427 results on '"Cui, Yanou"'
Search Results
52. Stochastic gravitational wave background from global cosmic strings
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Chang, Chia-Feng and Cui, Yanou
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- 2020
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53. Detecting Boosted Dark Matter from the Sun with Large Volume Neutrino Detectors
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Berger, Joshua, Cui, Yanou, and Zhao, Yue
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High Energy Physics - Phenomenology ,Astrophysics - High Energy Astrophysical Phenomena ,High Energy Physics - Experiment - Abstract
We study novel scenarios where thermal dark matter (DM) can be efficiently captured in the Sun and annihilate into boosted dark matter. In models with semi-annihilating DM, where DM has a non-minimal stabilization symmetry, or in models with a multi-component DM sector, annihilations of DM can give rise to stable dark sector particles with moderate Lorentz boosts. We investigate both of these possibilities, presenting concrete models as proofs of concept. Both scenarios can yield viable thermal relic DM with masses O(1)-O(100) GeV. Taking advantage of the energetic proton recoils that arise when the boosted DM scatters off matter, we propose a detection strategy which uses large volume terrestrial detectors, such as those designed to detect neutrinos or proton decays. In particular, we propose a search for proton tracks pointing towards the Sun. We focus on signals at Cherenkov-radiation-based detectors such as Super-Kamiokande (SK) and its upgrade Hyper-Kamiokande (HK). We find that with spin-dependent scattering as the dominant DM-nucleus interaction at low energies, boosted DM can leave detectable signals at SK or HK, with sensitivity comparable to DM direct detection experiments while being consistent with current constraints. Our study provides a new search path for DM sectors with non-minimal structure., Comment: 19 pages, 3 figures. Typos corrected, some rewording, results unchanged
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- 2014
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54. Probing Baryogenesis with Displaced Vertices at the LHC
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Cui, Yanou and Shuve, Brian
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Nongalactic Astrophysics ,High Energy Physics - Experiment - Abstract
The generation of the asymmetric cosmic baryon abundance requires a departure from thermal equilibrium in the early universe. In a large class of baryogenesis models, the baryon asymmetry results from the out-of-equilibrium decay of a new, massive particle. We highlight that in the interesting scenario where this particle has a weak scale mass, this out-of-equilibrium condition requires a proper decay length larger than O(1) mm. Such new fields are within reach of the LHC, at which they can be pair produced leaving a distinctive, displaced-vertex signature. This scenario is realized in the recently proposed mechanism of baryogenesis where the baryon asymmetry is produced through the freeze-out and subsequent decay of a meta-stable weakly interacting massive particle ("WIMP baryogenesis"). In analogy to missing energy searches for WIMP dark matter, the LHC is an excellent probe of these new long-lived particles responsible for baryogenesis via the low-background displaced vertex channel. In our paper, we estimate the limits on simplified models inspired by WIMP baryogenesis from two of the most sensitive collider searches by CMS and ATLAS with 8 TeV LHC data. We also estimate the LHC reach at 13 TeV using current strategies, and demonstrate that O(10) improvements in cross-section limits can be achieved by requiring two displaced vertices while lowering kinematic thresholds. For meta-stable WIMPs produced through electroweak interactions, the high luminosity LHC is sensitive to masses up to 2.5 TeV for lifetimes around 1 cm, while for singlets pair-produced through the off-shell-Higgs portal, the LHC is sensitive to production cross sections of O(50) ab for benchmark masses around 150 GeV. Our analysis and proposals also generally apply to displaced vertex signatures from other new physics such as hidden valley models, twin Higgs models and displaced supersymmetry., Comment: 31 pages, 14 figures, 2 tables. Corrected issue with references
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- 2014
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55. (In)direct Detection of Boosted Dark Matter
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Agashe, Kaustubh, Cui, Yanou, Necib, Lina, and Thaler, Jesse
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Nongalactic Astrophysics ,High Energy Physics - Experiment - Abstract
We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. These stable particles are typically a subdominant DM component, but because they are produced with a large Lorentz boost in this process, they can be detected in large volume terrestrial experiments via neutral-current-like interactions with electrons or nuclei. This novel DM signal thus combines the production mechanism associated with indirect detection experiments (i.e. galactic DM annihilation) with the detection mechanism associated with direct detection experiments (i.e. DM scattering off terrestrial targets). Such processes are generically present in multi-component DM scenarios or those with non-minimal DM stabilization symmetries. As a proof of concept, we present a model of two-component thermal relic DM, where the dominant heavy DM species has no tree-level interactions with the standard model and thus largely evades direct and indirect DM bounds. Instead, its thermal relic abundance is set by annihilation into a subdominant lighter DM species, and the latter can be detected in the boosted channel via the same annihilation process occurring today. Especially for dark sector masses in the 10 MeV-10 GeV range, the most promising signals are electron scattering events pointing toward the galactic center. These can be detected in experiments designed for neutrino physics or proton decay, in particular Super-K and its upgrade Hyper-K, as well as the PINGU/MICA extensions of IceCube. This boosted DM phenomenon highlights the distinctive signatures possible from non-minimal dark sectors., Comment: 40 pages, 11 figures, 1 table; v2: references added, appendix B revised; v3: improved presentation of signal/background, added section 4.4 on earth attenuation, version to appear in JCAP; v4: typos fixed, appendix B bounds weakened, conclusions unchanged
