4.5 Article

Open-charm mesons in nuclear matter at finite temperature beyond the zero-range approximation

期刊

PHYSICAL REVIEW C
卷 84, 期 1, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevC.84.015208

关键词

-

资金

  1. EU [MRTN-CT-2006-035482]
  2. MIC (Spain) [FIS2008-01661]
  3. Generalitat de Catalunya [2009SGR-1289]
  4. FEDER/FCT (Portugal) [PTDC/FIS/113292/2009, CERN/FP/116366/2010]
  5. European Community [227431]
  6. University of Groningen (the Netherlands)
  7. Helmholtz International Center for FAIR within the State of Hesse (Germany)
  8. Fundação para a Ciência e a Tecnologia [CERN/FP/116366/2010] Funding Source: FCT

向作者/读者索取更多资源

The properties of open charm mesons, D, <(D)over bar, D-s, and <(D)over bar>(s) in nuclear matter at finite temperature are studied within a self-consistent coupled-channel approach. The interaction of the low-lying pseudoscalar mesons with the ground-state baryons in the charm sector is derived from a t-channel vector-exchange model. The in-medium scattering amplitudes are obtained by solving the Lippmann-Schwinger equation at finite temperature including Pauli blocking effects, baryon dressing, as well as D, (D) over bar, D-s, and (D) over bar (s) self-energies taking their mutual influence into account. We find that the in-medium properties of the D meson are affected by the D-s-meson self-energy through the intermediate DsY loops coupled to DN states. Similarly, dressing the (D) over bar meson in the (D) over barY loops has an influence over the properties of the (D) over bar (s) meson.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.5
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

Article Geochemistry & Geophysics

Toward a Practical Appraisal for Waveform Tomography of Band- and Offset-Limited Marine Seismic Data

Claudia Gras, Clara Estela Jimenez-Tejero, Valenti Sallares, Adria Melendez, Cesar R. Ranero

Summary: The study introduces a generalized workflow for retrieving high-resolution P-wave velocity models of complex Earth's subsurface structures from traditional marine near-vertical seismic reflection experiments. By combining downward continuation, travel-time tomography, and full-waveform inversion, the workflow overcomes nonlinearity issues and accurately predicts the quality of the results. Testing with challenging synthetic target models shows that the workflow is efficient in obtaining high-resolution velocity models using limited field datasets.

IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING (2022)

Article Geochemistry & Geophysics

Downward continuation of marine seismic reflection data: an undervalued tool to improve velocity models

C. E. Jimenez-Tejero, Cesar R. Ranero, Valenti Sallares, Claudia Gras

Summary: The purpose of marine seismic experiments is to provide information about the structure and physical properties of the subsurface. This study presents a user-friendly open source software for redatuming 2-D streamer field data to the sea bottom, and provides assessment tools to evaluate data quality. The results show that the conducted experiments can improve the imaging of deep structures and retrieve velocity models through traveltime and full waveform inversion.

GEOPHYSICAL JOURNAL INTERNATIONAL (2022)

Article Astronomy & Astrophysics

Equation of state for hot hyperonic neutron star matter

Hristijan Kochankovski, Angels Ramos, Laura Tolos

Summary: The FSU2H equation-of-state model is extended to finite temperature and it is found that temperature has a stronger effect on thermodynamical observables and the composition of neutron star cores when considering hyperonic degrees of freedom. The widely used Gamma law is not appropriate to reproduce the true thermal effects, especially when hyperons become abundant in the neutron star core. Simple parametrizations of the thermal index for nucleonic and hyperonic beta-stable neutrino-free matter are provided to make finite temperature equations of state easily accessible.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Physics, Nuclear

Machine learning light hypernuclei

Isaac Vidana

Summary: In this study, a feed-forward artificial neural network is employed to extrapolate the separation energy BA of the lightest hypernuclei "3AH, 4AH, and 4AHe" obtained from ab-initio hypernuclear No-Core Shell Model calculations to large model spaces. The overfitting problem is addressed by increasing the size of the input dataset and by introducing Gaussian noise during the training process of the neural network. The results show that the neural network with a single hidden layer of eight neurons is capable of accurately extrapolating the A separation energy to model spaces of size Nmax = 100.

