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High Energy Physics - Phenomenology

New submissions

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New submissions for Mon, 6 May 24

[1]  arXiv:2405.01648 [pdf, other]
Title: Electric dipole moments of charged leptons in models with pseudo-Dirac sterile fermions
Comments: 18 pages, 7 figures
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Experiment (hep-ex)

In this work, we address the impact of a small lepton number violation on charged lepton electric dipole moments - EDMs. Low-scale seesaw models protected by lepton number symmetry and leading to pseudo-Dirac pairs in the neutrino heavy spectrum provide a natural explanation for the smallness of neutrino masses with potentially testable consequences. Among which, it was thought that the small mass gap in each pair of pseudo-Dirac neutrinos may induce important contribution to the charged lepton EDMs. Recently, it has been shown that the contribution from some of the Feynman diagrams to charged lepton EDMs exactly cancel by virtue of the Ward-Takahashi identity in quantum electrodynamics. We thus consider here the Standard Model minimally extended with pairs of pseudo-Dirac sterile fermions and derive the complete analytical formula at two loops for the charged lepton EDMs. In addition, we numerically evaluate the order of the predicted EDMs consistent with the experimental bounds and constraints such as neutrino oscillation data, charged lepton flavour violating processes, sterile neutrino direct searches, meson decays, sterile neutrino decays, and cosmological and astrophysical observations. We find that, in the minimal setup accommodating neutrino data (masses and mixings) with only two pseudo-Dirac pairs, the predicted electron EDM is $\mathcal{O}(10^{-36})~e\hspace{0.05cm}\mathrm{cm}$, at most, which is much smaller than the current experimental bound and even future sensitivity. Hopefully, the electron EDM might reach future sensitivity, once extra pseudo-Dirac neutrinos are taken into account. The analytical formulae we derive are generic to any model involving pseudo-Dirac pairs in the heavy neutrino spectrum.

[2]  arXiv:2405.01679 [pdf, other]
Title: Enhanced primordial gravitational waves from a stiff post-inflationary era due to an oscillating inflaton
Comments: 21 pages, 6 figures
Subjects: High Energy Physics - Phenomenology (hep-ph)

We investigate two classes of inflationary models, which lead to a stiff period after inflation that boosts the signal of primordial gravitational waves (GWs). In both families of models studied, we consider an oscillating scalar condensate, which when far away from the minimum it is overdamped by a warped kinetic term, a la $\alpha$-attractors. This leads to successful inflation. The oscillating condensate is in danger of becoming fragmented by resonant effects when non-linearities take over. Consequently, the stiff phase cannot be prolonged enough to enhance primordial GWs at frequencies observable in the near future for low orders of the envisaged scalar potential. However, this is not the case for a higher-order scalar potential. Indeed, we show that this case results in a boosted GW spectrum that overlaps with future observations without generating too much GW radiation to de-stabilise Big Bang Nucleosynthesis. For example, taking $\alpha={\cal O}(1)$, we find that the GW signal can be safely enhanced up to $\Omega_{\rm GW}(f)\sim 10^{-11}$ at frequency $f\sim 10^2\,$Hz, which will be observable by the Einstein Telescope (ET). Our mechanism ends up with a characteristic GW spectrum, which if observed, can lead to the determination of the inflation energy scale, the reheating temperature and the shape (steepness) of the scalar potential around the minimum.

[3]  arXiv:2405.01712 [pdf, other]
Title: Multiplicity dependence of the $p_T$-spectra for identified particles and its relationship with partonic entropy
Comments: 10 pages, 6 figures
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Experiment (hep-ex)

We investigate the multiplicity dependence of the transverse momentum $p_T$ spectra of hadrons produced in high-energy collisions. We propose that the partonic distribution be parameterized by its non-extensive entropy and the parton saturation scale $Q_s(x)$. These two variables can be identified from the produced charged hadron distributions and provide important information on the gluon dynamics at the moment of interaction. From this perspective we interpret data from different ALICE multiplicity classes at $\sqrt{s}= 13$ TeV and $\sqrt{s}= 5.02$ TeV. A multiplicity dependent scaling function is presented and the dependence of the interaction area on multiplicity is also investigated.

