Pub Date : 2020-10-26DOI: 10.1016/j.physletb.2021.136584
F. Gao, J. Pawlowski
{"title":"Chiral phase structure and critical end point in QCD","authors":"F. Gao, J. Pawlowski","doi":"10.1016/j.physletb.2021.136584","DOIUrl":"https://doi.org/10.1016/j.physletb.2021.136584","url":null,"abstract":"","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"520 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-26","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"77094814","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-24DOI: 10.1103/PHYSREVD.103.075003
P. Bakhti, M. Rajaee
We investigate the potential of the next generation long-baseline neutrino experiments DUNE and T2HK as well as the upcoming reactor experiment JUNO to constrain Non-Standard Interaction (NSI) parameters. JUNO is going to provide the most precise measurements of solar neutrino oscillation parameters as well as determining the neutrino mass ordering. We study how the results of JUNO combined with those of long-baseline neutrino experiments such as DUNE and T2HK can help to determine oscillation parameters and to constrain NSI parameters. We present excluded regions in NSI parameter space, $epsilon_{alpha beta}$ assuming Standard Model (SM) as the null hypothesis. We further explore the correlations between the NSI parameters and CP-violation phase.
{"title":"Sensitivities of future reactor and long-baseline neutrino experiments to NSI","authors":"P. Bakhti, M. Rajaee","doi":"10.1103/PHYSREVD.103.075003","DOIUrl":"https://doi.org/10.1103/PHYSREVD.103.075003","url":null,"abstract":"We investigate the potential of the next generation long-baseline neutrino experiments DUNE and T2HK as well as the upcoming reactor experiment JUNO to constrain Non-Standard Interaction (NSI) parameters. JUNO is going to provide the most precise measurements of solar neutrino oscillation parameters as well as determining the neutrino mass ordering. We study how the results of JUNO combined with those of long-baseline neutrino experiments such as DUNE and T2HK can help to determine oscillation parameters and to constrain NSI parameters. We present excluded regions in NSI parameter space, $epsilon_{alpha beta}$ assuming Standard Model (SM) as the null hypothesis. We further explore the correlations between the NSI parameters and CP-violation phase.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-24","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"76477452","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-23DOI: 10.1103/PHYSREVD.103.036005
Zhi Hu, Siqi Xu, C. Mondal, Xingbo Zhao, J. Vary
We investigate the leading-twist transverse momentum-dependent distribution functions (TMDs) for a physical electron, a spin-1/2 composite system consisting of a bare electron and a photon, using the Basis Light-front Quantization (BLFQ) framework. The light-front wave functions of the physical electron are obtained from the eigenvectors of the light-front QED Hamiltonian. We evaluate the TMDs using the overlaps of the light-front wave functions. The BLFQ results are found to be in excellent agreement with those TMDs calculated using lowest-order perturbation theory.
{"title":"Transverse structure of electron in momentum space in basis light-front quantization","authors":"Zhi Hu, Siqi Xu, C. Mondal, Xingbo Zhao, J. Vary","doi":"10.1103/PHYSREVD.103.036005","DOIUrl":"https://doi.org/10.1103/PHYSREVD.103.036005","url":null,"abstract":"We investigate the leading-twist transverse momentum-dependent distribution functions (TMDs) for a physical electron, a spin-1/2 composite system consisting of a bare electron and a photon, using the Basis Light-front Quantization (BLFQ) framework. The light-front wave functions of the physical electron are obtained from the eigenvectors of the light-front QED Hamiltonian. We evaluate the TMDs using the overlaps of the light-front wave functions. The BLFQ results are found to be in excellent agreement with those TMDs calculated using lowest-order perturbation theory.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"7 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-23","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"79749328","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-22DOI: 10.1103/physrevd.102.094021
Wen-Long Sang, F. Feng, Yu Jia
Within the nonrelativistic QCD (NRQCD) factorization framework, we compute the ${mathcal O}(alpha_s v^2)$ corrections to the hadronic decay rate of vector quarkonia, exemplified by $J/psi$ and $Upsilon$. Setting both the renormalization and NRQCD factorization scales to be $m_Q$, we obtain $Gamma(J/psito {rm LH})= 0.0716frac{alpha_s^3}{m_c^2} langle mathcal{O}_1({}^3S_1)rangle_{J/psi} [1-1.19alpha_s+(-5.32+3.03alpha_s)langle v^2rangle_{J/psi}]$ and $Gamma(Upsilonto {rm LH})= 0.0716frac{alpha_s^3}{m_b^2}langlemathcal{O}_1({}^3S_1)rangle_{Upsilon}[1-1.56alpha_s+(-5.32+4.61alpha_s)langle v^2rangle_{Upsilon}]$. We confirm the previous calculation of $mathcal{O}(alpha_s)$ corrections on a diagram-by-diagram basis, with the accuracy significantly improved. For $J/psi$ hadronic decay, we find that the ${mathcal O}(alpha_sv^2)$ corrections are moderate and positive, nevertheless unable to counterbalance the huge negative corrections. On the other hand, the effect of ${mathcal O}(alpha_sv^2)$ corrections for $Upsilon(nS)$ is sensitive to the $mathcal{O}(v^2)$ NRQCD matrix elements. With the appropriate choice of the NRQCD matrix elements, our theoretical predictions for the decay rates may be consistent with the experimental data for $Upsilon(1S,2S)to {rm LH}$. As a byproduct, we also present the theoretical predictions for the branching ratio of $J/psi(Upsilon)to 3gamma$ accurate up to $mathcal{O}(alpha_s v^2)$.