NUCLEAR PHYSICS A (2023)

Article Physics, Multidisciplinary

Double-Strangeness Molecular-Type Pentaquarks from Coupled-Channel Dynamics

J. A. Marse-Valera, V. K. Magas, A. Ramos

Summary: The existence of pentaquarks with strangeness content zero and one is a significant discovery in recent years in the field of hadron physics. These states can be explained as hadronic molecules and were predicted before their discovery based on a model using unitarized meson-baryon amplitudes obtained from vector meson exchange interactions. Contrary to previous beliefs, this model also predicts the existence of pentaquarks with double strangeness at approximately 4500 and 4600 MeV, which are generated through a specific and unique mechanism involving a strong coupling between the two heaviest meson-baryon states.

PHYSICAL REVIEW LETTERS (2023)

Article Physics, Multidisciplinary

Constraint of the Nuclear Dissipation Coefficient in Fission of Hypernuclei

J. L. Rodriguez-Sanchez, J. Cugnon, J. -C. David, J. Hirtz, A. Kelic-Heil, I. Vidana

Summary: Experimental studies combined with advanced calculations have successfully investigated the nuclear dissipation mechanism in normal nuclear matter. The dissipation coefficients have been well constrained in transport theories through the use of various fission observables. However, the investigation of the dissipation coefficient needs to be extended to the strangeness sector due to the presence of hypernuclei and possible hyperons in neutron stars.

PHYSICAL REVIEW LETTERS (2023)

Article Astronomy & Astrophysics

X(3872), X(4014), and their bottom partners at finite temperature

Gloria Montana, Angels Ramos, Laura Tolos, Juan M. Torres-Rincon

Summary: This study investigates the properties of X(3872) and its spin partner X(4014) in both vacuum and at finite temperature. The X(3872) is dynamically generated through the s-wave rescattering of pseudoscalar and vector charm mesons, while the X(4014) is obtained from the scattering of charm vector mesons. The properties of their bottom counterparts are predicted using heavy-quark flavor symmetry. The dynamically generated states exhibit decreasing mass and increasing decay width with temperature, consistent with their meson constituents. These results have implications for relativistic heavy-ion collisions, analysis of the medium formed after hadronization, and femtoscopic studies, and can be tested in lattice-QCD calculations.

PHYSICAL REVIEW D (2023)

Article Astronomy & Astrophysics

Femtoscopy of D mesons and light mesons upon unitarized effective field theories

Juan M. Torres-Rincon, Angels Ramos, Laura Tolos

Summary: Hadron femtoscopy is a useful tool for studying heavy-ion collisions and hadron interactions. In this study, the authors focus on heavy-flavor femtoscopy using the ALICE detector at the LHC. They compute correlation functions of D mesons and light mesons to access the wave function and predict correlation functions involving various meson combinations. The results provide insights into the energy states of meson systems.

PHYSICAL REVIEW D (2023)

Article Physics, Nuclear

Effect of chiral nuclear forces on the neutrino mean free path in hot neutron matter

Isaac Vidana, Domenico Logoteta, Ignazio Bombaci

Summary: We investigated the influence of chiral nuclear forces on the propagation of neutrinos in hot neutron matter. Our results showed that the dynamical structure factor and the neutrino mean free path depended on the cutoff only at leading order (LO) and next-to-leading order (NLO), but this dependence became strongly reduced at higher orders due to the contribution of three-nucleon forces. The uncertainty associated with our calculation of the neutrino mean free path was estimated and found to vary with density.

PHYSICAL REVIEW C (2022)

Proceedings Paper Engineering, Aerospace

The enhanced X-ray Timing and Polarimetry mission - eXTP: an update on its scientific cases, mission profile and development status

