PaperPanorama

HEP Phenomenology·hep-ph

Tue·Feb 11, 2020

33 papers26 primary·7 cross-listed·reconstructed*

  1. 01*

    Far-forward neutrinos at the Large Hadron Collider

    Weidong Bai🇺🇸 · Milind Diwan🇺🇸 · Maria Vittoria Garzelli🇮🇹 · Yu Seon Jeong🇨🇭 · Mary Hall Reno🇺🇸

    We present a new calculation of the energy distribution of high-energy neutrinos from the decay of charm and bottom hadrons produced at the Large Hadron Collider (LHC). In the kinematical region of very forward rapidities, heavy-flavor production and decay is a source of tau neutrinos that leads to thousands of { charged-current} tau neutrino events in a 1 m long, 1 m radius lead neutrino detector at a distance of 480 m from the interaction region. In our computation, next-to-leading order QCD radiative corrections are accounted for in the production cross-sections. Non-perturbative intrinsic- effects are approximated by a simple phenomenological model introducing a Gaussian -smearing of the parton distribution functions, which might also mimic perturbative effects due to multiple initial-state soft-gluon emissions. The transition from partonic to hadronic states is described by phenomenological fragmentation functions. To study the effect of various input parameters, theoretical predictions for production are compared with LHCb data on double-differential cross-sections in transverse momentum and rapidity. The uncertainties related to the choice of the input parameter values, ultimately affecting the predictions of the tau neutrino event distributions, are discussed. We consider a 3+1 neutrino mixing scenario to illustrate the potential for a neutrino experiment to constrain the 3+1 parameter space using tau neutrinos and antineutrinos. We find large theoretical uncertainties in the predictions of the neutrino fluxes in the far-forward region. Untangling the effects of tau neutrino oscillations into sterile neutrinos and distinguishing a 3+1 scenario from the standard scenario with three active neutrino flavours, will be challenging due to the large theoretical uncertainties from QCD.

    hep-phhep-exnucl-exnucl-thJHEP(2020)·66 citations
  2. 02*

    Midi-review: Status of weak scale supersymmetry after LHC Run 2 and ton-scale noble liquid WIMP searches

    Howard Baer🇺🇸 · Vernon Barger🇺🇸 · Shadman Salam🇺🇸 · Dibyashree Sengupta🇺🇸 · Kuver Sinha🇺🇸

    While LHC has discovered a very Standard Model-like Higgs boson of mass m_h~ 125 GeV, no solid signal for physics beyond the Standard Model has emerged so far at LHC or at WIMP seach experiments. For the case of weak scale supersymmetry (SUSY), LHC has found rather generally that gluinos are beyond about 2.2 TeV whilst top squark must lie beyond 1.1 TeV. These limits contradict older simplistic notions of naturalness that emerged in the 1980s-1990s, leading to the rather pessimistic view that SUSY is now excluded except for perhaps some remaining narrow corners of parameter space. Yet, this picture ignores several important developments in SUSY/string theory that emerged in the 21st century: 1. the emergence of the string theory landscape and its solution to the cosmological constant problem, 2. a more nuanced view of naturalness including the notion of "stringy naturalness", 3. the emergence of anomaly-free discrete R-symmetries and their connection to R-parity, Peccei-Quinn symmetry, the SUSY mu problem and proton decay and 4. the importance of including a solution to the strong CP problem. Rather general considerations from the string theory landscape favor large values of soft terms, subject to the vacuum selection criteria that electroweak symmetry is properly broken (no CCB minima) and the resulting magnitude of the weak scale is not too far from our measured value. Then stringy naturalness predicts a Higgs mass m_h~ 125 GeV whilst sparticle masses are typically lifted beyond present LHC bounds. In light of these refinements in theory perspective confronted by LHC and dark matter search results, we review the most likely LHC, ILC and dark matter signatures that are expected to arise from weak scale SUSY as we understand it today.