{"title":"O(αsv2)\u0000 corrections to the hadronic decay of vector quarkonia","authors":"Wen-Long Sang, F. Feng, Yu Jia","doi":"10.1103/physrevd.102.094021","DOIUrl":"https://doi.org/10.1103/physrevd.102.094021","url":null,"abstract":"Within the nonrelativistic QCD (NRQCD) factorization framework, we compute the ${mathcal O}(alpha_s v^2)$ corrections to the hadronic decay rate of vector quarkonia, exemplified by $J/psi$ and $Upsilon$. Setting both the renormalization and NRQCD factorization scales to be $m_Q$, we obtain $Gamma(J/psito {rm LH})= 0.0716frac{alpha_s^3}{m_c^2} langle mathcal{O}_1({}^3S_1)rangle_{J/psi} [1-1.19alpha_s+(-5.32+3.03alpha_s)langle v^2rangle_{J/psi}]$ and $Gamma(Upsilonto {rm LH})= 0.0716frac{alpha_s^3}{m_b^2}langlemathcal{O}_1({}^3S_1)rangle_{Upsilon}[1-1.56alpha_s+(-5.32+4.61alpha_s)langle v^2rangle_{Upsilon}]$. We confirm the previous calculation of $mathcal{O}(alpha_s)$ corrections on a diagram-by-diagram basis, with the accuracy significantly improved. For $J/psi$ hadronic decay, we find that the ${mathcal O}(alpha_sv^2)$ corrections are moderate and positive, nevertheless unable to counterbalance the huge negative corrections. On the other hand, the effect of ${mathcal O}(alpha_sv^2)$ corrections for $Upsilon(nS)$ is sensitive to the $mathcal{O}(v^2)$ NRQCD matrix elements. With the appropriate choice of the NRQCD matrix elements, our theoretical predictions for the decay rates may be consistent with the experimental data for $Upsilon(1S,2S)to {rm LH}$. As a byproduct, we also present the theoretical predictions for the branching ratio of $J/psi(Upsilon)to 3gamma$ accurate up to $mathcal{O}(alpha_s v^2)$.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"48 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-22","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"80615958","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-21DOI: 10.1103/PHYSREVD.103.083528
Bugeon Jo, HyeonTae Kim, Hyungdo Kim, C. Shin
We study the cosmology of a dark sector consisting of (ultra) light scalars. Since the scalar mass is radiatively unstable, a special explanation is required to make it much smaller than the UV scale. There are two well-known mechanisms for the origin of scalar mass. The scalar can be identified as a pseudo-Goldstone boson, whose shift symmetry is explicitly broken by non-perturbative corrections, like the axion. Alternatively, it can be identified as a composite particle like the glueball, whose mass is limited by the confinement scale of the theory. In both cases, the scalar can be naturally light, but interaction behavior is quite different. The lighter the axion (glueball) mass is, the weaker (stronger) the interaction strength is. We consider the dark axion whose shift symmetry is anomalously broken by the hidden non-abelian gauge symmetry. After the confinement of the gauge group, the dark axion and the dark glueball get masses and both form multicomponent dark matter. We carefully consider the effects of energy flow from the dark gluons to the dark axions and derive the full equations of motion for the background and the perturbed variables. The effect of the dark axion-dark gluon coupling on the evolution of the entropy and the isocurvature perturbations is also clarified. Finally, we discuss the gravo-thermal collapse of the glueball subcomponent dark matter after the halos form, in order to explore the potential to contribute to the formation of seeds for the supermassive black holes observed at high redshifts. With simplified assumptions, the glueball subcomponent dark matter with the mass of $sim 0.01-1{rm MeV}$, and the axion dark matter with the GUT scale decay constant (the mass of ${cal O}(10^{-18}),{rm eV}$) can provide the hint on the origin of the supermassive black holes at high redshifts.