Shuang-Nan Zhang, Andrea Santangelo, Yupeng Xu, Marco Feroci, Margarita Hernanz, Fangjun Lu, Yong Chen, Hua Feng, Kirpal Nandra, Weichun Jiang, Jiri Svoboda, Soren Brandt, Stephane Schanne, Jean in't Zand, Malgorzata Michalska, Enrico Bozzo, Emrah Kalemci, Ivan Agudo, Mahdi Ahangarianabhari, Gabby Aitink-Kroes, Giovanni Ambrosi, Filippo Ambrosino, Zhenghua An, Miguel Angel Perez Torres, Matias Antonelli, Andrea Argan, Viktor Babinec, Luca Baldini, Marco Barbera, Coen van Baren, David Baudin, Joerg Bayer, Ronaldo Bellazzini, Pierluigi Bellutti, Bruna Bertucci, Giuseppe Bertuccio, Xingzi Bi, Mirko Boezio, Valter Bonvicini, Walter Bonvicini, Pol Bordas, Alice Borghese, Giacomo Borghi, Florent Bouyjou, Ayhan Bozkurt, Alessandro Brez, Daniele Brienza, Franck Cadoux, Riccardo Campana, Jiewei Cao, Xuelei Cao, Jorge Casares, Elisabetta Cavazzuti, Francesco Ceraudo, Tianxiang Chen, Wen Chen, Can Chen, Yupeng Chen, Xin Chen, Yehai Chen, Jerome Chenevez, Yaodong Cheng, Daniela Cirrincione, Marta Civitani, Min Cong, Francesco Coti Zelati, Weiwei Cui, Tao Cui, Wei Cui, Boyu Dai, Thomas Dauser, Nicolas De Angelis, Barbara De Marco, Alessandra De Rosa, Ettore Del Monte, Sergio Di Cosimo, Sebastian Diebold, Giuseppe Dilillo, Fei Ding, Roman Dohnal, Zefang Dong, Immacolata Donnarumma, Michal Dovciak, Yuanyuan Du, Lorenzo Ducci, Yuri Evangelista, Qingmei Fan, Yannick Favre, Patricia Ferres, Emanuele Fiandrini, Francesco Ficorella, Fabio Fuschino, Jose Luis Galvez, Na Gao, Min Gao, Yuqiang Ge, Mingyu Ge, Olivier Gevin, Marco Grassi, Yudong Gu, Quanying Gu, Ju Guan, Manuel Guedel, Xingbo Han, Dawei Han, Huilin He, Junwang He, Paul Hedderman, Jan-Willem den Herder, Bin Hong, Ander Hormaetxe, Dongjie Hou, Zexun Hu, Hao Hu, Qingbao Hu, Yu Hu, Yue Huang, Jiangjiang Huang, Qiushi Huang, Jia Huo, Richard Hynek, Kazumi Iwasawa, Lucca Izzo, Long Ji, Shumei Jia, Bowen Jiang, Wei Jiang, Jiechen Jiang, Xiaowei Jiang, Yang Jiao, Ge Jin, Fan Jin, Jordi Jose, Vladimir Karas, Thomas Kennedy, Christian Kirsch, Merlin Kole, Martin Komarek, Ingo Kreykenbohm, Lucien Kuiper, Irfan Kuvvetli, Claudio Labanti, Luca Latronico, Phillip Laubert, Tao Li, Longhui Li, Hong Li, Duo Li, Wei Li, Maoshun Li, Gang Li, Xiaobo Li, Chengkui Li, Bing Li, Haibo Li, Hong Liang, Qiuyan Liao, Jinyuan Liao, Olivier Limousin, Yanjian Lin, Manuel Linares, Rui Liu, Yichen Liu, Zhihao Liu, Hongwei Liu, Xiaojing Liu, Xiaohua Liu, Ugo Lo Cicero, Jens Loehring, Giovanni Lombardi, Maximilian Lorenz, Bing Lu, Leonardo Lucchesi, Tao Luo, Laidan Luo, Jia Ma, Xiang Ma, Daniele Macera, Piero Malcovati, Alberto Manfreda, Josep Maria Paredes, Andrea Marinucci, Adrian Martindale, Norbert Meidinger, Filippo Mele, Vasco Mendes, Bin Meng, Martin Merkl, Aline Meuris, Giovanni Miniutti, Massimo Minuti, Alfredo Morbidini, Gianluca Morgante, Fabio Muleri, Riccardo Munini, Lorenzo Mussolin, Barbara Negri, Jianyin Nie, Petr Novak, Witold Nowosielski, Alessio Nuti, Ahmet Onat, Piotr Orleanski, Leonardo Orsini, Roland Ottensamer, Ge Ou, Luigi Pacciani, Stephane Paltani, Teng Pan, Kai Pan, Giovanni Pareschi, Alessandro Patruno, Giancarlo Pepponi, Emanuele Perinati, Raffaele Piazzolla, Antonino Picciotto, Claudio Piemonte, Michele Pinchera, Samuel Pliego, Juri Poutanen, Liqiang Qi, Fazhi Qi, Pengfei Qiang, Fangjian Qiao, Zheng Qiao, Xiangbiao Qiu, Chengbo Qiu, Jinlu Qu, Alexandre Rachevski, Irina Rashevskaia, Nanda Rea, Marc Ribo, Rob de la Rie, Jerome Rodriguez, Pablo Rodriguez Gil, Gloria Sala, Thomas Schanz, Roberto Serafinelli, Carmelo Sgro, Zhengxiang Shen, Lizhi Sheng, Jingyan Shi, Giorgia Sironi, Konrad Skup, Liming Song, Zeyu Song, Jiangbo Song, Gloria Spandre, Daniele Spiga, Yongquan Su, Liang Sun, Muberra Sungur, Libor Sveda, Gianpiero Tagliaferri, Ying Tan, Lian Tao, Denis Tcherniak, Chris Tenzer, Michela Todaro, Laura Tolos, Gabriel Torok, Diego F. Torres, Alessio Trois, Onur Turhan, Phil Uttley, Andrea Vacchi, Enrico Virgilli, Channah Vogel, Dave Walton, Jian Wang, Xianqi Wang, Bo Wang, Langping Wang, Xiaofeng Wang, Dianlong Wang, Yusa Wang, Juan Wang, Hao Wang, Ruijie Wang, Ping Wang, Lingjun Wang, Wenshuai Wang, Tian Wang, Haoyu Wang, Zhanshan Wang, Anna L. Watts, Xiangyang Wen, Joern Wilms, Berend Winter, Xin Wu, Chao Wu, Zhenyu Wu, Qiong Wu, Kaiji Wu, Hao Xiong, Shaolin Xiong, Wei Xu, Zhao Xu, Jingjing Xu, Xiongwei Xu, Jiadai Xue, Yongqing Yan, Xingtao Yan, Xianghui Yang, Yanji Yang, Xiongtao Yang, Sheng Yang, Jiawei Yang, Yingquan Yang, Shuxu Yi, Yonggao Yu, Ke Yu, Ganluigi Zampa, Nicola Zampa, Silvia Zane, Andrzej A. Zdziarski, Long Zhang, Shu Zhang, Wenda Zhang, Xiaoli Zhang, Zhen Zhang, Jiawei Zhang, Fan Zhang, Ziliang Zhang, Dali Zhang, Honglin Zhang, Aimei Zhang, Tong Zhang, Hongmei Zhang, Juan Zhang, Liang Zhang, Yueting Zhang, Li Zhao, Baosheng Zhao, Zijian Zhao, Xiaofan Zhao, Haisheng Zhao, Xiaoyun Zhao, Shijie Zheng, Yupeng Zhou, Xiaohong Zhou, Jiahuan Zhu, Yuxuan Zhu, Cheng Zhu, Zhencai Zhu, Nicola Zorzi, Frans Zwart