    hep-phEur.Phys.J.ST(2020)·100 citations
  3. 03*

    On charm-mass dependent NNLO corrections to B -> Xs gamma

    M. Misiak🇵🇱 · A. Rehman🇩🇪 · M. Steinhauser🇩🇪

    The inclusive radiative decay of the B meson is known to provide strong constraints on many popular extensions of the Standard Model. Such constraints crucially depend on precision of the Standard Model predictions. One of the main contributions to the theoretical uncertainty is due to certain Next-to-Next-to-Leading Order QCD corrections whose values at the physical charm quark mass m_c have been estimated using interpolation between the m_c=0 and m_c >> m_b limits. A direct determination of such corrections at the physical value of m_c requires calculating hundreds of two-scale four-loop propagator diagrams with unitarity cuts. Applying the integration-by-parts method, we express the corrections in terms of master integrals. Asymptotic expansions of these integrals at m_c >> m_b serve as boundary conditions for differential equations in z=m_c^2/m_b^2 that are being numerically solved. Here, we present our final results for the diagrams involving massless and massive fermion loops on the gluon lines. For the two-body cuts, we confirm the analytical expressions and/or numerical fits that are already present in the literature. In the four-body case, we make the correction complete by including several diagrams that have previously been only estimated using interpolation in m_c. We also report the status of the ongoing calculation of the remaining diagrams where no closed fermion loops on the gluon lines are present.

    hep-phPoS(2019)·3 citations
  4. 04*

    Galactic Condensates composed of Multiple Axion Species

    Joshua Eby🇮🇱 · Madelyn Leembruggen🇺🇸 · Lauren Street🇺🇸 · Peter Suranyi🇺🇸 · L.C.R. Wijewardhana🇺🇸

    Ultralight scalar dark matter has been proposed to constitute a component of dark matter, though the minimal scenarios have increasingly become constrained. In this work, we analyze scenarios where the dark matter consists of more than one ultralight boson, each with different masses. This potentially leads to formation of gravitationally-bound Bose-Einstein condensates with structures that are very different from condensates composed of a single scalar field. By generalizing from the well-understood single-flavor case, we explore a large range of input parameters, subject to stability criteria, and determine the allowed parameter space for two-flavor condensates as a function of particle physics parameters, paying particular attention to cases where such condensates could compose galactic cores. We also analyze single-flavor condensates subject to external gravity from massive inner bodies and find that such systems may mimic the size of galactic cores as well.

    hep-phastro-ph.COhep-thJCAP(2020)·24 citations
  5. 05*

    A global analysis strategy to resolve neutrino NSI degeneracies with scattering and oscillation data

    Bhaskar Dutta🇺🇸 · Rafael F. Lang🇺🇸 · Shu Liao🇺🇸 · Samiran Sinha🇺🇸 · Louis Strigari🇺🇸 · Adrian Thompson🇺🇸

    Neutrino non-standard interactions (NSI) with the first generation of standard model fermions can span a parameter space of large dimension and exhibit degeneracies that cannot be broken by a single class of experiment. Oscillation experiments, together with neutrino scattering experiments, can merge their observations into a highly informational dataset to combat this problem. We consider combining neutrino-electron and neutrino-nucleus scattering data from the Borexino and COHERENT experiments, including a projection for the upcoming coherent neutrino scattering measurement at the CENNS-10 liquid argon detector. We extend the reach of these data sets over the NSI parameter space with projections for neutrino scattering at a future multi-ton scale dark matter detector and future oscillation measurements from atmospheric neutrinos at the Deep Underground Neutrino Experiment (DUNE). In order to perform this global analysis, we adopt a novel approach using the copula method, utilized to combine posterior information from different experiments with a large, generalized set of NSI parameters. We find that the contributions from DUNE and a dark matter detector to the Borexino and COHERENT fits can improve constraints on the electron and quark NSI parameters by up to a factor of 2 to 3, even when relatively many NSI parameters are left free to vary in the analysis.

    hep-phJHEP(2020)·50 citations
  6. 06*

    Triangle singularity in the reaction and sensitivity to the mass

    Shuntaro Sakai🇨🇳 · Eulogio Oset🇪🇸 · Feng-Kun Guo🇨🇳

    We have done a study of the reaction by means of a triangle mechanism via the chain of reactions: ; ; . We show that this mechanism generates a triangle singularity in the invariant mass for a very narrow window of the mass, around the present measured values, and show that the peak positions and the shape of the mass distributions are sensitive to the mass, such that a measurement of the reaction can serve to improve on the present values of this mass. In particular, we point out that the mass relative to the threshold may be extracted from the asymmetry of the line shape.

