PaperPanorama

HEP Phenomenology·hep-ph

Wed·Mar 30, 2022

29 papers14 primary·15 cross-listed·reconstructed*

  1. 01*

    Machine Learning model driven prediction of the initial geometry in Heavy-Ion Collision experiments

    Abhisek Saha🇮🇳 · Debasis Dan🇮🇳 · Soma Sanyal🇮🇳

    We demonstrate high prediction accuracy of three important properties that determine the initial geometry of the heavy-ion collision (HIC) experiments by using supervised Machine Learning (ML) methods. These properties are the impact parameter, the eccentricity and the participant eccentricity. Though ML techniques have been used previously to determine the impact parameter of these collisions, we study multiple ML algorithms, their error spectrum, and sampling methods using exhaustive parameter scans and ablation studies to determine a combination of efficient algorithm and tuned training set that gives multi-fold improvement in accuracy for all three different heavy-ion collision models. The three models chosen are a transport model, a hydrodynamic model and a hybrid model. The motivation of using three different heavy-ion collision models was to show that even if the model is trained using a transport model, it gives accurate results for a hydrodynamic model as well as a hybrid model. We show that the accuracy of the impact parameter prediction depends on the centrality of the collision. With the standard application of ML training methods, prediction accuracy is considerable low for central collisions. Our method increases this accuracy by multiple folds. We also show that the eccentricity prediction accuracy can be improved by inclusion of the impact parameter as a feature in all these algorithms. We discuss how the errors can be minimized and the accuracy can be improved to a great extent in all the ranges of impact parameter and eccentricity predictions.

    hep-phPRC(2022)·8 citations
  2. 02*

    Dark Matter Production in Weyl Inflation

    Qing-Yang Wang🇨🇳 · Yong Tang🇨🇳 · Yue-Liang Wu🇨🇳

    Dark matter and inflation are two key elements to understand the origin of cosmic structures in modern cosmology, and yet their exact physical models remain largely uncertain. The Weyl scaling invariant theory of gravity may provide a feasible scheme to solve these two puzzles jointly, which contains a massive gauge boson playing the role of dark matter candidate, and allows the quadratic scalar curvature term, namely , to realize a viable inflationary mechanism in agreement with current observations. We ponder on the production of dark matters in the Weyl model, including the contribution from the non-perturbative production due to the quantum fluctuations from inflationary vacuum and perturbative ones from scattering. We demonstrate that there are generally three parameter ranges for viable dark matter production: (1) If the reheating temperature is larger than , the Weyl gauge boson as dark matter can be produced abundantly with mass larger than the inflation scale . (2) Small mass region with for a higher reheating temperature. (3) Annihilation channel becomes important in the case of higher reheating temperature, which enables the Weyl gauge boson with mass up to to be produced through freeze-in.

    hep-phastro-ph.COgr-qcPRD(2022)·15 citations
  3. 03*

    Single pion production in electron-proton interactions

    M. Kabirnezhad🇨🇦

    This paper presents an extension of the MK single pion production model \cite{MK, MK2} to high hadron invariant mass () and high momentum transfer to conform to the predictions of perturbative QCD due to quark-hadron duality. New form factors for several resonant interactions and non-resonant background in the electron-nucleon cross-sections are determined taking into account the experimental data and improved evaluation techniques. Fits to electron-proton scattering data are used to calculate the vector-current form factors, and to assign uncertainties to the constrained free parameters of the model. The %hadron currents results from this work can be used to determine the vector current in the corresponding neutrino-nucleon cross-sections, which are an important input for event generators in long baseline neutrino oscillation measurements.

    hep-phhep-exPRC(2023)·10 citations
  4. 04*

    QCD sum rule study for hidden-strange pentaquarks

    Pengfei Yang🇨🇳 · Wei Chen🇨🇳

    Inspired by the LHCb's observations of hidden-charm states, we study their hidden-strange analogues states in both and configurations. We investigate the pentaquark states in , , , and structures with and and with , and calculate their masses in the framework of QCD sum rules. Our numerical results show that the extracted hadron masses for all the , , , and structures are much higher than mass threshold and masses for and also higher than threshold of corresponding hadron, so that no bound state exists in such channels, which is consistent with the experimental status to date.