[4]  arXiv:2405.01782 [pdf, other]
Title: Exploring hadronic de-excitation via Lepton Flavor Violation
Comments: 6 pages, 5 figures
Subjects: High Energy Physics - Phenomenology (hep-ph)

In this work, we consider a particular case of hadronic de-excitation via lepton flavor violation (LFV). Namely, $\rho^\prime \to \rho \mu e$ decay, described considering effective dim-5 and dim-7 operators. Using the current bounds for the couplings from direct processes, we exhibit the different features in the dilepton invariant mass distribution and the branching ratios, depending on the effective operator. The results, although heavily suppressed, show that they may be useful to impose constraints on individual contributions and help to disentangle them, when complemented with observables from nuclei. Our particular case can be taken as an initial step to look for other hadronic states, such as in quarkonia, where the de-excitation can have enough energy to search for LFV involving the $\tau$ lepton.

[5]  arXiv:2405.01900 [pdf, ps, other]
Title: Excited electron production at the SPPC-based ep colliders via contact interactions
Comments: 21 pages, 9 Figures, 5 Tables
Subjects: High Energy Physics - Phenomenology (hep-ph)

If a linear electron accelerator is installed into the SPPC (Super Proton-Proton Collider) complex, ep collision options will be available in addition to pp collisions. We consider the production of excited electrons with spin-1/2 at the future SPPC-based electron-proton colliders with center-of-mass energies of $8.44$, $11.66$, $26.68$ and $36.88$ TeV. In the $ep\rightarrow e^{\star}X\rightarrow e\gamma X$ signal process, excited electrons are produced by contact interactions and decay into the photon channel by gauge interactions. Taking into account the corresponding background process, the pseudorapidity and transverse momentum distributions of the final state particles are plotted. We reported the discovery, observation and exclusion mass limits of excited electrons by applying appropriate kinematical cuts best suited for amplify the signal of the excited electron signature. We also investigated the highest achievable values of the compositeness scale for the discovery of excited electrons at these colliders.

[6]  arXiv:2405.02009 [pdf, other]
Title: On the (in)consistency of perturbation theory at finite temperature
Comments: 21 pages, 8 figures; Figure data attached
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Lattice (hep-lat); High Energy Physics - Theory (hep-th); Nuclear Theory (nucl-th)

A well-known difficulty of perturbative approaches to quantum field theory at finite temperature is the necessity to address theoretical constraints that are not present in the vacuum theory. In this work, we use lattice simulations of scalar correlation functions in massive $\phi^{4}$ theory to analyse the extent to which these constraints affect the perturbative predictions. We find that the standard perturbative predictions deteriorate even in the absence of infrared divergences at relatively low temperatures, and that this is directly connected to the analytic structure of the propagators used in the expansion. This suggests that the incorporation of non-perturbative thermal effects in the propagators is essential for a consistent perturbative formulation of scalar quantum field theories at finite temperature. By utilising the spectral constraints imposed on finite-temperature correlation functions, we explore how these effects manifest themselves in the lattice data, and discuss why the presence of distinct thermoparticle excitations provides a potential resolution to these issues.

[7]  arXiv:2405.02084 [pdf, other]
Title: Muon g-2, Long-Range Muon Spin Force, and Neutrino Oscillations
Comments: 8 pages, 2 figures
Subjects: High Energy Physics - Phenomenology (hep-ph)