    hep-phPRD(2020)·31 citations
  7. 08*

    The studies on at the next-to-leading-order QCD accuracy

    Zhan Sun🇨🇳

    In this paper, we carry out the next-to-leading-order (NLO) studies on via the color-singlet (CS) state. We find the newly calculated NLO QCD corrections to this process can significantly influence its leading-order (LO) results, and greatly improve the dependence on the renormalization scale. By including the considerable feeddown contributions, the branching ratio is predicted to be , which can reach up to of the LO predictions given by the CS dominant process . Moreover, also seriously affect the CS predictions on the energy distributions, especially when is relatively small. In summary, for the inclusive productions in decay, besides , the gluon radiation process can provide indispensable contributions as well.

    hep-phEPJC(2020)·5 citations
  8. 09*

    Possibility of charmoniumlike state as state

    Ming-Xiao Duan🇨🇳 · Si-Qiang Luo🇨🇳 · Xiang Liu🇨🇳 · Takayuki Matsuki🇯🇵

    In this work, we seriously discuss whether can be treated as a state. Based on an unquenched quark model, we give the mass spectrum of the states, where there are no free input parameters in our calculation. Our result shows that the mass gap between and can reach 13 MeV, which can reproduce the mass difference between and . Additionally, the calculated masses of and are consistent with experimental values of and , respectively. Besides, giving the mass spectrum analysis to support as , we also calculate the width of with the same framework, which is also consistent with the experimental data of . Thus, the possibility of charmoniumlike state as state is further enforced.

    hep-phhep-exPRD(2020)·46 citations
  9. 10*

    Constraints on anomalous quartic gauge couplings via production at the LHC

    Yu-Chen Guo🇨🇳 · Ying-Ying Wang🇨🇳 · Ji-Chong Yang🇨🇳 · Chong-Xing Yue🇨🇳

    The vector boson scattering at the Large Hadron Collider (LHC) is sensitive to anomalous quartic gauge couplings (aQGCs). In this paper, we investigate the aQGC contribution to production at the LHC with TeV in the context of an effective field theory (EFT). The unitarity bound is applied as a cut on the energy scale of this production process, which is found to have significant suppressive effects on the signals. To enhance the statistical significance, we analyse the kinematic and polarization features of the aQGC signals in detail. We find that the polarization effects induced by the aQGCs are unique and can discriminate the signals from the SM backgrounds well. With the proposed event selection strategy, we obtain the constraints on the coefficients of dimension-8 operators with current luminosity. The results indicate that the process is powerful for searching for the and operators.

    hep-phCPC(2020)·29 citations
  10. 11*

    On the beta-decay of the accelerated proton and neutrino oscillations: a three-flavor description with CP violation

    Massimo Blasone🇮🇹 · Gaetano Lambiase🇮🇹 · Giuseppe Gaetano Luciano🇮🇹 · Luciano Petruzziello🇮🇹

    The (inverse) beta-decay of uniformly accelerated protons (p -> n + e+ + ne) has been recently analyzed in the context of two-flavor neutrino mixing and oscillations. It has been shown that the decay rates as measured by an inertial and comoving observer are in agreement, provided that: i) the thermal nature of the accelerated vacuum (Unruh effect) is taken into account; ii) the asymptotic behavior of neutrinos is described through flavor (rather than mass) eigenstates; iii) the Unruh radiation is made up of oscillating neutrinos. Here we extend the above considerations to a more realistic scenario including three generations of Dirac neutrinos. By following the outlined recipe, we find that the equality between the two rates still holds true, confirming that mixing is perfectly consistent with the General Covariance of Quantum Field Theory. Notably, we prove that the analysis of CP violation in neutrino oscillations provides a further solid argument for flavor states as fundamental representation of asymptotic neutrino states. Our approach is finally discussed in comparison with the other treatments appeared in literature.

    hep-phEPJC(2020)·36 citations
  11. 12*

    Explicit parity violation in models

    Henry Diaz🇵🇪 · E. Castillo-Ruiz🇵🇪 · O. P. Ravinez🇵🇪 · V. Pleitez🇧🇷

    Here we propose models with electroweak gauge symmetry in which parity (or charge conjugation) is broken explicitly and the interactions of left- and right-handed fermions are completely different from each other at any energy scale. In these sort of models there is no restoration of parity at high energies. However, as in all left-right symmetric models, the electroweak charged interactions of quarks and leptons appear to be only left-handed at low energies, because the right-handed interactions are suppressed by the mass of the respective charged vector bosons and/or because these interactions may be much weaker than the left-handed ones.