    hep-phhep-exCPC(2023)·7 citations
  5. 05*

    Systematic Parametrization of the Leading -meson Light-Cone Distribution Amplitude

    Thorsten Feldmann🇩🇪 · Philip Lüghausen🇩🇪 · Danny van Dyk🇩🇪

    We propose a parametrization of the leading -meson light-cone distribution amplitude (LCDA) in heavy-quark effective theory (HQET). In position space, it uses a conformal transformation that yields a systematic Taylor expansion and an integral bound, which enables control of the truncation error. Our parametrization further produces compact analytical expressions for a variety of derived quantities. At a given reference scale, our momentum-space parametrization corresponds to an expansion in associated Laguerre polynomials, which turn into confluent hypergeometric functions under renormalization-group evolution at one-loop accuracy. Our approach thus allows a straightforward and transparent implementation of a variety of phenomenological constraints, regardless of their origin. Moreover, we can include theoretical information on the Taylor coefficients by using the local operator production expansion. We showcase the versatility of the parametrization in a series of phenomenological pseudo-fits.

    hep-phJHEP(2022)·25 citations
  6. 06*

    NLO QCD corrections to full off-shell production of including leptonic decays

    Giuseppe Bevilacqua🇭🇺 · Heribertus Bayu Hartanto🇬🇧 · Manfred Kraus🇺🇸 · Jasmina Nasufi🇩🇪 · Malgorzata Worek🇩🇪

    Motivated by ongoing new physics searches in the top-quark sector at the Large Hadron Collider we report on the calculation of NLO QCD corrections to the Standard Model process in the tetra-lepton decay channel. This calculation is based on the matrix elements for the final state and includes all resonant and non-resonant Feynman diagrams, interferences and off-shell effects of the top quark as well as the and gauge bosons. Also incorporated are photon-induced contributions. As it is customary for such studies, we show theoretical predictions for both fixed and dynamical factorisation and renormalisation scale choices and different PDF sets. Furthermore, we study the main theoretical uncertainties that are associated with neglected higher-order terms in the perturbative expansion and with the parameterisation of the PDF sets. In order to investigate the size of off-shell effects and higher-order corrections in top-quark decays, we perform a second computation for this process, which is based on the narrow-width-approximation where the top quarks, and gauge bosons are kept on-shell. Results are given for the integrated and differential fiducial cross sections for the LHC Run II center-of-mass energy of TeV.

    hep-phhep-exJHEP(2022)·27 citations
  7. 07*

    Interdependence of the new "MUON G-2" Result and the -Boson Mass

    E. Bagnaschi🇨🇭 · M. Chakraborti🇵🇱 · S. Heinemeyer🇪🇸 · I. Saha🇯🇵 · G. Weiglein🇩🇪

    The electroweak (EW) sector of the Minimal Supersymmetric extension of the Standard Model (MSSM), assuming the lightest neutralino as Dark Matter (DM) candidate, can account for a variety of experimental results. In particular it can account for the discrepancy between the experimental result for the anomalous magnetic moment of the muon, , and its Standard Model (SM) prediction. The new "MUON G-2" result, combined with the older BNL result on , yields a deviation from the SM prediction of , corresponding to . Using this updated bound, together with the other constraints, we calculate the MSSM prediction for the mass of the boson, . We assume contributions only from the EW sector, with the colored sector of the MSSM taken to be heavy. We investigate five scenarios, distinguished by the mechanisms which yield a relic DM density in agreement with the latest Planck bounds. We find that with the new result taken into account and depending on the scenario, values up to are reached. The largest values are obtained for wino DM and in the case of slepton co-annihilation, where points well within the range of the experimental world average of are reached, whereas the SM predicts a too small value of . We analyze the dependence of on the relevant masses of the EW superpartners and demonstrate that future measurements, e.g. at the ILC, could distinguish between various MSSM realizations. Sizable contributions to are associated with a relatively light , accompanied by either a light chargino or a light smuon, setting interesting targets for future collider searches.