Recent studies have proposed using a geocentric muon spin force to account for the $(g-2)_\mu$ anomaly, with the long-range force mediator being a light axion-like particle. The mediator exhibits a CP-violating scalar coupling to nucleons and a normal derivative coupling to muons. Due to the weak symmetry, this axion inevitably couples to neutrinos, providing potential impact on neutrino oscillations. By utilizing neutrino data from BOREXINO, IceCube DeepCore, Super-Kamiokande, and SNO, we have identified that atmospheric neutrino data can impose stringent constraints on the long-range muon spin force model and the $(g-2)_\mu$ parameter space. Additionally, solar neutrino data places a strong limit on the model but provides a weaker constraint on the $(g-2)_\mu$ parameter space due to a sign mismatch. With optimized data analysis techniques and the potential from future experiments, such as JUNO, Hyper-Kamiokande, SNO+, and IceCube PINGU, there exists a promising opportunity to achieve even greater sensitivities. Indeed, neutrino oscillations offer a robust and distinctive cross-check for the model, offering stringent constraints on the $(g-2)_\mu$ parameter space.

[8]  arXiv:2405.02104 [pdf, other]
Title: Searching for a new light gauge boson with axial couplings in muon beam dump experiments
Subjects: High Energy Physics - Phenomenology (hep-ph)

We present a formalism for new $U(1)$ interactions involving weak hypercharge, baryon, and lepton numbers, and a possible axial symmetry generator $F_A$ in the presence of a second Brout-Englert-Higgs doublet. The resulting $U$ boson, after mixing with the $Z$, interpolates between a generalised dark photon, a dark $Z$, and an axially coupled gauge boson. We especially focus on the axial couplings originating from $F_A$ or from mixing with the $Z$, determined by the scalar sector via parameters like $\tan\beta$ and the v.e.v. of an extra dark singlet. We explore the distinctive features of axially coupled interactions, especially in the ultrarelativistic limit, where the $U$ boson behaves much as an axion-like particle, with enhanced interactions to quarks and leptons. This enhancement is particularly relevant for future muon beam dump experiments, since the muon mass considerably increases the effective coupling, proportional to $2m_\mu/m_U$, compared to analogous experiments with electrons. We also analyse the shape of the expected beam dump exclusion or discovery regions, influenced by $U$ boson interactions and the experiment geometry. Different situations are considered, limited in particular by cases for which the $U$ decays before reaching the detector, or has too small couplings to produce detectable events. We also compare to vectorially coupled bosons and axion-like pseudoscalars, highlighting the importance of understanding the parameter space for future experiment design and optimisation.

[9]  arXiv:2405.02116 [pdf, other]
Title: Intriguing aspects of light baryon resonances
Comments: Proceedings for the XLV Symposium on Nuclear Physics, held in Cocoyoc, Morelos, Mexico
Subjects: High Energy Physics - Phenomenology (hep-ph); Nuclear Theory (nucl-th)

We discuss that some light baryon resonances exhibit properties which cannot be described when attributing a three-valence quark structure to them. Besides pointing out the hadron resonances which clearly require description beyond the quark model, we focus on the third $s_{11},~ N^*$ state and its decay to final states consisting of the lightest hyperon resonances which have a partial width comparable to that for the decay to $\pi N$. Such properties of the mentioned nucleon resonance get manifested in the cross sections and other observables related to processes producing the lightest hyperon resonances. We show that all these findings arise from the strong association of the baryon resonances to the dynamics among the ground-state hadrons.

[10]  arXiv:2405.02210 [pdf, other]
Title: Pseudoscalar Higgs plus jet production at Next-to-Next-to-Leading Order in QCD
Comments: 39 pages, 10 figures
Subjects: High Energy Physics - Phenomenology (hep-ph)

We present a calculation of pseudoscalar Higgs production in association with a jet at Next-to-Next-to Leading Order (NNLO) accuracy in QCD. We work in an effective field theory in which $m_t \rightarrow \infty$ resulting in effective operators which couple the pseudoscalar to gluons and (massless) quarks. We have calculated all of the relevant amplitudes for the two-loop, one-loop and tree-level contributions. As a cross-check of our calculation we have re-calculated all of the scalar Higgs plus parton amplitudes and perform a detailed comparison to the literature. In order to regulate the infra-red singularities present at this order we employ the $N-$jettiness slicing method. In addition to a detailed validation of our calculation at this order we investigate LHC phenomenology for a selection of pseudoscalar Higgs masses. Our results are implemented into the parton-level Monte Carlo code MCFM.