    hep-phJ.Phys.G(2021)·5 citations
  12. 13*

    Non-perturbative renormalization of the average color charge and multi-point correlators of color charge from a non-Gaussian small- action

    Andre V. Giannini🇧🇷 · Yasushi Nara🇯🇵

    The McLerran-Venugopalan (MV) model is a Gaussian effective theory of color charge fluctuations at small- in the limit of large valence charge density, {\it i}.{\it e}., a large nucleus made of uncorrelated color charges. In this work, we explore the effects of the first non-trivial (even C-parity) non-Gaussian correction on the color charge density to the MV model ("quartic" term) in SU(2) and SU(3) color group in the non-perturbative regime. We compare our (numerical) non-perturbative results to (analytical) perturbative ones in the limit of small or large non-Gaussian fluctuations. The couplings in the non-Gaussian action, for the quadratic and for the quartic term, need to be renormalized in order to match the two-point function in the Gaussian theory. We investigate three different choices for the renormalization of these couplings: i) is proportional to a power of ; ii) is kept constant and iii) is kept constant. We find that the first two choices lead to a scenario where the small- action evolves towards a theory dominated by large non-Gaussian fluctuations, regardless of the system size, while the last one allows for controlling the deviations from the MV model.

    hep-phnucl-thNPA(2021)·5 citations
  13. 14*

    The Observation of Jet Azimuthal Angular Decorrelation at FCC-ep

    I. Hos🇹🇷 · S. Kuday🇹🇷 · H. Saygın🇹🇷

    Higher collision energies at future colliders may eventually lead to the falsification of standard fixed-order perturbation theory and linear evolutions due to non-linear structure of QCD at small-x. New physics researches that is strictly based on accurate jet measurements will undoubtedly have this observation known as BFKL effect via angular jet decorrelations taking into account the Mueller-Navelet jets. As one of the frontier colliders, FCC-ep, has a great observation potential on parton densities through asymmetrical collisions. We aim to test the observability of azimuthal angular jet decorrelations with the recent event generators (HERWIG, PYTHIA) at the particle level for FCC-ep centre of mass energies 3.5 TeV in proton-electron collisions. Jets are reconstructed by the Anti-kT algorithm (R = 0.5), with and selected in the range of |y|<6. Relevant rapidity regions has been analyzed with the azimuthal-angle difference between Mueller-Navelet Jets () in the rapidity seperation () and the distributions of cosn() are presented in comparison as the result.

    hep-phInt.J.Mod.Phys.A(2023)·0 citations
  14. 15*

    Scalegenesis and fermionic dark matters in the flatland scenario

    Yu Hamada🇯🇵 · Koji Tsumura🇯🇵 · Masatoshi Yamada🇩🇪

    We propose an extension of the standard model with Majorana-type fermionic dark matters based on the flatland scenario where all scalar coupling constants, including scalar mass terms, vanish at the Planck scale, i.e. the scalar potential is flat above the Planck scale. This scenario could be compatible with the asymptotic safety paradigm for quantum gravity. We search the parameter space so that the model reproduces the observed values such as the Higgs mass, the electroweak vacuum and the relic abundance of dark matter. We also investigate the spin-independent elastic cross section for the Majorana fermions and a nucleon. It is shown that the Majorana fermions as dark matter candidates could be tested by dark matter direct detection experiments such as XENON, LUX and PandaX-II. We demonstrate that within the minimal setup compatible with the flatland scenario at the Planck scale or asymptotically safe quantum gravity, the extended model could have a strong predictability.

    hep-phhep-thEPJC(2020)·43 citations
  15. 16*

    A Study of Excited States in Hypercentral Constituent Quark Model via Artificial Neural Network

    Halil Mutuk🇹🇷

    In this work, we have obtained mass spectra, radiative decay widths and strong decay widths of newly observed excited states, i.e. , , , and . Mass spectrum is obtained in Hypercentral Constituent Quark Model (hCQM) by solving six-dimensional nonrelativistic Schrödinger equation via Artificila Neural Network (ANN). In this respect, radiative decay widhts are calculated by a generalization of a framework from meson to baryon. Also, strong decay widths of the low-lying states within model are calculated. Obtained results are presented with the comparison of available experimental data and other theoretical studies.