    hep-phEPJC(2022)·35 citations
  8. 08*

    Evaluating the ILC SUSY reach in the most challenging scenario: NLSP, low , lowest cross-section

    M.T. Núñez Pardo de Vera🇩🇪 · M. Berggren🇩🇪 · J. List🇩🇪

    Pair-production of the superpartner of the -lepton, the , is one of the most interesting channels to search for SUSY in: The is likely to be the lightest scalar lepton, and the signature of pair production is one of the experimentally most difficult ones, thereby constituting the "worst" possible scenario for SUSY searches. The current model-independent limits comes from analyses performed at LEP but they suffer from the limited energy of this facility. Limits obtained at the LHC do extend to higher masses, but they are only valid under strong assumptions. The International Linear Collider, the ILC, is a future electron-positron collider, to operate initially at an energy of 250 GeV, then to be upgraded to 500 GeV, and possibly to 1 TeV at a later stage. ILC will be a powerful facility for SUSY searches. The capability of the ILC for determining exclusion/discovery limits for the in a model-independent way is shown in this paper. A detailed study of the "worst" scenario for exclusion/discovery, taking into account the effect of the mixing on production cross-section and detection efficiency, is presented. The study also includes an analysis of the effect of the overlay particles in the searches. The conclusion is that both the exclusion and discovery reaches for this "worst" case would extend to only a few GeV below the kinematic limit at the ILC. Also scenarios with the and the Lightest SUSY Particle (the LSP) quite close in mass can be discovered or excluded at most masses. The studies were done using detailed detector simulation of the ILD concept at the ILC. For signal, the fast detector simulation SGV was used, while the full Geant4 based DDSim was used for the standard model backgrounds.

    hep-ph5 citations
  9. 09*

    On gravitational preheating

    Oleg Lebedev🇫🇮 · Jong-Hyun Yoon🇫🇮

    We consider dark matter production during the inflaton oscillation epoch. It is conceivable that renormalizable interactions between dark matter and inflaton may be negligible. In this case, the leading role is played by higher dimensional operators generated by gravity and thus suppressed by the Planck scale. We focus on dim-6 operators and study the corresponding particle production in perturbative and non-perturbative regimes. We find that the dark matter production rate is dominated by non-derivative operators involving higher powers of the inflaton field. Even if they appear with small Wilson coefficients, such operators can readily account for the correct dark matter abundance.

    hep-phastro-ph.COJCAP(2022)·24 citations
  10. 10*

    Prospects for precise predictions of in the Standard Model

    G. Colangelo🇨🇭 · M. Davier🇫🇷 · A. X. El-Khadra🇺🇸 · M. Hoferichter🇨🇭 · C. Lehner🇩🇪 · L. Lellouch🇫🇷 · T. Mibe🇯🇵 · B. L. Roberts🇺🇸 · T. Teubner🇬🇧 · H. Wittig🇩🇪 · B. Ananthanarayan🇮🇳 · A. Bashir🇲🇽 and 70 other authors

    We discuss the prospects for improving the precision on the hadronic corrections to the anomalous magnetic moment of the muon, and the plans of the Muon Theory Initiative to update the Standard Model prediction.

    hep-phhep-exhep-latnucl-ex+1136 citations
  11. 11*

    Axion signatures from supernova explosions through the nucleon electric-dipole portal

    Giuseppe Lucente🇮🇹 · Leonardo Mastrototaro🇮🇹 · Pierluca Carenza🇸🇪 · Luca Di Luzio🇮🇹 · Maurizio Giannotti🇺🇸 · Alessandro Mirizzi🇮🇹

    We consider axions coupled to nucleons and photons only through the nucleon electric-dipole moment (EDM) portal. This coupling is a model-independent feature of QCD axions, which solve the strong CP problem, and might arise as well in more general axion-like particle setups. We revise the supernova (SN) axion emission induced by the nucleon EDM coupling and refine accordingly the SN 1987A bound. Furthermore, we calculate the axion flux from a future Galactic SN and show that it might produce a peculiar and potentially detectable gamma-ray signal in a large underground neutrino detector such as the proposed Hyper-Kamiokande. The possibility to detect such a signal offers a way to search for an oscillating nucleon EDM complementary to CASPERe, without relying on the assumption that axions are a sizeable component of the dark matter. Furthermore, if axions from SN produce an observable signal, they could also lead to an amount of cosmological extra-radiation observable in future cosmic surveys.

