PaperPanorama

HEP Phenomenology·hep-ph

Fri·Jun 29, 2018

25 papers—18 primary·7 cross-listed·reconstructed*

  1. 01*

    Sterile Neutrinos with Secret Interactions -- Cosmological Discord?

    Xiaoyong Chu🇦🇹 · Basudeb Dasgupta🇮🇳 · Mona Dentler🇩🇪 · Joachim Kopp🇩🇪 · Ninetta Saviano🇩🇪

    Several long-standing anomalies from short-baseline neutrino oscillation experiments -- most recently corroborated by new data from MiniBooNE -- have led to the hypothesis that extra, 'sterile', neutrino species might exist. Models of this type face severe cosmological constraints, and several ideas have been proposed to avoid these constraints. Among the most widely discussed ones are models with so-called 'secret interactions' in the neutrino sector. In these models, sterile neutrinos are hypothesized to couple to a new interaction, which dynamically suppresses their production in the early Universe through finite-temperature effects. Recently, it has been argued that the original calculations demonstrating the viability of this scenario need to be refined. Here, we update our earlier results from arXiv:1310.6337 [JCAP 1510 (2015) no.10, 011] accordingly. We confirm that much of the previously open parameter space for secret interactions is in fact ruled out by cosmological constraints on the sum of neutrino masses and on free-streaming of active neutrinos. We then discuss possible modifications of the vanilla scenario that would reconcile sterile neutrinos with cosmology.

    hep-phJCAP(2018)·100 citations
  2. 02*

    Assessing signals of TMD physics in SIDIS azimuthal asymmetries and in the extraction of the Sivers function

    M. Boglione🇮🇹 · U. D'Alesio🇮🇹 · C. Flore🇮🇹 · J.O. Gonzalez-Hernandez🇮🇹

    New data on the Sivers azimuthal asymmetry measured in semi-inclusive deep-inelastic scattering processes have recently been released by the COMPASS Collaboration at CERN. Their increased precision and their particular binning, in terms of as well as , motivates a new extraction of the Sivers function, within the framework of a simple and transparent parametrization. Signals of TMD effects visible in the Sivers asymmetries are critically assessed. A thorough study of the uncertainties affecting the extracted Sivers function is presented, including the low- and large- regions.

    hep-phJHEP(2018)·40 citations
  3. 03*

    Linear Seesaw for Dirac Neutrinos with Flavour Symmetry

    Debasish Borah🇮🇳 · Biswajit Karmakar🇮🇳

    We propose a linear seesaw model to realise light Dirac neutrinos within the framework of discrete flavour symmetry. The additional fields and their transformations under the flavour symmetries are chosen in such a way that naturally predicts the hierarchies of different elements of the seesaw mass matrix and also keeps the unwanted terms away. For generic choices of flavon alignments, the model predicts normal hierarchical light neutrino masses with the atmospheric mixing angle in the lower octant. Apart from predicting interesting correlations between different neutrino parameters as well as between neutrino and model parameters, the model also predicts the leptonic Dirac CP phase to lie in a specific range and that includes the currently preferred maximal value. The predictions for the absolute neutrino masses in one specific version of the model can also saturate the cosmological upper bound on sum of absolute neutrino masses.

    hep-phPLB(2019)·69 citations
  4. 04*

    Neutral-naturalness from a holographic SO(6)/SO(5) composite Higgs model

    Barry M. Dillon🇸🇮

    We study a holographic realisation of a composite Higgs model with an SO(6)/SO(5) symmetry breaking coset in which the top sector includes colour-neutral twin-partners that reduce the sensitivity of the Higgs mass to the cut-off. Key to this neutral-naturalness mechanism is a Z2 symmetry that leaves the Yukawa couplings to the Higgs boson invariant under an exchange of the top quark and twin top quark, but the symmetry structure of the model means that the Z2 symmetry is not present in the gauge boson couplings to the Higgs. Within the calculable framework of holography we construct and study the Higgs potential. We examine the relation between the Higgs mass, top-partner spectra, and the input parameters, finding that the presence of the twin-partners pushes the masses of the lightest coloured top-partners up to approximately 1500 GeV while the decay constant remains at approximately 700 GeV. Interestingly, no additional Z2 breaking terms are required to reproduce the observed masses of the electroweak gauge bosons, Higgs boson, and top quark.