    hep-phEPJA(2020)·18 citations
  16. 17*

    Covariant Spin Kinetic Theory I: Collisionless Limit

    Yu-Chen Liu🇨🇳 · Kazuya Mameda🇨🇳 · Xu-Guang Huang🇨🇳

    We develop a covariant kinetic theory for massive fermions in curved spacetime and external electromagnetic field based on quantum field theory. We derive four coupled semi-classical kinetic equations accurate at , which describe the transports of particle number and spin degrees of freedom. The relation with the chiral kinetic theory is discussed. As an application, we study the spin polarization in the presence of finite Riemann curvature and electromagnetic field in both local and global equilibrium states.

    hep-phcond-mat.mes-hallhep-thnucl-thCPC(2020)·116 citations
  17. 18*

    Back-reaction in strong field QED: a toy model

    Robin Ekman🇬🇧 · Anton Ilderton🇬🇧

    As a toy model for QED in strong background fields, we consider the impact of back-reaction and loop effects on scattering processes in quantum optics. We show that neglecting back-reaction misses qualitative and quantitative features of strong-field physics. We are able to study an analogue of the Narozhny-Ritus conjecture on the scaling of higher loop diagrams with intensity: we prove that there is no corresponding behaviour in our model. Implications for QED are identified and discussed.

    hep-phPRD(2020)·12 citations
  18. 19*

    QCD calculations of radiative heavy meson decays with subleading power corrections

    Hua-Dong Li🇨🇳 · Cai-Dian Lü🇨🇳 · Chao Wang🇨🇳 · Yu-Ming Wang🇨🇳 · Yan-Bing Wei🇨🇳

    We revisit QCD calculations of radiative heavy meson decay form factors by including the subleading power corrections from the twist-two photon distribution amplitude at next-to-leading-order in with the method of the light-cone sum rules (LCSR). The desired hard-collinear factorization formula for the vacuum-to-photon correlation function with the interpolating currents for two heavy mesons is constructed with the operator-product-expansion technique in the presence of evanescent operators. Applying the background field approach, the higher twist corrections from both the two-particle and three-particle photon distribution amplitudes are further computed in the LCSR framework at leading-order in QCD, up to the twist-four accuracy. Combining the leading power "point-like" photon contribution at tree level and the subleading power resolved photon corrections from the newly derived LCSR, we update theory predictions for the nonperturbative couplings describing the electromagnetic decay processes of the heavy mesons , , (with ). Furthermore, we perform an exploratory comparisons of our sum rule computations of the heavy-meson magnetic couplings with the previous determinations based upon different QCD approaches and phenomenological models.

    hep-phhep-exhep-latJHEP(2020)·49 citations
  19. 20*

    Exclusive and diffractive production in collisions at the LHC, HE -- LHC and FCC

    R. O. Coelho🇧🇷 · V. P. Goncalves🇧🇷 · D. E. Martins🇧🇷 · M. S. Rangel🇧🇷

    In this paper we present a detailed analysis of the contribution of the Light -- by -- Light (LbL), Durham and double diffractive processes for the diphoton production in ultraperipheral collisions at the Large Hadron Collider (LHC), High -- Energy LHC (HE -- LHC) and Future Circular Collider (FCC). The acceptance of the central and forward LHC detectors is taken into account and predictions for the invariant mass, rapidity, transverse momentum and acoplanarity distributions are presented. Our results indicate that the contribution of the Durham and double diffractive processes can be strongly suppressed by the exclusivity cuts, which will allow to perform a precise analysis of the LbL scattering, as well the search of beyond Standard Model physics in this final state.

    hep-phhep-exEPJC(2020)·13 citations
  20. 21*

    Relativistic dissipative spin dynamics in the relaxation time approximation

    Samapan Bhadury🇮🇳 · Wojciech Florkowski🇵🇱 · Amaresh Jaiswal🇮🇳 · Avdhesh Kumar🇵🇱 · Radoslaw Ryblewski🇵🇱

    The concept of the Wigner function is used to construct a semi-classical kinetic theory describing the evolution of the axial-current phase-space density of spin-1/2 particles in the relaxation time approximation. The resulting approach can be used to study spin-polarization effects in relativistic matter, in particular, in heavy-ion collisions. An expression for the axial current based on the classical treatment of spin is also introduced and we show that it is consistent with earlier calculations using Wigner functions. Finally, we derive non-equilibrium corrections to the spin tensor, which are used to define, for the first time, the structure of spin transport coefficients in relativistic matter.