    hep-phastro-ph.HEPRD(2022)·68 citations
  12. 12*

    Glueballs in a Thermal Squeezeout Model

    Pouya Asadi🇺🇸 · Eric David Kramer🇮🇱 · Eric Kuflik🇮🇱 · Tracy R. Slatyer🇺🇸 · Juri Smirnov🇸🇪

    It has been shown that a first order confinement phase transition can drastically change the relic dark matter abundance in confining dark sectors with only heavy dark quarks. We study the phenomenology of one such model with a Z' portal to Standard Model. We find that dark glueballs are long-lived in this setup and dilute the dark matter abundance after their decay to Standard Model. With this effect, the correct relic abundance is obtained with dark matter masses up to ~TeV. We find that while a part of the parameter space is already ruled out by direct detection and collider searches, there is still a broad space of viable scenarios that can be probed by future experiments.

    hep-phhep-thJHEP(2022)·35 citations
  13. 13*

    Altered Axion Abundance from a Dynamical Peccei-Quinn Scale

    Itamar J. Allali🇺🇸 · Mark P. Hertzberg🇺🇸 · Yi Lyu🇺🇸

    We build a model in which the relic abundance of axions is altered from the standard misalignment mechanism, either increased or decreased, due to the presence of a new light scalar that couples to the radial part of the Peccei-Quinn (PQ) field. The light scalar makes the effective PQ symmetry-breaking scale dynamical, altering the early-time dynamics for the axion and affecting its late-time dark matter abundance. We analyze this new mechanism semianalytically and numerically, showing that we can accommodate both lighter or heavier axion dark matter, compared to the standard treatments. We discuss implications of the model for axion searches and fundamental physics.

    hep-phastro-ph.COhep-thPRD(2022)·22 citations
  14. 14*

    Comment on "Poynting vector controversy in axion modified electrodynamics"

    Kevin Zhou🇺🇸

    In a recent publication, Tobar, McAllister, and Goryachev claim that using an alternative definition of the Poynting vector can dramatically enhance the sensitivity of their proposed axion dark matter detector. While the choice of Poynting vector is indeed ambiguous, it cannot affect physical results, such as the reading on a voltmeter, as long as the same definition is used consistently. I explain this point in detail, and locate the specific errors in their calculation.

    hep-phhep-exphysics.ins-det4 citations
  15. 15*

    Nonextensive hydrodynamics of boost-invariant plasmas

    Mubarak Alqahtani🇸🇦 · Nasser Demir🇰🇼 · Michael Strickland🇺🇸

    We use quasiparticle anisotropic hydrodynamics to study the non-conformal and non-extensive dynamics of a system undergoing boost-invariant Bjorken expansion. To introduce nonextensivity, we use an underlying Tsallis distribution with a time-dependent nonextensivity parameter . By taking moments of the quasiparticle Boltzmann equation in the relaxation-time approximation, we obtain dynamical equations which allow us to determine the time evolution of all microscopic parameters including . We compare numerical solutions for bulk observables obtained using the nonextensive evolution with results obtained using quasiparticle anisotropic hydrodynamics with a Boltzmann distribution function (). We show that the evolution of the temperature, pressure ratio, and scaled energy density, are quite insensitive to which distribution function is assumed. However, we find significant differences in the early-time evolution of the bulk pressure which are observed for even small deviations from the Boltzmann distribution function. Finally, we discuss the existence of non-conformal hydrodynamic attractors for the longitudinal and transverse pressures, the bulk and shear viscous corrections, and the nonextensivity parameter .

    nucl-thhep-phEPJC(2022)·16 citations
  16. 16*

    Quintessence Dark Energy from strongly-coupled Higgs mass gap: Local and Non-local higher-derivative non-perturbative scenarios