[11]  arXiv:2405.02222 [pdf, other]
Title: Unitarity in the non-relativistic regime and implications for dark matter
Comments: 9 pages, 2 figures
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Theory (hep-th)

Unitarity sets upper limits on partial-wave elastic and inelastic cross-sections, which are often violated by perturbative computations. We discuss the dynamics underlying these limits in the non-relativistic regime, namely long-range interactions, and show how the resummation of the elastic 2-particle-irreducible diagrams arising from squaring inelastic processes unitarizes inelastic cross-sections. Our results are model-independent, apply to all partial waves, and affect elastic and inelastic cross-sections, with extensive implications for new physics scenarios, including dark-matter freeze-out and self-interactions.

[12]  arXiv:2405.02254 [pdf, ps, other]
Title: QCD analysis of valence structure functions using deep inelastic lepton-nucleon scattering
Comments: 26 pages, 15 figures, 4 tables
Subjects: High Energy Physics - Phenomenology (hep-ph)

A new ''$\mathtt{SK24}$'' non-singlet QCD analysis of the structure functions at the NNLO approximation is performed, utilizing the global fit of the data from various charged lepton scattering experiments. We extract the valence parton distribution functions (PDFs) and provide a parametrization of them, along with the correlated errors for a wide range of $x$ and $Q^2$. We compare valence PDFs and their uncertainties with those from different PDF sets provided by various groups. We also obtain valence PDFs and the strong coupling constant $\alpha_{s}(M_Z^2)$, taking into account the nuclear correction concerning large $x$ as well as the target mass correction (TMC) and higher twist (HT) effects at the NNLO. In the large $x$ region, we extract the higher twist contributions of $xF_3(x,Q^2)$, $F_2^p (x,Q^2)$, and $F_2^d(x,Q^2)$. We determine $\alpha_{s}(M_Z^2)$ without and with considering the TMC and HT corrections and perform a comparison with the world average of $\alpha_{s}(M_Z^2)$ and other reported results. The extracted results concerning valence PDFs with their uncertainties and $\alpha_{s}(M_Z^2)$ value agree with available theoretical models.

Cross-lists for Mon, 6 May 24

[13]  arXiv:2404.16933 (cross-list from hep-th) [pdf, other]
Title: Flavor's Delight
Comments: 13 pages + citations, 4 figures. Contribution to the Special Issue of MDPI-entropy: Particle Theory and Theoretical Cosmology-Dedicated to Professor Paul Howard Frampton on the Occasion of His 80th Birthday
Journal-ref: Entropy 2024, 26, 355
Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph)

Discrete flavor symmetries provide a promising approach to understand the flavor sector of the standard model of particle physics. Top-down (TD) explanations from string theory reveal two different types of such flavor symmetries: traditional and modular flavor symmetries that combine to the eclectic flavor group. There have been many bottom-up (BU) constructions to fit experimental data within this scheme. We compare TD and BU constructions to identify the most promising groups and try to give a unified description. Although there is some progress in joining BU and TD approaches, we point out some gaps that have to be closed with future model building.

[14]  arXiv:2405.01626 (cross-list from astro-ph.CO) [pdf, other]
Title: Mineral Detection of Neutrinos and Dark Matter 2024. Proceedings
Comments: Summary and proceedings of the MDvDM'24 conference, Jan 8-11 2024
Subjects: Cosmology and Nongalactic Astrophysics (astro-ph.CO); Instrumentation and Methods for Astrophysics (astro-ph.IM); High Energy Physics - Experiment (hep-ex); High Energy Physics - Phenomenology (hep-ph); Instrumentation and Detectors (physics.ins-det)

