue Selected Papers from Applied Nuclear Physics Conference 2021)
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12 pages, 353 KiB  
Article
The Birth of the Universe as a Result of the Change of the Metric Signature
by Tatyana P. Shestakova
Physics 2022, 4(1), 160-171; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010012 - 07 Feb 2022
Cited by 2 | Viewed by 2167
Abstract
In this paper, I discuss the idea that the birth of our Universe may be a result of a quantum transition from a physical continuum with the Euclidean signature to a Lorentzian spacetime. A similar idea was expressed by Andrei D. Sakharov At [...] Read more.
In this paper, I discuss the idea that the birth of our Universe may be a result of a quantum transition from a physical continuum with the Euclidean signature to a Lorentzian spacetime. A similar idea was expressed by Andrei D. Sakharov At the classical level, the idea was studied by George F. R. Ellis and his collaborators, who explored if solutions to the classical Einstein equation exist which admit a change of metric signature. The present paper aims at examining possible realizations of this idea at the level of quantum gravity, in the framework of the Wheeler–DeWitt theory and in the extended phase space approach to quantization of gravity. I intend to answer the questions: to answer the questions: Does the Hartle–Hawking wave function imply such a realization? How can this idea be realized in the extended phase space approach to quantum gravity, where the change of signature is described by imposing special conditions on g00-component of the metric in different regions of the physical continuum? The conclusion is that the idea can be realized from a formal mathematical point of view, but it can hardly help in understanding how spacetime structure and time itself appeared from a timeless continuum. Full article
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28 pages, 665 KiB  
Review
A Review on Scene Prediction for Automated Driving
by Anne Stockem Novo, Martin Krüger, Marco Stolpe and Torsten Bertram
Physics 2022, 4(1), 132-159; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010011 - 01 Feb 2022
Cited by 3 | Viewed by 4010
Abstract
Towards the aim of mastering level 5, a fully automated vehicle needs to be equipped with sensors for a 360 surround perception of the environment. In addition to this, it is required to anticipate plausible evolutions of the traffic scene such that [...] Read more.
Towards the aim of mastering level 5, a fully automated vehicle needs to be equipped with sensors for a 360 surround perception of the environment. In addition to this, it is required to anticipate plausible evolutions of the traffic scene such that it is possible to act in time, not just to react in case of emergencies. This way, a safe and smooth driving experience can be guaranteed. The complex spatio-temporal dependencies and high dynamics are some of the biggest challenges for scene prediction. The subtile indications of other drivers’ intentions, which are often intuitively clear to the human driver, require data-driven models such as deep learning techniques. When dealing with uncertainties and making decisions based on noisy or sparse data, deep learning models also show a very robust performance. In this survey, a detailed overview of scene prediction models is presented with a historical approach. A quantitative comparison of the model results reveals the dominance of deep learning methods in current state-of-the-art research in this area, leading to a competition on the cm scale. Moreover, it also shows the problem of inter-model comparison, as many publications do not use standardized test sets. However, it is questionable if such improvements on the cm scale are actually necessary. More effort should be spent in trying to understand varying model performances, identifying if the difference is in the datasets (many simple situations versus many corner cases) or actually an issue of the model itself. Full article
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8 pages, 261 KiB  
Review
Modeling Turbulence in Permeable Media: The Double-Decomposition Concept Revisited
by Marcelo J. S. de Lemos
Physics 2022, 4(1), 124-131; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010010 - 27 Jan 2022
Cited by 2 | Viewed by 1864
Abstract
In this article, a concept named double decomposition, which is used to model turbulent flows in porous media, is examined. This concept is based on the idea that in a turbulent flow through a porous matrix, local instantaneous variables can be averaged in [...] Read more.
In this article, a concept named double decomposition, which is used to model turbulent flows in porous media, is examined. This concept is based on the idea that in a turbulent flow through a porous matrix, local instantaneous variables can be averaged in time and space, simultaneously. Depending on how these operators are applied, averaged equations take different forms. In this article, instantaneous local equations are averaged using both operators and a different set of equations resulting from such operations are commented upon. Additional terms proposed for the averaged equations are discussed. Full article
20 pages, 2712 KiB  
Article
Quantum Cryptography—A Simplified Undergraduate Experiment and Simulation
by Yuval Bloom, Ilai Fields, Alona Maslennikov and Georgi Gary Rozenman
Physics 2022, 4(1), 104-123; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010009 - 25 Jan 2022
Cited by 15 | Viewed by 4954
Abstract
Quantum cryptography is a topic of considerable interest. A simple and robust experiment and theory for a senior level undergraduate investigation of quantum key distribution are described. In the proposed experiment, key principles from the BB84 protocol, used in quantum cryptography, are emulated [...] Read more.