    Marco Frasca🇮🇹 · Anish Ghoshal🇵🇱 · Alexey Koshelev🇵🇹

    We entertain the possibility that dark energy arises from the Higgs field of quintessence type in the non-perturbative regimes. For this purpose we utilize a set of exact solutions of Higgs field theory recently devised, in terms of Jacobi elliptical function for a massless quartic scalar field, that satisfy a massive dispersion relation. In certain regions of the parameter space, determined by the quartic coupling value, we show that such solutions have the property to give the correct behavior for the equation of state of the dark energy depending on the initial value of periodicity of the Jacobi elliptical function solution. It is seen that on a time scale determined by the Hubble constant and the strength of the self-interaction of the scalar field, when conformal invariance is restored, the equation of state for the dark energy becomes manifest. Further we investigate scenarios within standard field theory framework and also extending to higher-derivative theories, namely infinite-derivative theory, motivated from p-adic string field theory, and Lee-Wick theories and in all cases, we find suitable choices of the parameter space leads to dark energy behavior of the Higgs field, which we compare.

    hep-thastro-ph.COhep-phEPJC(2022)·13 citations
  17. 17*

    EstrellaNueva: an open-source software to study the interactions and detection of neutrinos emitted by supernovae

    O. I. González-Reina🇲🇽 · J. Rumleskie🇨🇦 · E. Vázquez-Jáuregui🇲🇽

    Supernovae emit large fluxes of neutrinos which can be detected by detectors on Earth. Future tonne-scale detectors will be sensitive to several neutrino interaction channels, with thousands of events expected if a supernova emerges in the galaxy neighborhood. There is a limited number of tools to study the interaction rates of supernova neutrinos, although a plethora of available supernova models exists. EstrellaNueva is an open-source software to calculate expected rates of supernova neutrinos in detectors using target materials with typical compositions, and additional compositions can be easily added. This software considers the flavor transformation of neutrinos in the supernova through the adiabatic Mikheyev--Smirnov--Wolfenstein effect, and their interaction in detectors through several channels. Most of the interaction cross sections have been analytically implemented, such as neutrino-electron and neutrino-proton elastic scattering, inverse beta decay, and coherent elastic neutrino-nucleus scattering. This software provides a link between supernova simulations and the expected events in detectors by calculating fluences and event rates to ease any comparison between theory and observation. It provides a simple and standalone tool to explore many physics scenarios offering an option to add analytical cross sections and define any target material.

    astro-ph.IMastro-ph.HEastro-ph.SRhep-ex+1ApJ(2022)·3 citations
  18. 18*

    Search for the chiral magnetic effect in collisions between two isobars with deformed and neutron-rich nuclear structures

    Xin-Li Zhao🇨🇳 · Guo-Liang Ma🇨🇳

    Isobar collisions which were thought to have the same background and different magnetic fields provide an opportunity to verify the chiral magnetic effect (CME) in relativistic heavy-ion collisions. However, the first result from the RHIC-STAR isobar experiment did not observe the CME signal, but discovered that the backgrounds are different between and collisions. We test eighteen cases of Woods-Saxon parameter settings resulting from different nuclear deformation or nuclear structure effects using a mutiphase transport model. We find out that seven cases can reasonably reproduce three reference ratios measured by the STAR experiment. Considering both the halo-type neutron skin structure and CME-like charge separation, we demonstrate that it is difficult for the CME observables (, ratio, and ratio) to distinguish the presence or absence of the CME, if the CME strength is weak in isobar collisions. It is because the final state interactions significantly weaken the initial CME signal, resulting in non-linear sensitivities of the CME observables to the CME strength. Therefore, more sensitive observables are required to search for the possible small CME signal in isobar collisions.

    nucl-thhep-phnucl-exPRC(2022)·29 citations
  19. 19*

    An accurate relativistic chiral nucleon-nucleon interaction up to the next-to-next-to-leading order