The second "Mineral Detection of Neutrinos and Dark Matter" (MDvDM'24) meeting was held January 8-11, 2024 in Arlington, VA, USA, hosted by Virginia Tech's Center for Neutrino Physics. This document collects contributions from this workshop, providing an overview of activities in the field. MDvDM'24 was the second topical workshop dedicated to the emerging field of mineral detection of neutrinos and dark matter, following a meeting hosted by IFPU in Trieste, Italy in October 2022. Mineral detectors have been proposed for a wide variety of applications, including searching for dark matter, measuring various fluxes of astrophysical neutrinos over gigayear timescales, monitoring nuclear reactors, and nuclear disarmament protocols; both as paleo-detectors using natural minerals that could have recorded the traces of nuclear recoils for timescales as long as a billion years and as detectors recording nuclear recoil events on laboratory timescales using natural or artificial minerals. Contributions to this proceedings discuss the vast physics potential, the progress in experimental studies, and the numerous challenges lying ahead on the path towards mineral detection. These include a better understanding of the formation and annealing of recoil defects in crystals; identifying the best classes of minerals and, for paleo-detectors, understanding their geology; modeling and control of the relevant backgrounds; developing, combining, and scaling up imaging and data analysis techniques; and many others. During the last years, MDvDM has grown rapidly and gained attention. Small-scale experimental efforts focused on establishing various microscopic readout techniques are underway at institutions in North America, Europe and Asia. We are looking ahead to an exciting future full of challenges to overcome, surprises to be encountered, and discoveries lying ahead of us.

[15]  arXiv:2405.01633 (cross-list from astro-ph.HE) [pdf, other]
Title: Constraints on conformal ultralight dark matter couplings from the European Pulsar Timing Array
Comments: 17 pages, 5 figures
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); Cosmology and Nongalactic Astrophysics (astro-ph.CO); Astrophysics of Galaxies (astro-ph.GA); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Phenomenology (hep-ph)

Millisecond pulsars are extremely precise celestial clocks: as they rotate, the beamed radio waves emitted along the axis of their magnetic field can be detected with radio telescopes, which allows for tracking subtle changes in the pulsars' rotation periods. A possible effect on the period of a pulsar is given by a potential coupling to dark matter, in cases where it is modeled with an "ultralight" scalar field. In this paper, we consider a universal conformal coupling of the dark matter scalar to gravity, which in turn mediates an effective coupling between pulsars and dark matter. If the dark matter scalar field is changing in time, as expected in the Milky Way, this effective coupling produces a periodic modulation of the pulsar rotational frequency. By studying the time series of observed radio pulses collected by the European Pulsar Timing Array experiment, we present constraints on the coupling of dark matter, improving on existing bounds. These bounds can also be regarded as constraints on the parameters of scalar-tensor theories of the Fierz-Jordan-Brans-Dicke and Damour-Esposito-Far\`{e}se types in the presence of a (light) mass potential term.

[16]  arXiv:2405.01887 (cross-list from nucl-th) [pdf, other]
Title: Ab initio calculation of hyper-neutron matter
Comments: 17 pages, 10 figures
Subjects: Nuclear Theory (nucl-th); High Energy Astrophysical Phenomena (astro-ph.HE); Solar and Stellar Astrophysics (astro-ph.SR); General Relativity and Quantum Cosmology (gr-qc); High Energy Physics - Lattice (hep-lat); High Energy Physics - Phenomenology (hep-ph)

The equation of state (EoS) of neutron matter plays a decisive role in our understanding of the properties of neutron stars as well as the generation of gravitational waves in neutron star mergers. At sufficient densities, it is known that the appearance of hyperons generally softens the EoS, thus leading to a reduction in the maximum mass of neutron stars well below the observed values of about 2 solar masses. Even though repulsive three-body forces are known to solve this so-called "hyperon puzzle", so far performing \textit{ab initio} calculations with a substantial number of hyperons has remained elusive. In this work, we address this challenge by employing simulations based on Nuclear Lattice Effective Field Theory with up to 232 neutrons (pure neutron matter) and up to 116 $\Lambda$ hyperons (hyper-neutron matter) in a finite volume. We introduce a novel auxiliary field quantum Monte Carlo algorithm, allowing us to simulate for both pure neutron matter and hyper-neutron matter systems up to 5 times the density of nuclear matter using a single auxiliary field without any sign oscillations. Also, for the first time in {\em ab initio} calculations, we not only include $N\Lambda$ two-body and $NN\Lambda$ three-body forces, but also $\Lambda\Lambda$ and $N \Lambda\Lambda$ interactions. Consequently, we determine essential astrophysical quantities such as the mass-radius relation, the speed of sound and the tidal deformability of neutron stars. Our findings also confirm the existence of the $I$-Love-$Q$ relation, which gives access to the moment of inertia of the neutron star.