Quantum cryptography is a topic of considerable interest. A simple and robust experiment and theory for a senior level undergraduate investigation of quantum key distribution are described. In the proposed experiment, key principles from the BB84 protocol, used in quantum cryptography, are emulated using an optical apparatus and computational scripts independently. Full article
(This article belongs to the Section Physics Education)
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24 pages, 908 KiB  
Article
Determining Pitch-Angle Diffusion Coefficients for Electrons in Whistler Turbulence
by Felix Spanier, Cedric Schreiner and Reinhard Schlickeiser
Physics 2022, 4(1), 80-103; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010008 - 20 Jan 2022
Viewed by 2288
Abstract
Transport of energetic electrons in the heliosphere is governed by resonant interaction with plasma waves, for electrons with sub-GeV kinetic energies specifically with dispersive modes in the whistler regime. In this paper, particle-in-cell simulations of kinetic turbulence with test-particle electrons are performed. The [...] Read more.
Transport of energetic electrons in the heliosphere is governed by resonant interaction with plasma waves, for electrons with sub-GeV kinetic energies specifically with dispersive modes in the whistler regime. In this paper, particle-in-cell simulations of kinetic turbulence with test-particle electrons are performed. The pitch-angle diffusion coefficients of these test particles are analyzed and compared to an analytical model for left-handed and right-handed polarized wave modes. Full article
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12 pages, 5940 KiB  
Article
Dissipative Ion-Acoustic Solitary Waves in Magnetized κ-Distributed Non-Maxwellian Plasmas
by Sharmin Sultana and Ioannis Kourakis
Physics 2022, 4(1), 68-79; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010007 - 20 Jan 2022
Cited by 5 | Viewed by 2545
Abstract
The propagation of dissipative electrostatic (ion-acoustic) solitary waves in a magnetized plasma with trapped electrons is considered via the Schamel formalism. The direction of propagation is assumed to be arbitrary, i.e., oblique with respect to the magnetic field, for generality. A non-Maxwellian (nonthermal) [...] Read more.
The propagation of dissipative electrostatic (ion-acoustic) solitary waves in a magnetized plasma with trapped electrons is considered via the Schamel formalism. The direction of propagation is assumed to be arbitrary, i.e., oblique with respect to the magnetic field, for generality. A non-Maxwellian (nonthermal) two-component plasma is considered, consisting of an inertial ion fluid, assumed to be cold for simplicity, and electrons. A (kappa) κ-type distribution is adopted for the electron population, in addition to particle trapping taken into account in phase space. A damped version of the Schamel-type equation is derived for the electrostatic potential, and its analytical solution, representing a damped solitary wave, is used to examine the nonlinear features of dissipative ion-acoustic solitary waves in the presence of trapped electrons. The influence of relevant plasma configuration parameters, namely the percentage of trapped electrons, the electron superthermality (spectral) index, and the direction of propagation on the solitary wave characteristics is investigated. Full article
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2 pages, 155 KiB  
Editorial
Acknowledgment to Reviewers of Physics in 2021
by Physics Editorial Office
Physics 2022, 4(1), 66-67; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010006 - 19 Jan 2022
Viewed by 1555
Abstract
Rigorous peer-reviews are the basis of high-quality academic publishing [...] Full article
15 pages, 2538 KiB  
Article
The Influence of Bounding Plates on Species Separation in a Vertical Thermogravitational Column
by Abdelkader Mojtabi, Pierre Costeseque, Bafétigué Ouattara, Marie-Catherine Charrier-Mojtabi and D. Andrew S. Rees
Physics 2022, 4(1), 51-65; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010005 - 18 Jan 2022
Viewed by 2072
Abstract
In this paper, an analytical and numerical analysis of the species separation in a binary mixture is performed. The main objective is to study the influence of the thickness and the nature of the bounding plates of the thermogravitational column (TGC) on species [...] Read more.
In this paper, an analytical and numerical analysis of the species separation in a binary mixture is performed. The main objective is to study the influence of the thickness and the nature of the bounding plates of the thermogravitational column (TGC) on species separation. The theory of Furry, Jones and Onsager is extended to the cases where bounding conducting walls enclose the TGC. The governing 2-dimensional equations are solved numerically using COMSOL Multiphysics software. A good agreement is found between the analytical and the numerical results. It is shown that the determination of the thermal diffusion coefficient, DT, from the measurement of the vertical mass fraction gradient of binary solutions, does not depend on the temperature difference imposed on the vertical column either on the outer walls of the cavity or on the inner walls in contact with the binary solutions. However, it is found that this result is no longer valid in the case of a binary gas. To our knowledge, in all earlier studies, dealing with the measurement of Soret coefficients in binary fluids, the nature and the thickness of the bounding walls were not considered. Full article
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14 pages, 3970 KiB  
Review
Application of Ion Beam Analysis in Studies of First Wall Materials in Controlled Fusion Devices
by Marek Rubel, Anna Widdowson, Laura Dittrich, Sunwoo Moon, Armin Weckmann and Per Petersson
Physics 2022, 4(1), 37-50; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010004 - 17 Jan 2022
Viewed by 2365
Abstract
The paper provides a concise overview of ion beam analysis methods and procedures in studies of materials exposed to fusion plasmas in controlled fusion devices with magnetic confinement. An impact of erosion–deposition processes on the morphology of wall materials is presented. In particular, [...] Read more.