    Jun-Xu Lu🇨🇳 · Yang Xiao🇨🇳 · Chun-Xuan Wang🇨🇳 · Li-Sheng Geng🇨🇳

    We report on the construction of an accurate relativistic chiral nucleon-nucleon interaction up to the next-to-next-to-leading (NNLO) order. We compare the so-obtained neutron-proton phaseshifts with the next-to-next-to-next-to-leading order (NLO) nonrelativistic ones and we show that up to MeV, the relativistic chiral nuclear force can describe the PWA93 phaseshifts and inelasticities as well as its NLO nonrelativistic counterparts. As a result, the relativistic chiral nuclear force can be readily used for relativistic ab initio nuclear structure, reaction, as well astrophysical studies.

    nucl-thhep-lathep-phnucl-exPoS(2024)·2 citations
  20. 20*

    Gravitational waves detectable in laser interferometers from axion-SU(2) inflation

    Tomohiro Fujita🇯🇵 · Kaname Imagawa🇯🇵 · Kai Murai🇯🇵

    Chromo-natural inflation (CNI) is an inflationary model where an axion coupled with SU gauge fields acts as the inflaton. In CNI, the gauge fields have nonzero vacuum expectation values (VEVs), which results in the enhancement of gravitational waves (GWs). The original CNI is ruled out by the Planck observations due to the overproduction of GWs. In this work, we consider an inflationary model where the gauge fields acquire nonzero VEVs after the CMB modes exit the horizon. Moreover, we add to the model another field that dominates the universe and drives inflation after the axion starts to oscillate and the gauge field VEVs vanish. By performing numerical simulations, we find a parameter space where the enhanced GWs do not violate the CMB constraints and can be detected by the future GWs observations such as BBO and ET.

    astro-ph.COhep-phJCAP(2022)·21 citations
  21. 21*

    Sliding Dumbbell Method to search for the CME in heavy ion collisions

    Madan M. Aggarwal🇮🇳 · Anjali Attri🇮🇳 · Sonia Parmar🇮🇳 · Anjali Sharma🇮🇳 · Jagbir Singh🇮🇳

    This study explores the Chiral Magnetic Effect (CME) in ultra-relativistic heavy-ion collisions. The CME, observed as back-to-back charge separation along the magnetic field axis, is investigated using the newly developed Sliding Dumbbell Method (SDM) applied to Au+Au events at a center-of-mass energy = 200 GeV generated by the AMPT model with string melting configuration. The CME-like signal is externally injected in events by flipping charges of pairs of the particles perpendicular to the reaction plane. The study reports a significant enhancement of the CME-sensitive 3-particle correlator in events with high back-to-back charge separation, in a given collision centrality. Additionally, a linear relationship is observed between the correlator for same-sign charge pairs and positive charge asymmetry () across the dumbbell in CME-enriched sub-samples. Furthermore, the fraction of CME in (difference between opposite and same sign correlators) is presented across different collision centralities having different percentages of externally injected CME-like signal. Overall, the research aims to understand and detect the Chiral Magnetic Effect through innovative experimental method and detailed analysis of event structure.

    nucl-thhep-phPramana(2024)·3 citations
  22. 22*

    A new experiment to detect dark matter in sub-MeV range using semiconductor superlattice superstructures (SSS)

    Kalpana Bora🇮🇳

    About of the matter in our Universe is made up of Dark Matter (DM), which interacts with Standard Model (SM) matter only through gravitational or weak interactions. Many proposals have been made by scientists about the possible candidates of DM - WIMPs, axions, ALPs, black holes etc. And range of its mass could be extremely broad - from Planck scale to as light as eV. Experiments to detect DM are extremely challenging, as DM does not exhibit appreciable interactions with ordinary matter. May be due to such elusive nature, so far it has not been possible to detect DM, though many experiments are going on worldwide to do so. With about 40 orders of magnitude variation in their mass, it is possible that their gravitational interaction too is very weak, and many creative proposals have been made to detect possible DM candidates, with vast variation of techniques and target materials. In this work, we propose a new experiment to detect sub-MeV range DM particles, using the semiconductor superlattice superstructure (SSS) as the target material. Such materials have band gap of the order of few hundreds of milli eV, and are suitable for detecting sub-MeV range particles scattering off electrons. The photons emitted as a result of excitation of SSS lie in the micrometer range and may be detected via quantum cascade lasers (QCL).