    hep-phnucl-thPLB(2021)·178 citations
  21. 22*

    Implications of extra dimensions on the effective charge and the beta function in quantum electrodynamics

    E. Martínez-Pascual🇲🇽 · G. Nápoles-Cañedo🇲🇽 · H. Novales-Sánchez🇲🇽 · A. Sierra-Martínez🇲🇽 · J. J. Toscano🇲🇽

    A comprehensive analysis on the photon self-energy, the fermion self-energy, and the fermion vertex function is presented at one loop in the context of quantum electrodynamics (QED) with 1 extra dimension. In 5-dimensional theories, characterized by an infinite number of Kaluza-Klein fields, one-loop amplitudes involve discrete as well as continuous sums, , that could diverge. Using dimensional regularization, we express such sums as products of gamma and Epstein functions, both defined on the complex plane, with divergences arising from poles of these functions in the limit as . Using the analytical properties of the Epstein function, we show that the ultraviolet divergences generated by the Kaluza-Klein sums can be consistently renormalized, which means that the corresponding renormalized quantities reduce to the usual ones of QED at the limit of a very large compactification scale . The main features of QED at the one-loop level were studied. We use the mass-dependent -scheme to calculate, in QED with an arbitrary number of extra dimensions, a beta function fulfilling all desirable physical requirements. We argue that in this type of theories, with a large mass spectrum covering a wide energy range, beta functions should not be calculated by using mass-independent renormalization schemes. We show that the beta function is finite for any energy . In particular, it reduces to the usual QED result for and vanishes for , with the usual fermion mass. Throughout the work, the decoupling nature of all our results obtained from the analytical properties of the Epstein function is stressed.

    hep-phPRD(2020)·6 citations
  22. 23*

    The one-loop amplitudes for Higgs + 4 partons with full mass effects

    Lucy Budge🇬🇧 · John M. Campbell🇺🇸 · Giuseppe De Laurentis🇬🇧 · R. Keith Ellis🇬🇧 · Satyajit Seth🇮🇳

    We present compact analytic formulae for the one-loop amplitudes for Higgs + 4 parton scattering, , and , mediated by a loop of massive coloured quarks. We exploit the correspondence with a theory in which a massive coloured scalar circulates in the loop to avoid a proliferation in the number of terms in the result. In addition, we use momentum twistors and high precision numerical evaluations to simplify the expressions. The analytic results in this paper, in terms of spinor products, allow construction of an efficient numerical program to calculate the amplitude.

    hep-phJHEP(2020)·37 citations
  23. 24*

    Jet quenching and medium response in high-energy heavy-ion collisions: a review

    Shanshan Cao🇺🇸 · Xin-Nian Wang🇨🇳

    Jet quenching has been used successfully as a hard probe to study properties of the quark-gluon plasma (QGP) in high-energy heavy-collisions at both the Relativistic Heavy-Ion Collider (RHIC) and the Large Hadron Collider (LHC). We will review recent progresses in theoretical and phenomenological studies of jet quenching with jet transport models. Special emphasis is given to effects of jet-induced medium response on a wide variety of experimental measurements and their implication on extracting transport properties of the QGP in heavy-ion collisions.

    hep-phnucl-thRept.Prog.Phys.(2021)·250 citations
  24. 25*

    Co-SIMP Miracle

    Juri Smirnov🇺🇸 · John F. Beacom🇺🇸

    We present a new mechanism for thermally produced dark matter, based on a semi-annihilation-like process, , with intriguing consequences for the properties of dark matter. First, its mass is low, GeV (but keV to avoid structure-formation constraints). Second, it is strongly interacting, leading to kinetic equilibrium between the dark and visible sectors, avoiding the structure-formation problems of models. Third, in the process, one dark matter particle is consumed, giving the standard-model particle a monoenergetic recoil. We show that this new scenario is presently allowed, which is surprising (perhaps a "minor miracle"). However, it can be systematically tested by novel analyses in present and near-term experiments. In particular, the Co-SIMP model for thermal-relic dark matter can explain the XENON1T excess.