[17]  arXiv:2405.01949 (cross-list from gr-qc) [pdf, other]
Title: Bubble wall velocity and gravitational wave in the minimal left-right symmetric model
Comments: 22 pages, 12 figures
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Phenomenology (hep-ph)

The bubble wall velocity in the first order phase transition plays an important role in determining both the amplitude and the pivot frequency of stochastic gravitational wave background. In the framework of the minimal left-right symmetric model, we study the wall velocity when the first order phase transition can occur. The wall velocity can be determined by matching the distribution functions in the free particle approximation and the local thermal equilibrium approximation. It is found that the wall velocity can be determined in the range $ 0.2 < v_w < 0.5 $ for the parameter space with the first order phase transition. It is also found that for the case when the wall velocity is close to the speed of sound, the peak amplitude of gravitational wave spectrum can be larger than that in the runaway case. Moreover, It is also found that there exists an approximate power law between the wall velocity and pressure difference between broken and symmetry phases, and the power index is equal to 0.41 or so.

[18]  arXiv:2405.02193 (cross-list from gr-qc) [pdf, other]
Title: Relic gravitons and non-stationary processes
Comments: 28 pages, 3 figures
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)

Stationary processes do not accurately describe the diffuse backgrounds of relic gravitons whose correlations are homogeneous in space (i.e. only dependent upon the distance between the two spatial locations) but not in time. The symmetries of the autocorrelations ultimately reflect the quantum mechanical origin of the diffuse backgrounds and lead to non-stationary observables at late time. In particular, large oscillations are believed to arise in the spectral energy density that is customarily (but approximately) related to the tensor power spectrum. When the full expression of the spectral energy density is employed the amplitudes of oscillation are instead suppressed in the large-scale limit and the non-stationary features of the late-time signal practically disappear. For similar reasons the relations between the spectral energy density and the spectral amplitude are ambiguous in the presence of non-stationary features. While it is debatable if the non-stationary features are (or will be) directly detectable, we argue that the spectral amplitude following from the Wiener-Khintchine theorem is generally inappropriate for a consistent description of the relic signal. Nevertheless the strong oscillatory behaviour of the late-time observables is naturally smeared out provided the spectral energy density is selected as pivotal variable.

[19]  arXiv:2405.02224 (cross-list from hep-th) [pdf, other]
Title: Lectures on Resurgence in Integrable Field Theories
Authors: Marco Serone
Comments: 45 pages, 7 figures
Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Lattice (hep-lat); High Energy Physics - Phenomenology (hep-ph)

There has been recently considerable progress in understanding the nature of perturbation theory in UV free and gapped $2d$ integrable field theories with renormalon singularities. Thanks to Bethe ansatz and large $N$ techniques, non-perturbative corrections can also be computed and lead to the reconstruction of the trans-series for the free energy in presence of a chemical potential. This is an ideal arena to test resurgence in QFT and determine if and how the exact result can be reconstructed from the knowledge of the perturbative series only. In these notes we give a pedagogical introduction to this subject starting from the basics. In the first lecture we give an overview of applications in QFT of Borel resummations before the advent of resurgence. The second lecture introduces the key concepts of resurgence and finally in the third lecture we discuss a specific application in the context of the principal chiral field model. Extended version of three lectures given at IHES and review talks given at Les Diablerets and Mainz, in 2023.