    hep-phPRD(2019)·18 citations
  5. 05*

    Remarks on the Debye Length and the Topological Susceptibilty in Non-Abelian Gauge Theory

    Michael Dine🇺🇸 · Di Xu🇺🇸

    We study the Debye mass, , and the topological susceptibility, , at high temperatures in non-abelian gauge theory. Both exhibit, at some order in the perturbation expansion, infrared sensitivity. As a result, a perturbative analysis can at best provide an estimate of these quantities, subject to some uncertainty. The size of these uncertainties, particularly in the case of , has been the subject of some debate. For the perturbative free energy, reframing an analysis of Braaten and Pisarski, the estimate and the associated error, can be understood in terms of a {\it Wilsonian} effective action for the low energy effective three dimensional theory. This action can be obtained completely from a perturbative calculation, which terminates at a finite order. This action provides the desired estimate. The size of the error follows from dimensional analysis in the low energy theory. The Debye length computation and its error can be obtained from a similar study of a non-relativistic effective theory for an adjoint scalar in three dimensions. requires a four dimensional analysis involving finite temperature instantons, but again the dominant sources of uncertainty are three dimensional, and we provide a procedure to estimate and an associated error. This uncertainty is of order relative to the leading semiclassical result, and in situations of interest is small.

    hep-phhep-th0 citations
  6. 06*

    The Angantyr model for Heavy-Ion Collisions in PYTHIA8

    Christian Bierlich🇸🇪 · Gösta Gustafson🇸🇪 · Leif Lönnblad🇸🇪 · Harsh Shah🇸🇪

    We present a new model for building up complete exclusive hadronic final states in high energy nucleus collisions. It is a direct extrapolation of high energy pp collisions (as described by PYTHIA), and thus bridges a large part of the existing gap between heavy ion and high energy physics phenomenology. The model is inspired by the old Fritiof model and the notion of wounded nucleons. Two essential features are the treatment of multi-parton interactions and diffractive excitation in each NN sub-collision. Diffractive excitation is related to fluctuations in the nucleon partonic sub-structure, and fluctuations in both projectile and target are here included for the first time. The model is able to give a good description of general final-state properties such as multiplicity and transverse momentum distributions, both in pA and AA collisions. The model can therefore serve as a baseline for understanding the non-collective background to observables sensitive to collective behaviour. As PYTHIA does not include a mechanism to reproduce the collective effects seen in pp collisions, such effects are also not reproduced by the present version of Angantyr. Effects of high string density, shown to be able to reproduce e.g. higher strangeness ratios and the ridge in pp, will be added in future studies

    hep-phJHEP(2018)·312 citations
  7. 07*

    Scaling Properties of Multiplicity Fluctuations in the AMPT Model

    Rohni Sharma🇮🇳 · Ramni Gupta🇮🇳

    From the events generated from the MC code of a multi-phase transport (AMPT) model with string melting, the properties of multiplicity fluctuations of charged particles in Pb-Pb collisions at are studied. Normalized factorial moments, , of spatial distributions of the particles have been determined in the framework of intermittency. Those moments are found in some kinematic regions to exhibit scaling behavior at small bin sizes, but not in most regions. However, in relating to scaling behavior is found in nearly all regions. The corresponding scaling exponents, , determined in the low transverse momentum () region 1.0 GeV/c are observed to be independent of the bin position and width. The value of is found to be larger than 1.304, which is the value that characterizes the Ginzburg-Landau type second order phase transition. Thus there is no known signature for phase transition in the AMPT model. This study demonstrates that, for the system under investigation, the method of analysis is effective in extracting features that are relevant to the question of whether the dynamical processes leading phase transition are there or not.

    hep-phAdv.High Energy Phys.(2018)·13 citations
  8. 08*

    Single spin asymmetries in ultra-peripheral collisions

    Sanjin Benić🇯🇵 · Yoshitaka Hatta🇯🇵

    We suggest inclusive hadron production in ultra-peripheral proton-nucleus collisions (UPCs) as a new channel to investigate single spin asymmetries (SSAs), in particular, to test the assumed dominance of the contribution from twist-three fragmentation functions. The UPC cross sections are obtained by considering the photoproduction limit of semi-inclusive deep inelastic scattering (SIDIS). In particular, we find simple formulas for the polarized UPC cross sections in the collinear twist-three framework. We then numerically calculate the fragmentation contribution to SSA in at GeV and find a few percent asymmetry in the forward region.