    hep-phastro-ph.COhep-exPRL(2020)·106 citations
  25. 26*

    Natural Supersymmetry: Status and Prospects

    Xerxes Tata🇺🇸

    The realization that supersymmetry (SUSY), if softly broken at the weak scale, can stabilize the Higgs sector led many authors to explore the role it may play in particle physics. It was widely anticipated that superpartners would reveal themselves once the TeV scale was probed in high energy collisions. Experiments at the LHC have not yet revealed any sign for direct production of superpartners, or for any other physics beyond the Standard Model. This has led to some authors to question whether weak scale SUSY has a role to play in stabilizing the Higgs sector. We show that SUSY models with just the minimal particle content may well be consistent with data and simultaneously serve to stabilize the Higgs sector, if model parameters generally regarded as independent turn out to be appropriately correlated. In our view, it would be premature to ignore this possibility, given that we do not understand the underlying mechanism of SUSY breaking. We advocate using the electroweak scale quantity, , to determine whether a given SUSY spectrum might arise from a theory with low fine-tuning, even when the parameters correlations mentioned above are present. We find that all such models contain light higgsinos and that this leads to the possibility of new strategies for searching for SUSY. We discuss phenomenological implications of these models for SUSY searches at the LHC and its luminosity and energy upgrades, as well as at future electron-positron colliders. We conclude that natural SUSY, defined as no worse than a part in 30 fine-tuning, will not escape detection at a collider operating at 27~TeV and an integrated luminosity of 15~ab, or at an electron-positron collider with a centre-of-mass energy of 600~GeV.

    hep-phhep-exEur.Phys.J.ST(2020)·29 citations
  26. 27*

    A New Approach to Mass and Radius of Neutron Stars with Supernova Neutrinos

    Ken'ichiro Nakazato🇯🇵 · Hideyuki Suzuki🇯🇵

    Neutron stars are formed in core-collapse supernova explosions, where a large number of neutrinos are emitted. In this paper, supernova neutrino light curves are computed for the cooling phase of protoneutron stars, which lasts a few minutes. In the numerical simulations, 90 models of the phenomenological equation of state with different incompressibilities, symmetry energies, and nucleon effective masses are employed for a comprehensive study. It is found that the cooling timescale is longer for a model with a larger neutron star mass and a smaller neutron star radius. Furthermore, a theoretical expression of the cooling timescale is presented as a function of the mass and radius and it is found to describe the numerical results faithfully. These findings suggest that diagnosing the mass and radius of a newly formed neutron star using its neutrino signal is possible.

    astro-ph.HEhep-phnucl-thApJ(2020)·32 citations
  27. 28*

    The Quenched in Nuclei and Emergent Scale Symmetry in Baryonic Matter

    Yong-Liang Ma🇨🇳 · Mannque Rho🇫🇷

    A recent RIKEN experiment on the quenched in the superallowed Gamow-Telller transition from Sn indicates a role of scale anomaly encoded in the anomalous dimension of the gluonic stress tensor . This observation provides a support to the notion of hidden scale symmetry emerging by strong nuclear correlations with an IR fixed point realized -- in the chiral limit -- in the Nambu-Goldstone mode. We suggest there is an analogy in the way scale symmetry manifests in nuclear medium to the continuity from the unitarity limit at low density (in light nuclei) to the dilaton limit at high density (in compact stars). In between the limits, say, at normal nuclear matter density, the symmetry is not visible, hence hidden.

    nucl-thhep-phPRL(2020)·30 citations
  28. 29*

    Impact of longitudinal bulk viscous effects to heavy quark transport in a strongly magnetized hot QCD medium

    Manu Kurian🇮🇳 · Vinod Chandra🇮🇳 · Santosh K. Das🇮🇳

    The effects of longitudinal bulk viscous pressure on the heavy quark dynamics have been estimated in a strongly magnetized quark-gluon plasma within the Fokker-Planck approach. The bulk viscous modification to the momentum distribution of bulk degrees of freedom has been obtained in the presence of a magnetic field while incorporating the realistic equation of state of the hot magnetized QCD medium. As the magnetic field breaks the isotropy of the medium, the analysis is done along the directions longitudinal and transverse to the field. The longitudinal bulk viscous contribution is seen to have sizable effects in the heavy quark momentum diffusion in the magnetized medium. The dependence of higher Landau levels and the equation of state on the viscous correction to the heavy quark transport has been explored in the analysis.