[20]  arXiv:2405.02245 (cross-list from nucl-th) [pdf, ps, other]
Title: Measurement of the flow harmonic correlations via multi-particle symmetric and asymmetric cumulants in Au+Au collisions at $\sqrt{s_{NN}}$ = 200 GeV
Comments: 9 pages, 6 figures
Subjects: Nuclear Theory (nucl-th); High Energy Physics - Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)

We study multi-particle azimuthal correlations in Au+Au collisions at $\sqrt{s_{NN}} = 200$ GeV. We use initial conditions obtained from a Monte-Carlo Glauber model and evolve them within a viscous relativistic hydrodynamics framework that eventually gives way to a transport model in the late hadronic stage of the evolution. We compute the multi-particle symmetric and asymmetric cumulants and present the results for their sensitivity to the shear and bulk viscosities during the hydrodynamic evolution. We show that these observables are more sensitive to the transport coefficients than the traditional flow observables.

Replacements for Mon, 6 May 24

[21]  arXiv:2106.12623 (replaced) [pdf, other]
Title: Cubic color charge correlator in a proton made of three quarks and a gluon
Comments: v2: additional author, and new fig.8 with a numerical result for the impact parameter dependence of the C-odd correlator; to be published in PRD; v3: fixed symmetry factors for "fig.7 type" diagrams. arXiv admin note: text overlap with arXiv:2010.11245
Journal-ref: Phys. Rev. D 105, 036007 (2022)
Subjects: High Energy Physics - Phenomenology (hep-ph)
[22]  arXiv:2203.05889 (replaced) [pdf, other]
Title: Addressing the Gravitational Wave - Collider Inverse Problem
Comments: 14 pages, 5 figures
Subjects: High Energy Physics - Phenomenology (hep-ph)
[23]  arXiv:2205.05566 (replaced) [pdf, other]
Title: Muon g-2 Anomaly from Vectorlike Leptons in TeV scale Trinification and $E_6$ models
Subjects: High Energy Physics - Phenomenology (hep-ph)
[24]  arXiv:2207.10111 (replaced) [pdf, other]
Title: ALP Dark Matter Mini-Clusters from Kinetic Fragmentation
Comments: 60 pages, 23 figures, minor changes based on the referee comments. Published version
Journal-ref: JCAP 01 (2023) 009
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO)
[25]  arXiv:2303.13503 (replaced) [pdf, other]
Title: LiteBIRD and CMB-S4 Sensitivities to Reheating in Plateau Models of Inflation
Comments: 86 pages, 43 figures; matches version to appear in JCAP
Subjects: High Energy Physics - Phenomenology (hep-ph); Cosmology and Nongalactic Astrophysics (astro-ph.CO)
[26]  arXiv:2306.09029 (replaced) [pdf, other]
Title: Explanation of the Hints for a 95 GeV Higgs Boson within a 2-Higgs Doublet Model
Authors: Alexander Belyaev (1) (2), Rachid Benbrik (3), Mohammed Boukidi (3), Manimala Chakraborti (1), Stefano Moretti (1) (4), Souad Semlali (1) (2) ((1) School of Physics and Astronomy, University of Southampton, United Kingdom, (2) Particle Physics Department, Rutherford Appleton Laboratory, United Kingdom, (3) Polydisciplinary Faculty, Laboratory of Fundamental and Applied Physics, Cadi Ayyad University, Sidi Bouzid, Safi, Morocco, (4) Department of Physics and Astronomy, Uppsala University, Uppsala, Sweden)
Comments: 19 pages, 6 figures. Revised version, matches the version accepted by JHEP
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Experiment (hep-ex)
[27]  arXiv:2310.01484 (replaced) [pdf, other]
Title: Complexity in Tame Quantum Theories
Comments: 48 pages, 2 figures
Journal-ref: JHEP 05 (2024) 001
Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph); Algebraic Geometry (math.AG); Logic (math.LO); Quantum Physics (quant-ph)