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- 2014
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56. Exploring a Dark Sector Through the Higgs Portal at a Lepton Collider
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Chacko, Zackaria, Cui, Yanou, and Hong, Sungwoo
- Subjects
High Energy Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
We investigate the prospects for detecting a hidden sector at an $e^+ e^-$ collider. The hidden sector is assumed to be composed of invisible particles that carry no charges under the Standard Model gauge interactions, and whose primary interactions with ordinary matter are through the Higgs portal. We consider both the cases when the decays of an on-shell Higgs into a pair of hidden sector particles are kinematically allowed, and the case when such decays are kinematically forbidden. We find that at collider energies below a TeV, the most sensitive channel involves production of an on-shell or off-shell Higgs in association with a Z boson, and the subsequent decay of the Higgs into invisible hidden sector states. Focusing on this channel, we find that with order a thousand inverse fb of data at 250 GeV, the decay branching fraction of an on-shell Higgs to invisible hidden sector states can be constrained to lie below half a percent. The corresponding limits on Higgs portal dark matter will be stronger than the bounds from current and upcoming direct detection experiments in much of parameter space. With the same amount of data at 500 GeV, assuming order one couplings, decays of an off-shell Higgs to hidden sector states with a total mass up to about 200 GeV can also be probed. Both the on-shell and off-shell cases represent a significant improvement in sensitivity when compared to the Large Hadron Collider (LHC)., Comment: 7 pages, 6 figures, minor revisions, with added references, new version to appear in Physics Letters B
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- 2013
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57. Natural Baryogenesis from Unnatural Supersymmetry
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Cui, Yanou
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Nongalactic Astrophysics ,High Energy Physics - Theory - Abstract
We demonstrate here that the mini-split version of the Minimal Supersymmetric Standard Model (MSSM) including R-parity violating couplings naturally provides all the necessary ingredients for a novel baryogenesis mechanism. The baryogenesis is triggered by the late decay of a TeV scale bino after its thermal freezeout. A \mu-term larger than the sfermion masses is necessary for obtaining sufficient baryon asymmetry. Two example models of direct baryogenesis and leptogenesis are proposed, with viable parameter spaces presented. The cosmological conditions for the models--in particular, the requirements of a long lifetime of bino and sufficient baryon asymmetry--point towards the mini-split scale of $\sim$ 100-1000 TeV for the sfermion masses. This provides an independent motivation for mini-split SUSY, along with the constraints from flavor physics and Higgs mass measurement. We also discuss the potential multi-pronged search for the signatures of such models, including those at the Large Hadron Collider (LHC) and the low energy experiments at the intensity frontier., Comment: 17 pages, 7 figures
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- 2013
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58. New light on WW scattering at the LHC with W jet tagging
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Cui, Yanou and Han, Zhenyu
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High Energy Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
After the recent discovery of a 125 GeV Higgs-like particle at the Large Hadron Collider (LHC), it is crucial to examine its role in unitarizing high energy W_LW_L scattering, which may reveal its possible deviation from a Standard Model Higgs. We perform an updated study on WW scattering in the semileptonic channel at the LHC, improved by the recently developed W jet tagging method. The resultant statistical significance of a Strongly-Interacting Light Higgs (SILH) model is about 20% larger than that based on the conventionally "gold-plated" dileptonic channel, while 200% more signal events are retained. This allows the discovery of an SILH model if the signal strength is 100% (10%) of a pure Higgsless model, using about 40 (3000) fb^{-1} data at the 14 TeV LHC. Meanwhile, the excellent sensitivity to the anomalous Higgs-W boson coupling makes semileptonic WW scattering an important complement to precision measurements at the Higgs resonance., Comment: 25 pages, 4 figures, version published in Phys. Rev. D
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- 2013
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59. Baryogenesis for WIMPs
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Cui, Yanou and Sundrum, Raman
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We propose a robust, unified framework, in which the similar baryon and dark matter cosmic abundances both arise from the physics of weakly interacting massive particles (WIMPs), with the rough quantitative success of the so-called "WIMP miracle". In particular the baryon asymmetry arises from the decay of a meta-stable WIMP after its thermal freezeout at or below the weak scale. A minimal model and its embedding in R-parity violating (RPV) SUSY are studied as examples. The new mechanism saves RPV SUSY from the potential crisis of washing out primordial baryon asymmetry. Phenomenological implications for the LHC and precision tests are discussed., Comment: 5 pages, 1 figure
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- 2012
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60. Enhanced early galaxy formation in JWST from axion dark matter?