{"title":"Exploring the Universe with dark light scalars","authors":"Bugeon Jo, HyeonTae Kim, Hyungdo Kim, C. Shin","doi":"10.1103/PHYSREVD.103.083528","DOIUrl":"https://doi.org/10.1103/PHYSREVD.103.083528","url":null,"abstract":"We study the cosmology of a dark sector consisting of (ultra) light scalars. Since the scalar mass is radiatively unstable, a special explanation is required to make it much smaller than the UV scale. There are two well-known mechanisms for the origin of scalar mass. The scalar can be identified as a pseudo-Goldstone boson, whose shift symmetry is explicitly broken by non-perturbative corrections, like the axion. Alternatively, it can be identified as a composite particle like the glueball, whose mass is limited by the confinement scale of the theory. In both cases, the scalar can be naturally light, but interaction behavior is quite different. The lighter the axion (glueball) mass is, the weaker (stronger) the interaction strength is. We consider the dark axion whose shift symmetry is anomalously broken by the hidden non-abelian gauge symmetry. After the confinement of the gauge group, the dark axion and the dark glueball get masses and both form multicomponent dark matter. We carefully consider the effects of energy flow from the dark gluons to the dark axions and derive the full equations of motion for the background and the perturbed variables. The effect of the dark axion-dark gluon coupling on the evolution of the entropy and the isocurvature perturbations is also clarified. Finally, we discuss the gravo-thermal collapse of the glueball subcomponent dark matter after the halos form, in order to explore the potential to contribute to the formation of seeds for the supermassive black holes observed at high redshifts. With simplified assumptions, the glueball subcomponent dark matter with the mass of $sim 0.01-1{rm MeV}$, and the axion dark matter with the GUT scale decay constant (the mass of ${cal O}(10^{-18}),{rm eV}$) can provide the hint on the origin of the supermassive black holes at high redshifts.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"69 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"85818198","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-21DOI: 10.1103/physrevd.103.014003
Soeren Schlichting, Pragya Singh
We simulate the 3+1 D classical Yang-Mills dynamics of the collisions of longitudinally extended nuclei, described by eikonal color charges in the Color Glass Condensate framework. By varying the longitudinal thickness of the colliding nuclei, we discuss the violations of boost invariance and explore how the boost invariant high-energy limit is approached. Subsequently, we develop a more realistic model of the three dimensional color charge distributions that connects longitudinal and transverse fluctuations to the $x$ and $k_T$ dependence of transverse momentum dependent parton distributions, and explore the resulting rapidity profiles and their longitudinal fluctuations.
{"title":"3-D structure of the Glasma initial state: Breaking boost-invariance by collisions of extended shock waves in classical Yang-Mills theory","authors":"Soeren Schlichting, Pragya Singh","doi":"10.1103/physrevd.103.014003","DOIUrl":"https://doi.org/10.1103/physrevd.103.014003","url":null,"abstract":"We simulate the 3+1 D classical Yang-Mills dynamics of the collisions of longitudinally extended nuclei, described by eikonal color charges in the Color Glass Condensate framework. By varying the longitudinal thickness of the colliding nuclei, we discuss the violations of boost invariance and explore how the boost invariant high-energy limit is approached. Subsequently, we develop a more realistic model of the three dimensional color charge distributions that connects longitudinal and transverse fluctuations to the $x$ and $k_T$ dependence of transverse momentum dependent parton distributions, and explore the resulting rapidity profiles and their longitudinal fluctuations.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"20 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"78160296","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-21DOI: 10.1103/PHYSREVD.103.054015
Somenath Pal, G. Kadam, H. Mishra, A. Bhattacharyya
We investigate the effects of repulsive interaction between hadrons on the fluctuations of the conserved charges. We calculate the baryon,the electric charge and the strangeness susceptibilities within the ambit of hadron resonance gas model extended to include the short range repulsive interactions.The repulsive interactions are included through a mean-field approach where the single particle energy gets modified due to mean field interactions between hadrons proportional to the number density of hadrons.We assume different mean-field interactions for mesons and baryons. It is shown that the repulsive interactions play a very crucial role to describe hadronic matter near transition temperature. We also show that in order to consistently describe higher order conserved charge fluctuations mesonic repulsive interactions cannot be neglected. Further, we demonstrate that the repulsive interaction of baryons are essential to describe the lattice simulation results at finite baryonchemical potential for higher order fluctuations.