    hep-phPRD(2018)·5 citations
  9. 09*

    The Chiral Magnetic Effect and an experimental bound on the late time magnetic field strength

    Berndt Müller🇺🇸 · Andreas Schäfer🇩🇪

    We first compare different approaches to estimates of the magnitude of the chiral magnetic effect in relativistic heavy ion collisions and show that their main difference lies in the assumptions on the length of persistence of the magnetic field generated by the colliding nuclei. We then analyze recent measurements of the global polarization of and hyperons in terms of the bounds they set on the magnitude of the late time magnetic field.

    hep-phnucl-thPRD(2018)·57 citations
  10. 10*

    The twist-three distribution in a light-front model

    B. Pasquini (1, 2)🇮🇹 · S. Rodini (1, 2) ((1) Pavia U., (2) INFN, Pavia)🇮🇹

    We discuss the twist-three, unpolarized, chiral-odd, transverse momentum dependent parton distribution (TMD) within a light-front model. We review a model-independent decomposition of this TMD, which follows from the QCD equations of motion and is given in terms of a leading-twist mass term, a pure interaction-dependent contribution, and singular terms. The leading-twist and pure twist-three terms are represented in terms of overlap of light-front wave functions (LFWFs), taking into account the Fock states with three valence quark () and three-quark plus one gluon (). The and LFWFs with total orbital angular momentum zero are modeled using a parametrization derived from the conformal expansion of the proton distribution amplitudes, with parameters fitted to reproduce available phenomenological information on the unpolarized leading-twist quark and gluon collinear parton distributions. Numerical predictions for both the quark TMD and the collinear parton distribution are presented, discussing the role of the quark-gluon correlations in the proton.

    hep-phhep-exnucl-exnucl-thPLB(2019)·50 citations
  11. 11*

    Axion-modified photon propagator, Coulomb potential and Lamb-shift

    Selym Villalba-Chávez🇩🇪 · Alina Golub🇩🇪 · Carsten Müller🇩🇪

    A consistent renormalization of a quantum theory of axion-electrodynamics requires terms beyond the minimal coupling of two photons to a neutral pseudoscalar field. This procedure is used to determine the self-energy operators of the electromagnetic and the axion fields with an accuracy of second-order in the axion-diphoton coupling. The resulting polarization tensor is utilized for establishing the axion-modified Coulomb potential of a static pointlike charge. In connection, the plausible distortion of the Lamb-shift in hydrogenlike atoms is established and the scopes for searching axionlike particles in high-precision atomic spectroscopy and in experiments of Cavendish-type are investigated. Particularly, we show that these hypothetical degrees of freedom are ruled out as plausible candidates for explaining the proton radius anomaly in muonic hydrogen. A certain loophole remains, though, which is linked to the nonrenormalizable nature of axion-electrodynamics.

    hep-phPRD(2018)·7 citations
  12. 12*

    Coherent scattering and macroscopic coherence: Implications for neutrino, dark matter and axion detection

    Evgeny Akhmedov🇩🇪 · Giorgio Arcadi🇩🇪 · Manfred Lindner🇩🇪 · Stefan Vogl🇩🇪

    We study the question of whether coherent neutrino scattering can occur on macroscopic scales, leading to a significant increase of the detection cross section. We concentrate on radiative neutrino scattering on atomic electrons (or on free electrons in a conductor). Such processes can be coherent provided that the net electron recoil momentum, i.e. the momentum transfer from the neutrino minus the momentum of the emitted photon, is sufficiently small. The radiative processes is an attractive possibility as the energy of the emitted photons can be as large as the momentum transfer to the electron system and therefore the problem of detecting extremely low energy recoils can be avoided. The requirement of macroscopic coherence severely constrains the phase space available for the scattered particle and the emitted photon. We show that in the case of the scattering mediated by the usual weak neutral current and charged current interactions this leads to a strong suppression of the elementary cross sections and therefore the requirement of macroscopic coherence results in a reduction rather than an increase of the total detection cross section. However, for the scattering mediated by neutrino magnetic or electric dipole moments coherence effects can actually increase the detection rates. Effects of macroscopic coherence can also allow detection of neutrinos in 100 eV -- a few keV energy range, which is currently not accessible to the experiment. A similar coherent enhancement mechanism can work for relativistic particles in the dark sector, but not for the conventionally considered non-relativistic dark matter.