The paper provides a concise overview of ion beam analysis methods and procedures in studies of materials exposed to fusion plasmas in controlled fusion devices with magnetic confinement. An impact of erosion–deposition processes on the morphology of wall materials is presented. In particular, results for deuterium analyses are discussed. Underlying physics, advantages and limitations of methods are addressed. The role of wall diagnostics in studies of material migration and fuel retention is explained. A brief note on research and handling of radioactive and beryllium-contaminated materials is also given. Full article
(This article belongs to the Special Issue Selected Papers from Applied Nuclear Physics Conference 2021)
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16 pages, 4548 KiB  
Article
Magnetic Force-Free Theory: Nonlinear Case
by Brunello Tirozzi and Paolo Buratti
Physics 2022, 4(1), 21-36; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010003 - 10 Jan 2022
Viewed by 1999
Abstract
In this paper, a theory of force-free magnetic field useful for explaining the formation of convex closed sets, bounded by a magnetic separatrix in the plasma, is developed. This question is not new and has been addressed by many authors. Force-free magnetic fields [...] Read more.
In this paper, a theory of force-free magnetic field useful for explaining the formation of convex closed sets, bounded by a magnetic separatrix in the plasma, is developed. This question is not new and has been addressed by many authors. Force-free magnetic fields appear in many laboratory and astrophysical plasmas. These fields are defined by the solution of the problem ×B=ΛB with some field conditions BΩ on the boundary Ω of the plasma region. In many physical situations, it has been noticed that Λ is not constant but may vary in the domain Ω giving rise to many different interesting physical situations. We set Λ=Λ(ψ) with ψ being the poloidal magnetic flux function. Then, an analytic method, based on a first-order expansion of ψ with respect to a small parameter α, is developed. The Grad–Shafranov equation for ψ is solved by expanding the solution in the eigenfunctions of the zero-order operator. An analytic expression for the solution is obtained deriving results on the transition through resonances, the amplification with respect to the gun inflow. Thus, the formation of spheromaks or protosphera structure of the plasma is determined in the case of nonconstant Λ. Full article
(This article belongs to the Section Statistical Physics and Nonlinear Phenomena)
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9 pages, 279 KiB  
Article
Path Integral Estimates of the Quantum Fluctuations of the Relative Soliton-Soliton Velocity in a Gross-Pitaevskii Breather
by Sumita Datta, Vanja Dunjko and Maxim Olshanii
Physics 2022, 4(1), 12-20; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010002 - 10 Jan 2022
Cited by 3 | Viewed by 2086
Abstract
In this paper, the quantum fluctuations of the relative velocity of constituent solitons in a Gross-Pitaevskii breather are studied. The breather is confined in a weak harmonic trap. These fluctuations are monitored, indirectly, using a two-body correlation function measured at a quarter of [...] Read more.
In this paper, the quantum fluctuations of the relative velocity of constituent solitons in a Gross-Pitaevskii breather are studied. The breather is confined in a weak harmonic trap. These fluctuations are monitored, indirectly, using a two-body correlation function measured at a quarter of the harmonic period after the breather creation. The results of an ab initio quantum Monte Carlo calculation, based on the Feynman-Kac path integration method, are compared with the analytical predictions using the recently suggested approach within the Bogoliubov approximation, and a good agreement is obtained. Full article
(This article belongs to the Section Statistical Physics and Nonlinear Phenomena)
11 pages, 1048 KiB  
Article
GERARD: GEneral RApid Resolution of Digital Mazes Using a Memristor Emulator
by Pablo Dopazo, Carola de Benito, Oscar Camps, Stavros G. Stavrinides and Rodrigo Picos
Physics 2022, 4(1), 1-11; https://0-doi-org.brum.beds.ac.uk/10.3390/physics4010001 - 30 Dec 2021
Viewed by 2074
Abstract
Memristive technology is a promising game-changer in computers and electronics. In this paper, a system exploring the optimal paths through a maze, utilizing a memristor-based setup, is developed and concreted on a FPGA (field-programmable gate array) device. As a memristor, a digital emulator [...] Read more.
Memristive technology is a promising game-changer in computers and electronics. In this paper, a system exploring the optimal paths through a maze, utilizing a memristor-based setup, is developed and concreted on a FPGA (field-programmable gate array) device. As a memristor, a digital emulator has been used. According to the proposed approach, the memristor is used as a delay element, further configuring the test graph as a memristor network. A parallel algorithm is then applied, successfully reducing computing time and increasing the system’s efficiency. The proposed system is simple, easy to scale up and capable of implementing different graph configurations. The operation of the algorithm in the MATLAB (matrix laboratory) programming enviroment is checked beforehand and then exported to two different Intel FPGAs: a DE0-Nano board and an Arria 10 GX 220 FPGA. In both cases, reliable results are obtained quickly and conveniently, even for the case of a 300 × 300 nodes maze. Full article
(This article belongs to the Section Applied Physics)
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