{"title":"Effects of hadronic repulsive interactions on the fluctuations of conserved charges","authors":"Somenath Pal, G. Kadam, H. Mishra, A. Bhattacharyya","doi":"10.1103/PHYSREVD.103.054015","DOIUrl":"https://doi.org/10.1103/PHYSREVD.103.054015","url":null,"abstract":"We investigate the effects of repulsive interaction between hadrons on the fluctuations of the conserved charges. We calculate the baryon,the electric charge and the strangeness susceptibilities within the ambit of hadron resonance gas model extended to include the short range repulsive interactions.The repulsive interactions are included through a mean-field approach where the single particle energy gets modified due to mean field interactions between hadrons proportional to the number density of hadrons.We assume different mean-field interactions for mesons and baryons. It is shown that the repulsive interactions play a very crucial role to describe hadronic matter near transition temperature. We also show that in order to consistently describe higher order conserved charge fluctuations mesonic repulsive interactions cannot be neglected. Further, we demonstrate that the repulsive interaction of baryons are essential to describe the lattice simulation results at finite baryonchemical potential for higher order fluctuations.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"9 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-21","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"89800728","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-20DOI: 10.1140/EPJC/S10052-021-08983-3
Zhen Zhang, Liang Zheng, Gang Chen, Hong-ge Xu, D. Zhou, Yu-Liang Yan, B. Sa
{"title":"The study of exotic state $$Z_c^{pm }(3900)$$ decaying to $$J/psi pi ^{pm }$$ in the pp collisions at $$sqrt{s}$$ = 1.96, 7, and 13 TeV","authors":"Zhen Zhang, Liang Zheng, Gang Chen, Hong-ge Xu, D. Zhou, Yu-Liang Yan, B. Sa","doi":"10.1140/EPJC/S10052-021-08983-3","DOIUrl":"https://doi.org/10.1140/EPJC/S10052-021-08983-3","url":null,"abstract":"","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"81055467","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-20DOI: 10.1103/PhysRevC.102.054907
Yi-An Li, Song Zhang, Yugang Ma
$alpha$-clustered structures in light nuclei could be studied through "snapshots" taken by relativistic heavy-ion collisions. A multiphase transport (AMPT) model is employed to simulate the initial structure of collision nuclei and the proceeding collisions at center of mass energy $sqrt{s_{NN}}$ = 6.37 TeV. This initial structure can finally be reflected in the subsequent observations, such as elliptic flow ($v_{2}$), triangular flow ($v_{3}$) and quadrangular flow ($v_4$). Three sets of the collision systems are chosen to illustrate system scan is a good way to identify the exotic $alpha$-clustered nuclear structure, case I: $mathrm{^{16}O}$ nucleus (with or without $alpha$-cluster) + ordinary nuclei (always in Woods-Saxon distribution) in most central collisions, case II: $mathrm{^{16}O}$ nucleus (with or without $alpha$-cluster) + $mathrm{^{197}Au}$ nucleus collisions for centrality dependence, and case III: symmetric collision systems (namely, $^{10}$B + $^{10}$B, $^{12}$C + $^{12}$C, $^{16}$O + $^{16}$O (with or without $alpha$-cluster), $^{20}$Ne + $^{20}$Ne, and $^{40}$Ca + $^{40}$Ca) in most central collisions. Our calculations propose that relativistic heavy-ion collision experiments at $sqrt{s_{NN}}$ = 6.37 TeV are promised to distinguish the tetrahedron structure of $mathrm{^{16}O}$ from the Woods-Saxon one and shed lights on the system scan projects in experiments.