    hep-phastro-ph.COhep-exnucl-exJHEP(2018)·17 citations
  13. 13*

    Numerical study of multiparticle scattering in theory

    S.V. Demidov🇷🇺 · B.R. Farkhtdinov🇷🇺

    We study numerically classical collisions of waves in theory. These processes correspond to multiparticle scattering in the semiclassical regime. Parametrizing initial and final wavepackets by energy and particle numbers , we find classically allowed region in the parameter space. We describe properties of the scattering solutions at the boundary of the classically allowed region. We comment on the implications of our results for multiparticle production in the quantum regime.

    hep-phhep-thJHEP(2018)·8 citations
  14. 14*

    Loop induced decays in the aligned two-Higgs-doublet model

    Gauhar Abbas🇮🇳 · Diganta Das🇮🇳 · Monalisa Patra🇸🇮

    We present a complete one-loop computation of the decay in the aligned two-Higgs-doublet model. The constraints from the electroweak precision observables, perturbative unitarity, vacuum stability and flavour physics are all taken into account along with the latest Large Hadron Collider searches for the charged Higgs. It is observed that a large enhancement of the branching ratio can be obtained in the limit where there is a large splitting between the charged and pseudo-scalar Higgs masses as well as for the largest allowed values of the alignment parameter . We find that the maximum possible branching ratio in the case of a large mass splitting between and is for GeV which is in the reach of the high luminosity phase of the Large Hadron Collider.

    hep-phPRD(2018)·19 citations
  15. 15*

    Lepton Masses and Mixing from Modular Symmetry

    J. T. Penedo🇮🇹 · S. T. Petcov🇮🇹

    We study models of lepton masses and mixing based on broken modular invariance. We consider invariance under the finite modular group and focus on the minimal scenario where the expectation value of the modulus is the only source of symmetry breaking, such that no flavons need to be introduced. After constructing a basis for the lowest weight modular forms, we build two minimal models, one of which successfully accommodates charged lepton masses and neutrino oscillation data, while predicting the values of the Dirac and Majorana CPV phases.

    hep-phNPB(2019)·269 citations
  16. 16*

    Neutrino Mass Ordering from Oscillations and Beyond: 2018 Status and Future Prospects

    P.F. de Salas🇪🇸 · S. Gariazzo🇪🇸 · O. Mena🇪🇸 · C.A. Ternes🇪🇸 · M. Tórtola🇪🇸

    The ordering of the neutrino masses is a crucial input for a deep understanding of flavor physics, and its determination may provide the key to establish the relationship among the lepton masses and mixings and their analogous properties in the quark sector. The extraction of the neutrino mass ordering is a data-driven field expected to evolve very rapidly in the next decade. In this review, we both analyze the present status and describe the physics of subsequent prospects. Firstly, the different current available tools to measure the neutrino mass ordering are described. Namely, reactor, long-baseline (accelerator and atmospheric) neutrino beams, laboratory searches for beta and neutrinoless double beta decays and observations of the cosmic background radiation and the large scale structure of the universe are carefully reviewed. Secondly, the results from an up-to-date comprehensive global fit are reported: the Bayesian analysis to the 2018 publicly available oscillation and cosmological data sets provides \emph{strong} evidence for the normal neutrino mass ordering versus the inverted scenario, with a significance of 3.5 standard deviations. This preference for the normal neutrino mass ordering is mostly due to neutrino oscillation measurements. Finally, we shall also emphasize the future perspectives for unveiling the neutrino mass ordering. In this regard, apart from describing the expectations from the aforementioned probes, we also focus on those arising from alternative and novel methods, as 21~cm cosmology, core-collapse supernova neutrinos and the direct detection of relic neutrinos.

    hep-phastro-ph.COFront.Astron.Space Sci.(2018)·257 citations
  17. 17*

    Protecting the Stability of the EW Vacuum from Planck-Scale Gravitational Effects

    Vincenzo Branchina🇮🇹 · Filippo Contino🇮🇹 · Apostolos Pilaftsis🇬🇧

    We investigate the stability of the Standard-Model Electroweak (EW) vacuum in the presence of Planck-scale suppressed operators of the type that involve the Higgs field and could in principle be induced by quantum gravity effects. We show how minimal embeddings of the Standard Model (SM) in supergravity (SUGRA) can stabilize the EW vacuum against such operators up to very high values of the induced supersymmetry breaking scale , which may well be above the onset of the so-called SM metastability scale of GeV. In particular, we explicitly demonstrate how discrete symmetries could be invoked to suppress the occurrence of harmful Planck-scale operators of the form to arbitrary higher powers of . We analyze different scenarios of Planck-scale gravitational physics and derive lower limits on the power that is required in order to protect our EW vacuum from dangerous rapid decay. The significance of our results for theories of low-scale quantum gravity is illustrated.