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Bird, Simeon, Chang, Chia-Feng, Cui, Yanou, and Yang, Daneng
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- 2024
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61. Natural Islands for a 125 GeV Higgs in the scale-invariant NMSSM
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Agashe, Kaustubh, Cui, Yanou, and Franceschini, Roberto
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High Energy Physics - Phenomenology - Abstract
We study whether a 125 GeV standard model-like Higgs boson can be accommodated within the scale-invariant NMSSM in a way that is natural in all respects, i.e., not only is the stop mass and hence its loop contribution to Higgs mass of natural size, but we do not allow significant tuning of NMSSM parameters as well. We pursue as much as possible an analytic approach which gives clear insights on various ways to accommodate such a Higgs mass, while conducting complementary numerical analyses. We consider both scenarios with singlet-like state being heavier and lighter than SM-like Higgs. With A-terms being small, we find for the NMSSM to be perturbative up to GUT scale, it is not possible to get 125 GeV Higgs mass, which is true even if we tune parameters of NMSSM. If we allow some of the couplings to become non-perturbative below the GUT scale, then the non-tuned option implies that the singlet self-coupling, kappa, is larger than the singlet-Higgs coupling, lambda, which itself is order 1. This leads to a Landau pole for these couplings close to the weak scale, in particular below ~10^4 TeV. In both the perturbative and non-perturbative NMSSM, allowing large A_lambda, A_kappa gives "more room" to accommodate a 125 GeV Higgs, but a tuning of these A-terms may be needed. In our analysis we also conduct a careful study of the constraints on the parameter space from requiring global stability of the desired vacuum fitting a 125 GeV Higgs, which is complementary to existing literature. In particular, as the singlet-Higgs coupling lambda increases, vacuum stability becomes more serious of an issue., Comment: 34 pages, 4 figures, references added, minor corrections to text and figures, version to be published in JHEP
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- 2012
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62. A WIMPy Baryogenesis Miracle
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Cui, Yanou, Randall, Lisa, and Shuve, Brian
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
We explore models in which weakly interacting massive particle (WIMP) dark matter annihilation is directly responsible for baryogenesis, thereby connecting dark matter with baryogenesis. We call this process "WIMPy baryogenesis". The dark matter relic density in these models, as with conventional WIMP models, is obtained with only order one couplings and TeV-scale masses according to the WIMP miracle. Thus, WIMPy baryogenesis models naturally accommodate weak-scale dark matter. Furthermore, an extension of the WIMP miracle simultaneously explains the observed baryon asymmetry and the correct dark matter abundance. The models we present have the further feature that they create the baryon number asymmetry at the weak scale, thereby avoiding the problems in some models of baryogenesis associated with high reheat temperatures in supersymmetric theories. Some of these models yield observable consequences in ongoing and future experiments., Comment: 30 pages, 17 figures, version to appear in JHEP
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- 2011
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63. Emergent Dark Matter, Baryon, and Lepton Numbers
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Cui, Yanou, Randall, Lisa, and Shuve, Brian
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Extragalactic Astrophysics ,High Energy Physics - Theory - Abstract
We present a new mechanism for transferring a pre-existing lepton or baryon asymmetry to a dark matter asymmetry that relies on mass mixing which is dynamically induced in the early universe. Such mixing can succeed with only generic scales and operators and can give rise to distinctive relationships between the asymmetries in the two sectors. The mixing eliminates the need for the type of additional higher-dimensional operators that are inherent to many current asymmetric dark matter models. We consider several implementations of this idea. In one model, mass mixing is temporarily induced during a two-stage electroweak phase transition in a two Higgs doublet model. In the other class of models, mass mixing is induced by large field vacuum expectation values at high temperatures - either moduli fields or even more generic kinetic terms. Mass mixing models of this type can readily accommodate asymmetric dark matter masses ranging from 1 GeV to 100 TeV and expand the scope of possible relationships between the dark and visible sectors in such models., Comment: 36 pages, 5 figures
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- 2011
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64. Top condensation as a motivated explanation of the top forward-backward asymmetry
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Cui, Yanou, Han, Zhenyu, and Schwartz, Matthew D.