[28]  arXiv:2312.00382 (replaced) [pdf, other]
Title: The effective potential of composite operator in the first order region of QCD phase transition
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
[29]  arXiv:2312.03069 (replaced) [pdf, other]
Title: Dissecting the Stochastic Gravitational Wave Background with Astrometry
Comments: 34 pages, 8 figures. Published version in JCAP. v2: minor corrections
Journal-ref: JCAP 05 (2024) 030
Subjects: General Relativity and Quantum Cosmology (gr-qc); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Astrophysical Phenomena (astro-ph.HE); Instrumentation and Methods for Astrophysics (astro-ph.IM); High Energy Physics - Phenomenology (hep-ph)
[30]  arXiv:2312.03184 (replaced) [pdf, other]
Title: Kaluza-Klein tower and bubble nucleation in six dimensional Einstein-Maxwell theory
Authors: Min-Seok Seo
Comments: 23 pages, 10 figures
Journal-ref: Eur.Phys.J.C 84 (2024), 449
Subjects: High Energy Physics - Theory (hep-th); High Energy Physics - Phenomenology (hep-ph)
[31]  arXiv:2312.08339 (replaced) [pdf, ps, other]
Title: Non-relativistic nuclear reduction for tensor couplings in dark matter direct detection and $μ\to e$ conversion
Comments: 9 pages, 3 tables (additional terms and operators)
Subjects: High Energy Physics - Phenomenology (hep-ph); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
[32]  arXiv:2403.15639 (replaced) [pdf, other]
Title: Exotic tetraquarks at the HL-LHC with JETHAD: A high-energy viewpoint
Comments: 38 pages, 7 figures, 500 references. Invited review article
Journal-ref: Symmetry 16 (2024), 5, 550
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Experiment (hep-ex); High Energy Physics - Theory (hep-th); Nuclear Experiment (nucl-ex); Nuclear Theory (nucl-th)
[33]  arXiv:2404.01876 (replaced) [pdf, other]
Title: A nonperturbative test of nucleation calculations for strong phase transitions
Comments: 6 pages, 4 figures plus appendix, v2: fixed typo in tree-level and LPA calculation; conclusions unchanged
Subjects: High Energy Physics - Theory (hep-th); Cosmology and Nongalactic Astrophysics (astro-ph.CO); High Energy Physics - Lattice (hep-lat); High Energy Physics - Phenomenology (hep-ph)
[34]  arXiv:2404.09021 (replaced) [pdf, other]
Title: Is Doublet-Triplet Splitting Necessary?
Comments: 5 pages, 1 figure. Comments are welcome! Version-3: final remark is expanded to discuss the applicability of our mechanism to supersymmetric SU(5), along with three additional references
Subjects: High Energy Physics - Phenomenology (hep-ph)
[35]  arXiv:2404.10926 (replaced) [pdf, other]
Title: Ultra-light Dark Matter Limits from Astrophysical Neutrino Flavor
Comments: 6 pages, 3 figures, 1 table, v2
Subjects: High Energy Physics - Phenomenology (hep-ph)
[36]  arXiv:2404.17444 (replaced) [pdf, other]
Title: Global data-driven determination of baryon transition form factors
Comments: 6 pages, 4 figures
Subjects: Nuclear Theory (nucl-th); High Energy Physics - Phenomenology (hep-ph); Nuclear Experiment (nucl-ex)
[37]  arXiv:2404.18157 (replaced) [pdf, ps, other]
Title: The effects of Lorentz violation on unitarity in $e^{+}e^{-} \rightarrow μ^{+}μ^{-}$
Subjects: High Energy Physics - Phenomenology (hep-ph); High Energy Physics - Theory (hep-th)
[38]  arXiv:2405.01256 (replaced) [pdf, other]
Title: Automatic generation of helicity amplitudes in Feynman-Diagram gauge
Comments: 28 pages, 8 figures and 1 table; typos corrected
Subjects: High Energy Physics - Phenomenology (hep-ph)
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