$alpha$可以通过相对论性重离子碰撞拍摄的“快照”来研究轻核中的簇状结构。采用多相输运(AMPT)模型模拟了碰撞核的初始结构和在质能中心$sqrt{s_{NN}}$ = 6.37 TeV处的后续碰撞。这种初始结构最终可以在后续的观测中体现出来，如椭圆流($v_{2}$)、三角形流($v_{3}$)和四边形流($v_4$)。选择三组碰撞系统来说明系统扫描是识别奇异的$alpha$ -聚类核结构的好方法，情况I:在大多数中心碰撞中$mathrm{^{16}O}$核(有或没有$alpha$ -聚类)+普通核(总是在Woods-Saxon分布中)，情况II: $mathrm{^{16}O}$核(有或没有$alpha$ -聚类)+ $mathrm{^{197}Au}$核碰撞中心依赖性，情况III:对称碰撞系统(即$^{10}$ B + $^{10}$ B, $^{12}$ C + $^{12}$ C, $^{16}$ O + $^{16}$ O(有或没有$alpha$ -cluster)， $^{20}$ Ne + $^{20}$ Ne和$^{40}$ Ca + $^{40}$ Ca)在大多数中心碰撞中。我们的计算表明，$sqrt{s_{NN}}$ = 6.37 TeV的相对论重离子碰撞实验有望将$mathrm{^{16}O}$的四面体结构与Woods-Saxon结构区分开来，并为实验中的系统扫描项目提供了启示。
{"title":"Signatures of \u0000α\u0000-clustering in \u0000O16\u0000 by using a multiphase transport model","authors":"Yi-An Li, Song Zhang, Yugang Ma","doi":"10.1103/PhysRevC.102.054907","DOIUrl":"https://doi.org/10.1103/PhysRevC.102.054907","url":null,"abstract":"$alpha$-clustered structures in light nuclei could be studied through \"snapshots\" taken by relativistic heavy-ion collisions. A multiphase transport (AMPT) model is employed to simulate the initial structure of collision nuclei and the proceeding collisions at center of mass energy $sqrt{s_{NN}}$ = 6.37 TeV. This initial structure can finally be reflected in the subsequent observations, such as elliptic flow ($v_{2}$), triangular flow ($v_{3}$) and quadrangular flow ($v_4$). Three sets of the collision systems are chosen to illustrate system scan is a good way to identify the exotic $alpha$-clustered nuclear structure, case I: $mathrm{^{16}O}$ nucleus (with or without $alpha$-cluster) + ordinary nuclei (always in Woods-Saxon distribution) in most central collisions, case II: $mathrm{^{16}O}$ nucleus (with or without $alpha$-cluster) + $mathrm{^{197}Au}$ nucleus collisions for centrality dependence, and case III: symmetric collision systems (namely, $^{10}$B + $^{10}$B, $^{12}$C + $^{12}$C, $^{16}$O + $^{16}$O (with or without $alpha$-cluster), $^{20}$Ne + $^{20}$Ne, and $^{40}$Ca + $^{40}$Ca) in most central collisions. Our calculations propose that relativistic heavy-ion collision experiments at $sqrt{s_{NN}}$ = 6.37 TeV are promised to distinguish the tetrahedron structure of $mathrm{^{16}O}$ from the Woods-Saxon one and shed lights on the system scan projects in experiments.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"28 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"91148915","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
Pub Date : 2020-10-20DOI: 10.1103/PHYSREVD.103.035018
Luis A. Delgadillo, P. Huber
Tagged kaon beams are attractive neutrino sources, which would provide flavor pure $nu_e$-beams with exactly measured normalization. We point out that this also leads to an anti-tagged flavor pure $nu_mu$-beam, with equally well known normalization. Exposing a 1 kt liquid argon detector at a baseline of 1 km to this combination of unique beams allows to decisively test recent indications by IceCube and Neutrino-4 of sterile neutrino oscillations in the multi-eV range.
{"title":"Sterile neutrino searches at tagged kaon beams","authors":"Luis A. Delgadillo, P. Huber","doi":"10.1103/PHYSREVD.103.035018","DOIUrl":"https://doi.org/10.1103/PHYSREVD.103.035018","url":null,"abstract":"Tagged kaon beams are attractive neutrino sources, which would provide flavor pure $nu_e$-beams with exactly measured normalization. We point out that this also leads to an anti-tagged flavor pure $nu_mu$-beam, with equally well known normalization. Exposing a 1 kt liquid argon detector at a baseline of 1 km to this combination of unique beams allows to decisively test recent indications by IceCube and Neutrino-4 of sterile neutrino oscillations in the multi-eV range.","PeriodicalId":8457,"journal":{"name":"arXiv: High Energy Physics - Phenomenology","volume":"1 1","pages":""},"PeriodicalIF":0.0,"publicationDate":"2020-10-20","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"85538457","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":0,"RegionCategory":"","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
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