    nucl-thhep-phPRD(2020)·25 citations
  29. 30*

    Local Spin Polarization in 200 GeV Au+Au and 2.76 TeV Pb+Pb Collisions

    Hong-Zhong Wu🇨🇳 · Long-Gang Pang🇺🇸 · Xu-Guang Huang🇨🇳 · Qun Wang🇨🇳

    We calculated the azimuthal angle dependence of the local spin polarization of hyperons in 200 GeV Au+Au and 2.76 TeV Pb+Pb collisions in the framework of the (3+1)D viscous hydrodynamic model CLVisc with AMPT initial conditions encoding initial orbital angular momenta. We find that the azimuthal angle dependence of the hyperon polarization strongly depends on the choice of the spin chemical potential . With chosen to be proportional to the temperature vorticity, our simulation shows coincidental results with the recent measurements at RHIC.

    nucl-thhep-phNPA(2021)·19 citations
  30. 31*

    Probing Dark Matter with Future CMB Measurements

    Junsong Cang🇨🇳 · Yu Gao🇨🇳 · Yin-Zhe Ma🇿🇦

    Dark Matter (DM) annihilation and decay during the Dark Ages can affect the cosmic ionization history and leave imprints in the Cosmic Microwave Background (CMB) anisotropy spectra. CMB polarization anisotropy can be sensitive to such energy injection at higher redshifts and help reducing degeneracy with primordial spectral parameters in CDM and astrophysical ionization processes during reionization. In light of a number of upcoming CMB polarization experiments, such as AdvACTPol, AliCPT, CLASS, Simons Observatory, Simons Array, SPT-3G, we estimate their prospective sensitivity in probing dark matter annihilation and decay signals. We find that future missions have 95\% C.L. projected limits on DM decay and annihilation rates to orders of and respectively, significantly improving the sensitivity to DM from current experimental bounds.

    astro-ph.COhep-phPRD(2020)·52 citations
  31. 32*

    Beam-spread determination for luminosity measurement at CEPC

    Ivan Smiljanic🇷🇸 · Ivanka Bozovic-Jelisavcic🇷🇸 · Goran Kacarevic🇷🇸

    Any asymmetry in energy of the colliding beams will lead to a longitudinal boost of the center-of-mass frame of colliding particles w.r.t. the laboratory frame and consequently to the counting loss in luminometer due to the loss of colinearity of Bhabha final states. At CEPC running at the Z0 pole, asymmetry in energy of the colliding beams should be known as well as 12.5% of the beam-spread, in order to control the uncertainty of Bhabha count at the level of 0.01%. Here we discuss the method, initially proposed for FCCee, to determine variation of the beam-spread from the measurement of the effective center-of-mass energy in collisions.

    hep-exhep-phphysics.comp-ph0 citations
  32. 33*

    Combining Full-Shape and BAO Analyses of Galaxy Power Spectra: A 1.6% CMB-independent constraint on H0

    Oliver H.E. Philcox🇺🇸 · Mikhail M. Ivanov🇺🇸 · Marko Simonović🇨🇭 · Matias Zaldarriaga🇺🇸

    We present cosmological constraints from a joint analysis of the pre- and post-reconstruction galaxy power spectrum multipoles from the final data release of the Baryon Oscillation Spectroscopic Survey (BOSS). Geometric constraints are obtained from the positions of BAO peaks in reconstructed spectra, analyzed in combination with the unreconstructed spectra in a full-shape (FS) likelihood using a joint covariance matrix, giving stronger parameter constraints than FS-only or BAO-only analyses. We introduce a new method for obtaining constraints from reconstructed spectra based on a correlated theoretical error, which is shown to be simple, robust, and applicable to any flavor of density-field reconstruction. Assuming CDM with massive neutrinos, we analyze data from two redshift bins and obtain constraints on the Hubble constant , using only a single prior on the current baryon density from Big Bang Nucleosynthesis (BBN) and no knowledge of the power spectrum slope . This gives , with the inclusion of BAO data sharpening the measurement by , representing one of the strongest current constraints on independent of cosmic microwave background data. Restricting to the best-fit slope from Planck (but without additional priors on the spectral shape), we obtain a measurement of . We find strong constraints on the cosmological parameters from a joint analysis of the FS, BAO, and Planck data. This sets new bounds on the sum of neutrino masses (at confidence) and the effective number of relativistic degrees of freedom , though contours are not appreciably narrowed by the inclusion of BAO data.

    astro-ph.COgr-qchep-phJCAP(2020)·263 citations

* Reconstructed cohort: no mailing for this day survives in the archive. Papers are grouped by their submission times and arXiv's announcement cut-off, assuming announcement without delay; positions follow identifier order. Validated at ~91% exact-day agreement against the archived era.