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High Energy Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
Models of top condensation can provide both a compelling solution to the hierarchy problem as well as an explanation of why the top-quark mass is large. The spectrum of such models, in particular topcolor-assisted technicolor, includes top-pions, top-rhos and the top-Higgs, all of which can easily have large top-charm or top-up couplings. Large top-up couplings in particular would lead to a top forward-backward asymmetry through $t$-channel exchange, easily consistent with the Tevatron measurements. Intriguingly, there is destructive interference between the top-mesons and the standard model which conspire to make the overall top pair production rate consistent with the standard model. The rate for same-sign top production is also small due to destructive interference between the neutral top-pion and the top-Higgs. Flavor physics is under control because new physics is mostly confined to the top quark. In this way, top condensation can explain the asymmetry and be consistent with all experimental bounds. There are many additional signatures of topcolor with large tu mixing, such as top(s)+jet(s) events, in which a top and a jet reconstruct a resonance mass, which make these models easily testable at the LHC., Comment: 30 pages, 6 figures
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- 2011
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65. W-jet Tagging: Optimizing the Identification of Boosted Hadronically-Decaying W Bosons
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Cui, Yanou, Han, Zhenyu, and Schwartz, Matthew D.
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High Energy Physics - Phenomenology ,High Energy Physics - Experiment - Abstract
A method is proposed for distinguishing highly boosted hadronically decaying W's (W-jets) from QCD-jets using jet substructure. Previous methods, such as the filtering/mass-drop method, can give a factor of ~2 improvement in S/sqrt(B) for jet pT > 200 GeV. In contrast, a multivariate approach including new discriminants such as R-cores, which characterize the shape of the W-jet, subjet planar flow, and grooming-sensitivities is shown to provide a much larger factor of ~5 improvement in S/sqrt(B). For longitudinally polarized W's, such as those coming from many new physics models, the discrimination is even better. Comparing different Monte Carlo simulations, we observe a sensitivity of some variables to the underlying event; however, even with a conservative estimates, the multivariate approach is very powerful. Applications to semileptonic WW resonance searches and all-hadronic W+jet searches at the LHC are also discussed. Code implementing our W-jet tagging algorithm is publicly available at http://jets.physics.harvard.edu/wtag, Comment: Version to appear in PRD
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- 2010
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66. Fermion Masses in Emergent Electroweak Symmetry Breaking
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Cui, Yanou, Gherghetta, Tony, and Stokes, James
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High Energy Physics - Phenomenology - Abstract
We consider the generation of fermion masses in an emergent model of electroweak symmetry breaking with composite $W,Z$ gauge bosons. A universal bulk fermion profile in a warped extra dimension is used for all fermion flavors. Electroweak symmetry is broken at the UV (or Planck) scale where boundary mass terms are added to generate the fermion flavor structure. This leads to flavor-dependent nonuniversality in the gauge couplings. The effects are suppressed for the light fermion generations but are enhanced for the top quark where the $Zt{\bar t}$ and $Wt{\bar b}$ couplings can deviate at the $10-20%$ level in the minimal setup. By the AdS/CFT correspondence our model implies that electroweak symmetry is not a fundamental gauge symmetry. Instead the Standard Model with massive fermions and $W,Z$ gauge bosons is an effective chiral Lagrangian for some underlying confining strong dynamics at the TeV scale, where mass is generated without a Higgs mechanism., Comment: modified discussion in Sec 3.1, version published in JHEP
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- 2010
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67. General Analysis of Antideuteron Searches for Dark Matter
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Cui, Yanou, Mason, John D., and Randall, Lisa
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High Energy Physics - Phenomenology ,Astrophysics - Cosmology and Extragalactic Astrophysics - Abstract