Summary: The enhanced X-ray Timing and Polarimetry mission is a flagship observatory that explores the properties of matter and the propagation of light in extreme conditions found in the Universe. With its advanced technology and capabilities, the mission is of great significance. It is currently in progress and is expected to be completed by mid-2022.

SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY (2022)

Article Astronomy & Astrophysics

Quick Guides for Use of the CompOSE Data Base

Veronica Dexheimer, Marco Mancini, Micaela Oertel, Constanca Providencia, Laura Tolos, Stefan Typel

Summary: This article presents a combination of two quick guides that summarize relevant information about the CompOSE nuclear equation of state repository. The first guide is aimed at nuclear physicists and provides instructions on how to provide standard equation of state tables, while the second guide is meant for users and describes the basic procedures to obtain customized tables with equation of state data. Several examples are included to help both providers and users of the CompOSE database.

PARTICLES (2022)

Article Astronomy & Astrophysics

Second Love number of dark compact planets and neutron stars with dark matter

Yannick Dengler, Juergen Schaffner-Bielich, Laura Tolos

Summary: We study the mass-radius relation and the second Love number of compact objects made of ordinary matter and non-self-annihilating fermionic dark matter. We find that the second Love numbers of these objects can be significantly different from those of neutron stars without dark matter. Measuring the tidal deformability of these compact objects can determine the presence of dark matter inside neutron stars.

PHYSICAL REVIEW D (2022)

Article Physics, Nuclear

In-medium kinetic theory of D mesons and heavy-flavor transport coefficients

Juan M. Torres-Rincon, Gloria Montana, Angels Ramos, Laura Tolos

Summary: We extend the kinetic theory of D mesons to include thermal and off-shell effects caused by the modification of heavy-meson spectral functions in the medium. Using the Kadanoff-Baym approach, we derive the off-shell Fokker-Planck equation that encodes the heavy-flavor transport coefficients. We analyze the thermal width of D mesons due to their scattering off light mesons, focusing on new in-medium effects and find that the D-meson spatial diffusion coefficient matches well with lattice-QCD calculations and Bayesian analyses at higher temperatures.

PHYSICAL REVIEW C (2022)

暂无数据