    hep-phPRD(2018)·28 citations
  18. 18*

    Scalar singlet dark matter in non-standard cosmologies

    Nicolás Bernal🇨🇴 · Catarina Cosme🇵🇹 · Tommi Tenkanen🇬🇧 · Ville Vaskonen🇪🇪

    We study production of dark matter (DM) in models with a non-standard expansion history. We consider both freeze-out and freeze-in mechanisms for producing the observed DM abundance in a model where the DM consists of scalar singlet particles coupled to the Standard Model sector via the Higgs portal. We show that a non-standard expansion phase can lead to a significant change in the DM abundance and therefore to observational ramifications. For example, for DM freeze-in the required portal coupling can be much larger, whereas for DM freeze-out much smaller values become allowed. We evaluate the relevant constraints and discuss prospects for direct detection of such DM.

    hep-phastro-ph.COEPJC(2019)·88 citations
  19. 19*

    Internal Robustness of Growth Rate data

    Bryan Sagredo🇨🇱 · Savvas Nesseris🇪🇸 · Domenico Sapone🇨🇱

    We perform an Internal Robustness analysis (iR) to a compilation of the most recent data, using the framework of 1209.1897. The method analyzes combinations of subsets in the data set in a Bayesian model comparison way, potentially finding outliers, subsets of data affected by systematics or new physics. In order to validate our analysis and assess its sensitivity we performed several cross-checks, for example by removing some of the data or by adding artificially contaminated points, while we also generated mock data sets in order to estimate confidence regions of the iR. Applying this methodology, we found no anomalous behavior in the data set, thus validating its internal robustness.

    ↳ astro-ph.COgr-qchep-phPRD(2018)·92 citations
  20. 20*

    Updated Bounds on Sum of Neutrino Masses in Various Cosmological Scenarios

    Shouvik Roy Choudhury🇮🇳 · Sandhya Choubey🇮🇳

    We present strong bounds on the sum of three active neutrino masses () in various cosmological models. We use the following baseline datasets: CMB temperature data from Planck 2015, BAO measurements from SDSS-III BOSS DR12, the newly released SNe Ia dataset from Pantheon Sample, and a prior on the optical depth to reionization from 2016 Planck Intermediate results. We constrain cosmological parameters in model with 3 massive active neutrinos. For this model we find a upper bound of 0.152 eV at 95 C.L. Adding the high- polarization data from Planck strengthens this bound to 0.118 eV, which is very close to the minimum required mass of 0.1 eV for inverted hierarchy. This bound is reduced to 0.110 eV when we also vary r, the tensor to scalar ratio ( model), and add an additional dataset, BK14, the latest data released from the Bicep-Keck collaboration. This bound is further reduced to 0.101 eV in a cosmology with non-phantom dynamical dark energy ( model with for all ). Considering the model and adding the BK14 data again, the bound can be even further reduced to 0.093 eV. For the model without any constraint on , the bounds however relax to 0.276 eV. Adding a prior on the Hubble constant ( km/sec/Mpc) from Hubble Space Telescope (HST), the above mentioned bounds further improve to 0.117 eV, 0.091 eV, 0.085 eV, 0.082 eV, 0.078 eV and 0.247 eV respectively. This substantial improvement is mostly driven by a more than 3 tension between Planck 2015 and HST measurements of and should be taken cautiously. (abstract abridged)

    ↳ astro-ph.COhep-phJCAP(2018)·151 citations
  21. 21*

    Phase Transition in Interacting Boson System at Finite Temperatures

    D. Anchishkin🇺🇦 · I. Mishustin🇩🇪 · H. Stoecker🇩🇪

    Thermodynamical properties of an interacting boson system at finite temperatures and zero chemical potential are studied within the framework of the Skyrme-like mean-field toy model. It is assumed that the mean field contains both attractive and repulsive terms. Self-consistency relations between the mean field and thermodynamic functions are derived. It is shown that for sufficiently strong attractive interactions this system develops a first-order phase transition via formation of Bose condensate. An interesting prediction of the model is that the condensed phase is characterized by a constant total density of particles. The thermodynamical characteristics of the system are calculated for the liquid-gas and condensed phases. The energy density exhibits a jump at the critical temperature.