    hep-exhep-ph0 citations
  23. 23*

    Transport coefficients of quasi-particle models within a new relaxation time approximation of the Boltzmann equation

    Gabriel S. Rocha🇧🇷 · Maurício N. Ferreira🇧🇷 · Gabriel S. Denicol🇧🇷 · Jorge Noronha🇺🇸

    We investigate the transport properties of a kinetic theory model that is tuned to describe the thermodynamic properties of QCD at zero chemical potential using a new formulation of the relaxation time approximation. In contrast to previous approaches, the latter is constructed to preserve the fundamental properties of the collision term of the Boltzmann equation for any energy-dependence of the relaxation time. A novel choice of matching conditions is implemented to ensure that the background mean-field depends only on the temperature even when the system is out of equilibrium. We provide a consistent analysis of how the transport coefficients of relativistic Navier-Stokes theory vary with the energy dependence of the relaxation time. We also show that the entropy production of this theory is consistent with the second law of thermodynamics and verify that it is independent of the matching conditions employed. We used this fact to calculate the matching independent combination of transport coefficients.

    nucl-thhep-phhep-thPRD(2022)·21 citations
  24. 24*

    The effect of multiple features on the power spectrum in two-field inflation

    K. Boutivas🇬🇷 · I. Dalianis🇬🇷 · G.P. Kodaxis🇬🇷 · N. Tetradis🇬🇷

    We extend our previous work on the enhancement of the curvature spectrum during inflation to the two-field case. We identify the slow-roll parameter as the quantity that can trigger the rapid growth of perturbations. Its two components, along the background trajectory and perpendicular to it, remain small during most of the evolution, apart from short intervals during which they take large, positive or negative, values. The typical reason for the appearance of strong features in is sharp steps or inflection points in the inflaton potential, while grows large during sharp turns in field space. We focus on the additive effect of several features leading to the resonant growth of the curvature spectrum. Three or four features in the evolution of are sufficient in order to induce an enhancement of the power spectrum by six or seven orders of magnitude, which can lead to the significant production of primordial black holes and stochastic gravitational waves. A big part of our study focuses on understanding the evolution of the perturbations and the resulting spectra through analytic means. The presence of multiple features in the background evolution points to a more complex inflationary paradigm, which is also more natural in the multi-field case. The critical examination of this possibility is within the reach of experiment.

    astro-ph.COgr-qchep-phhep-thJCAP(2022)·22 citations
  25. 25*

    Majorana propagator on de Sitter space

    Tomislav Prokopec🇳🇱 · Vishnu Hari Unnithan🇳🇱

    We study the dynamics of Majorana fermions in an expanding de Sitter space and to that aim we construct the vacuum Feynman propagator for Majorana fermions in de Sitter space. Surprisingly, the Majorana propagator is identical to that of the Dirac fermions. We then use this propagator and calculate the one-loop effective action for Majorana fermions, and show that it differs from that of Dirac fermions by a factor of 1/2, which accounts for the reduced number of degrees of freedom of the Majorana particle. Finally, we derive the Majorana and Dirac propagators for mixing fermionic flavors, which are suitable for studying CP-violating effects in quantum loops.

    hep-thhep-phEPJC(2022)·5 citations
  26. 26*

    The cosmological constant as a boundary term

    Wilfried Buchmuller🇩🇪 · Norbert Dragon🇩🇪

    We compare the path integral for transition functions in unimodular gravity and in general relativity. In unimodular gravity the cosmological constant is a property of states that are specified at the boundaries whereas in general relativity the cosmological constant is a parameter of the action. Unimodular gravity with a nondynamical background spacetime volume element has a time variable that is canonically conjugate to the cosmological constant. Wave functions depend on time and satisfy a Schrödinger equation. On the contrary, in the covariant version of unimodular gravity with a 3-form gauge field, proposed by Henneaux and Teitelboim, wave functions are time independent and satisfy a Wheeler-DeWitt equation, as in general relativity. The 3-form gauge field integrated over spacelike hypersurfaces becomes a "cosmic time" only in the semiclassical approximation. In unimodular gravity the smallness of the observed cosmological constant has to be explained as a property of the initial state.