Low energy cosmic ray antideuterons provide a unique low background channel for indirect detection of dark matter. We compute the cosmic ray flux of antideuterons from hadronic annihilations of dark matter for various Standard Model final states and determine the mass reach of two future experiments (AMS-02 and GAPS) designed to greatly increase the sensitivity of antideuteron detection over current bounds. We consider generic models of scalar, fermion, and massive vector bosons as thermal dark matter, describe their basic features relevant to direct and indirect detection, and discuss the implications of direct detection bounds on models of dark matter as a thermal relic. We also consider specific dark matter candidates and assess their potential for detection via antideuterons from their hadronic annihilation channels. Since the dark matter mass reach of the GAPS experiment can be well above 100 GeV, we find that antideuterons can be a good indirect detection channel for a variety of thermal relic electroweak scale dark matter candidates, even when the rate for direct detection is highly suppressed., Comment: 44 pages, 15 Figures
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- 2010
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68. Emergent Electroweak Symmetry Breaking with Composite W, Z Bosons
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Cui, Yanou, Gherghetta, Tony, and Wells, James D.
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High Energy Physics - Phenomenology ,High Energy Physics - Theory - Abstract
We present a model of electroweak symmetry breaking in a warped extra dimension where electroweak symmetry is broken at the UV (or Planck) scale. An underlying conformal symmetry is broken at the IR (or TeV) scale generating masses for the electroweak gauge bosons without invoking a Higgs mechanism. By the AdS/CFT correspondence the W,Z bosons are identified as composite states of a strongly-coupled gauge theory, suggesting that electroweak symmetry breaking is an emergent phenomenon at the IR scale. The model satisfies electroweak precision tests with reasonable fits to the S and T parameter. In particular the T parameter is sufficiently suppressed since the model naturally admits a custodial SU(2) symmetry. The composite nature of the W,Z-bosons provide a novel possibility of unitarizing WW scattering via form factor suppression. Constraints from LEP and the Tevatron as well as discovery opportunities at the LHC are discussed for these composite electroweak gauge bosons., Comment: 39 pages, 4 figures
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- 2009
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69. Candidates for Inelastic Dark Matter
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Cui, Yanou, Morrissey, David E., Poland, David, and Randall, Lisa
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High Energy Physics - Phenomenology - Abstract
Although we have yet to determine whether the DAMA data represents a true discovery of new physics, among such interpretations inelastic dark matter (IDM) can match the energy spectrum of DAMA very well while not contradicting the results of other direct detection searches. In this paper we investigate the general properties that a viable IDM candidate must have and search for simple models that realize these properties in natural ways. We begin by determining the regions of IDM parameter space that are allowed by direct detection searches including DAMA, paying special attention to larger IDM masses. We observe that an inelastic dark matter candidate with electroweak interactions can naturally satisfy observational constraints while simultaneously yielding the correct thermal relic abundance. We comment on several other proposed dark matter explanations for the DAMA signal and demonstrate that one of the proposed alternatives -- elastic scattering of dark matter off electrons -- is strongly disfavored when the modulated and unmodulated DAMA spectral data are taken into account. We then outline the general essential features of IDM models in which inelastic scattering off nuclei is mediated by the exchange of a massive gauge boson, and construct natural models in the context of a warped extra dimension and supersymmetry., Comment: 44 pages, 6 figures, added references
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- 2009
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70. Unraveling cosmological anisotropies within stochastic gravitational wave backgrounds
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Cui, Yanou, primary, Kumar, Soubhik, additional, Sundrum, Raman, additional, and Tsai, Yuhsin, additional
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- 2023
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71. Non-Thermal Dark Matter from Cosmic Strings
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Cui, Yanou and Morrissey, David E.