    ↳ nucl-thhep-phJ.Phys.G(2019)·14 citations
  22. 22*

    Exotics at Belle and perspectives at Belle II

    Elisabetta Prencipe🇩🇪

    The search for multi-quark states beyond the constituent quark model (CQM) has resulted in the discovery of many new exotic states, starting with the observation of the X(3872), discovered by Belle in 2003. Also in the sector of charm-strange physics the CQM does not seem to describe properly all spectrum, despite of theoretical expectations. These new forms of quark bounds clearly show that mesons and baryons are not the only possibilities to be considered. We shortly report in this paper selected recent results on searching for such states at Belle, with the perspectives in the hadron physics program at the Belle II experiment.

    ↳ hep-exhep-phActa Phys.Polon.Supp.(2018)·1 citation
  23. 23*

    Transport peak in thermal spectral function of supersymmetric Yang-Mills plasma at intermediate coupling

    Jorge Casalderrey-Solana🇬🇧 · Sašo Grozdanov🇺🇸 · Andrei O. Starinets🇬🇧

    We study the structure of thermal spectral function of the stress-energy tensor in supersymmetric Yang-Mills theory at intermediate 't Hooft coupling and infinite number of colors. In gauge-string duality, this analysis reduces to the study of classical bulk supergravity with higher-derivative corrections, which correspond to (inverse) coupling corrections on the gauge theory side. We extrapolate the analysis of perturbative leading-order corrections to intermediate coupling by non-perturbatively solving the equations of motion of metric fluctuations dual to the stress-energy tensor at zero spatial momentum. We observe the emergence of a separation of scales in the analytic structure of the thermal correlator associated with two types of characteristic relaxation modes. As a consequence of this separation, the associated spectral function exhibits a narrow structure in the small frequency region which controls the dynamics of transport in the theory and may be described as a transport peak typically found in perturbative, weakly interacting thermal field theories. We compare our results with generic expectations drawn from perturbation theory, where such a structure emerges as a consequence of the existence of quasiparticles.

    ↳ hep-thhep-lathep-phnucl-thPRL(2018)·40 citations
  24. 24*

    On the de Sitter swampland criterion

    David Andriot🇨🇭

    A new swampland criterion has recently been proposed. As a consequence, it forbids the existence of de Sitter solutions in a low energy effective theory of a quantum gravity. However, there exist classical de Sitter solutions of ten-dimensional (10d) type II supergravities, even though they are unstable. This appears at first sight in contradiction with the criterion. Beyond possible doubts on the validity of these solutions, we propose two answers to this apparent puzzle. A first possibility is that the known 10d solutions always exhibit an energy scale of order or higher than a Kaluza-Klein scale, as we argue. A corresponding 4d low energy effective theory would then differ from the usual consistent truncations, and as we explain, would not admit a de Sitter solution. This would reconcile the existence of these 10d de Sitter solutions with the 4d criterion. A second, alternative possibility is to have a refined swampland criterion, that we propose. It forbids to have both the existence and the stability of a de Sitter solution, while unstable solutions are still allowed.

    ↳ hep-thastro-ph.COgr-qchep-phPLB(2018)·252 citations
  25. 25*

    Searching for Decaying and Annihilating Dark Matter with Line Intensity Mapping

    Cyril Creque-Sarbinowski🇺🇸 · Marc Kamionkowski🇺🇸

    The purpose of line-intensity mapping (IM), an emerging tool for extragalactic astronomy and cosmology, is to measure the integrated emission along the line of sight from spectral lines emitted from galaxies and the intergalactic medium. The observed frequency of the line then provides a distance determination allowing the three-dimensional distribution of the emitters to be mapped. Here we discuss the possibility to use these measurements to seek radiative decays or annihilations from dark-matter particles. The photons from monoenergetic decays will be correlated with the mass distribution, which can be determined from galaxy surveys, weak-lensing surveys, or the IM mapping experiments themselves. We discuss how to seek this cross-correlation and then estimate the sensitivity of various IM experiments in the dark-matter mass-lifetime parameter space. We find prospects for improvements of ten orders of magnitude in sensitivity to decaying/annihilating dark matter in the frequency bands targeted for IM experiments.

    ↳ astro-ph.COhep-phPRD(2018)·38 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.