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1. SÍGAME Simulations of the $$[{\rm{C}}\,{\rm{II}}]$$, $$[{\rm{O}}\,{\rm{I}}]$$, and $$[{\rm{O}}\,{\rm{III}}]$$ Line Emission from Star-forming Galaxies at $$z\simeq 6$$

   https://doi.org/10.3847/1538-4357/aa86b4  

   Olsen, Karen; Greve, Thomas R.; Narayanan, Desika; Thompson, Robert; Davé, Romeel; Rios, Luis Niebla; Stawinski, Stephanie (September 2017, The Astrophysical Journal)
2. Study of the doubly charmed tetraquark $${{{{{{\rm{T}}}}}}}_{{{{{{\rm{c}}}}}}{{{{{\rm{c}}}}}}}^{+}$$

   https://doi.org/10.1038/s41467-022-30206-w  

   Aaij, R.; Abdelmotteleb, A. S.; Beteta, C. Abellán; Gallego, F. J.; Ackernley, T.; Adeva, B.; Adinolfi, M.; Afsharnia, H.; Agapopoulou, C.; Aidala, C. A.; et al (December 2022, Nature Communications)

   Abstract Quantum chromodynamics, the theory of the strong force, describes interactions of coloured quarks and gluons and the formation of hadronic matter. Conventional hadronic matter consists of baryons and mesons made of three quarks and quark-antiquark pairs, respectively. Particles with an alternative quark content are known as exotic states. Here a study is reported of an exotic narrow state in the D 0 D 0 π + mass spectrum just below the D *+ D 0 mass threshold produced in proton-proton collisions collected with the LHCb detector at the Large Hadron Collider. The state is consistent with the ground isoscalar $${{{{{{\rm{T}}}}}}}_{{{{{{\rm{c}}}}}}{{{{{\rm{c}}}}}}}^{+}$$ T c c + tetraquark with a quark content of $${{{{{\rm{c}}}}}}{{{{{\rm{c}}}}}}\overline{{{{{{\rm{u}}}}}}}\overline{{{{{{\rm{d}}}}}}}$$ c c u ¯ d ¯ and spin-parity quantum numbers J P  = 1 + . Study of the DD mass spectra disfavours interpretation of the resonance as the isovector state. The decay structure via intermediate off-shell D *+ mesons is consistent with the observed D 0 π + mass distribution. To analyse the mass of the resonance and its coupling to the D * D system, a dedicated model is developed under the assumption of an isoscalar axial-vector $${{{{{{\rm{T}}}}}}}_{{{{{{\rm{c}}}}}}{{{{{\rm{c}}}}}}}^{+}$$ T c c + state decaying to the D * D channel. Using this model, resonance parameters including the pole position, scattering length, effective range and compositeness are determined to reveal important information about the nature of the $${{{{{{\rm{T}}}}}}}_{{{{{{\rm{c}}}}}}{{{{{\rm{c}}}}}}}^{+}$$ T c c + state. In addition, an unexpected dependence of the production rate on track multiplicity is observed. 

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3. Kinematic Links and the Coevolution of MHD Winds, Jets, and Inner Disks from a High-resolution Optical [$${\rm{O}}\,{\rm{I}}$$] Survey

   https://doi.org/10.3847/1538-4357/aaf1aa  

   Banzatti, Andrea; Pascucci, Ilaria; Edwards, Suzan; Fang, Min; Gorti, Uma; Flock, Mario (January 2019, The Astrophysical Journal)
4. The Elbert range of magnetostrophic convection. II. Comparing linear theory to nonlinear low- Rm simulations

   https://doi.org/10.1098/rspa.2024.0016  

   Horn, Susanne; Aurnou, Jonathan M (March 2025, Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences)

   The magnetostrophic dynamo hypothesis has greatly influenced planetary dynamo research. Many magnetostrophic dynamo theories are founded upon the linear stability analysis by Chandrasekhar and Elbert, and by the canonical laboratory photographs taken by Nakagawa that show a significant enlargement of the convective flow scales in the magnetostrophic regime of liquid metal rotating magnetoconvection (RMC). We test whether these linear predictions are relevant for the nonlinear RMC system by exploring the five possible regimes using direct numerical simulations of RMC in the low magnetic Reynolds number quasi-static approximation. We map out the heat and momentum transport in these regimes, look at the flow structures and focus especially on the length scales. We have also included numerical counterparts of Nakagawa’s experiments and our results show an excellent agreement with three of these cases and linear theory. However, agreement with Nakagawa is not found in the magnetostrophic case: no enlargement of scales is observed, but still in good agreement with linear theory. Oscillatory bulk modes dominate all the RMC cases in which they exist, thus, suggesting that oscillatory convective flows may dominate all the other convective modes in planetary cores and may provide the motions that primarily generate planetary dynamo action. 

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5. Blackbody radiation shift for the $${}^{1}{{\rm{S}}}_{0}{-}^{3}{{\rm{P}}}_{0}$$ optical clock transition in zinc and cadmium atoms

   https://doi.org/10.1088/1361-6455/ab4434  

   Dzuba, Vladimir A; Derevianko, Andrei (November 2019, Journal of Physics B: Atomic, Molecular and Optical Physics)