    hep-thgr-qchep-phJHEP(2022)·9 citations
  27. 27*

    spin polarization in event-by-event relativistic heavy-ion collisions

    Sahr Alzhrani🇺🇸 · Sangwook Ryu🇺🇸 · Chun Shen🇺🇸

    We present a systematic study of hyperon's polarization observables using event-by-event (3+1)D relativistic hydrodynamics. The effects of initial hot spot size and QGP's specific shear viscosity on the polarization observables are quantified. We examine the effects of the two formulations of the thermal shear tensor on the polarization observables using the same hydrodynamic background. With event-by-event simulations, we make predictions for the Fourier coefficients of 's longitudinal polarization with respect to the event planes of different orders of anisotropic flow. We propose new correlations among the Fourier coefficients of and charged hadron anisotropic flow coefficients to further test the mapping from fluid velocity gradients to hyperon's polarization. Finally, we present a system size scan with Au+Au, Ru+Ru, and O+O collisions at GeV to study the system size dependence of polarization observables at the Relativistic Heavy-ion Collider.

    nucl-thhep-phnucl-exPRC(2022)·77 citations
  28. 28*

    Galactic diffuse gamma rays meet the PeV frontier

    Pedro De la Torre Luque🇸🇪 · Daniele Gaggero🇪🇸 · Dario Grasso🇮🇹 · Ottavio Fornieri🇮🇹 · Kathrin Egberts🇩🇪 · Constantin Steppa🇩🇪 · Carmelo Evoli🇮🇹

    The Tibet AS and LHAASO collaborations recently reported the observation of a -ray diffuse emission with energy up to the PeV from the Galactic plane. We discuss the relevance of non-uniform cosmic-ray transport scenarios and the implications of these results for cosmic-ray physics. We use the {\tt DRAGON} and {\tt HERMES} codes to build high-resolution maps and spectral distributions of that emission for several representative models under the condition that they reproduce a wide set of local cosmic-ray data up to 100 PeV. We show that the energy spectra measured by Tibet AS, LHAASO, ARGO-YBJ and Fermi-LAT in several regions of interest in the sky can all be consistently described in terms of the emission arising by the Galactic cosmic-ray "sea". We also show that all our models are compatible with IceTop -ray upper limits. Our results favor transport models characterized by spatial-dependent diffusion although some degeneracy remains between the choice of the transport scenario and that of the cosmic-ray spectral shape above 10 TeV. We discuss the role of forthcoming measurements in resolving that ambiguity.

    astro-ph.HEhep-phAstron.Astrophys.(2023)·76 citations
  29. 29*

    Four-mode squeezed states in de Sitter space: A study with two field interacting quantum system

    Sayantan Choudhury🇮🇳 · Sudhakar Panda🇮🇳 · Nilesh Pandey🇮🇳 · Abhishek Roy🇮🇳

    In this paper we study the application of four-mode squeezed states in the cosmological context, studying two weakly coupled scalar fields in the planar patch of the de Sitter space. We construct the four-mode squeezed state formalism and connect this concept with the Hamiltonian of the two coupled inverted harmonic oscillators having a time-dependent effective frequency in the planar patch of the de Sitter space. Further, the corresponding evolution operator for the quantum Euclidean vacuum state has been constructed, which captures its dynamics. Using the Heisenberg picture coupled differential equations describing the time evolution for all squeezing parameters (amplitude, phase and angle) have been obtained, for the weakly coupled two scalar field model. With the help of these evolutions for the coupled system, we simulate the dynamics of the squeezing parameters in terms of conformal time. From our analysis, we observe interesting dynamics, which helps us to explore various underlying physical implications of the weakly coupled two scalar field system in the planar patch of the de Sitter cosmological background.

    gr-qchep-phhep-thquant-phFortsch.Phys.(2022)·8 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.