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High Energy Physics - Phenomenology ,Astrophysics - Abstract
Cosmic strings can be created in the early universe during symmetry-breaking phase transitions, such as might arise if the gauge structure of the standard model is extended by additional U(1) factors at high energies. Cosmic strings present in the early universe form a network of long horizon-length segments, as well as a population of closed string loops. The closed loops are unstable against decay, and can be a source of non-thermal particle production. In this work we compute the density of WIMP dark matter formed by the decay of gauge theory cosmic string loops derived from a network of long strings in the scaling regime or under the influence of frictional forces. We find that for symmetry breaking scales larger than 10^10 GeV, this mechanism has the potential to account for the observed relic density of dark matter. For symmetry breaking scales lower than this, the density of dark matter created by loop decays from a scaling string network lies below the observed value. In particular, the cosmic strings originating from a U(1) gauge symmetry broken near the electroweak scale, that could lead to a massive Z' gauge boson observable at the LHC, produce a negligibly small dark matter relic density by this mechanism., Comment: 22 pages, 4 figures, added discussion about boosted decay products from loop cusps
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- 2008
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72. Cosmic Strings from Supersymmetric Flat Directions
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Cui, Yanou, Martin, Stephen P., Morrissey, David E., and Wells, James D.
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High Energy Physics - Phenomenology ,Astrophysics ,High Energy Physics - Theory - Abstract
Flat directions are a generic feature of the scalar potential in supersymmetric gauge field theories. They can arise, for example, from D-terms associated with an extra abelian gauge symmetry. Even when supersymmetry is broken softly, there often remain directions in the scalar field space along which the potential is almost flat. Upon breaking a gauge symmetry along one of these almost flat directions, cosmic strings may form. Relative to the standard cosmic string picture based on the abelian Higgs model, these flat-direction cosmic strings have the extreme Type-I properties of a thin gauge core surrounded by a much wider scalar field profile. We perform a comprehensive study of the microscopic, macroscopic, and observational characteristics of this class of strings. We find many differences from the standard string scenario, including stable higher winding mode strings, the dynamical formation of higher mode strings from lower ones, and a resultant multi-tension scaling string network in the early universe. These strings are only moderately constrained by current observations, and their gravitational wave signatures may be detectable at future gravity wave detectors. Furthermore, there is the interesting but speculative prospect that the decays of cosmic string loops in the early universe could be a source of ultra-high energy cosmic rays or non-thermal dark matter. We also compare the observational signatures of flat-direction cosmic strings with those of ordinary cosmic strings as well as (p,q) cosmic strings motivated by superstring theory., Comment: 58 pages, 16 figures, v2. accepted to PRD, added comments about baryogenesis and boosted decay products from cusp annihilation
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- 2007
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73. Narrow Trans-TeV Higgs Bosons and $H\to hh$ Decays: Two LHC Search Paths for a Hidden Sector Higgs Boson
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Bowen, Matthew, Cui, Yanou, and Wells, James
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High Energy Physics - Phenomenology - Abstract
We consider the addition of a condensing singlet scalar field to the Standard Model. Such a scenario may be motivated by any number of theoretical ideas, including the common result in string-inspired model building of singlet scalar fields charged under some hidden sector gauge symmetry. For concreteness, we specify an example model of this type, and consider the relevant constraints on Higgs physics, such as triviality, perturbative unitarity and precision electroweak analysis. We then show that there are two unique features of the phenomenology that present opportunities for discovery at the Large Hadron Collider (LHC). First, it is possible to identify and discover a narrow trans-TeV Higgs boson in this scenario -- a mass scale that is well above the scale at which it is meaningful to discuss a SM Higgs boson. Second, the decays of the heavier scalar state into the lighter Higgs bosons can proceed at a high rate and may be the first discovery mode in the Higgs sector., Comment: 21 pages, 5 figures
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- 2007
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74. Adjoint Chiral Supermultiplets and Their Phenomenology
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Cui, Yanou
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High Energy Physics - Phenomenology ,High Energy Physics - Theory - Abstract
Matter fields in the MSSM are chiral supermultiplets in fundamental (or singlet) representations of the standard model gauge group. In this paper we introduce chiral superfields in the adjoint representation of $SU(3)_C$ and study the effective field theory and phenomenology of them. These states are well motivated by intersecting D-brane models in which additional massless adjoint chiral supermultiplets appear generically in the low energy spectrum. Although it has been pointed out that the existence of these additional fields may make it difficult to obtain asymptotic freedom, we demonstrate that this consideration does not rule out the existence of adjoints. The QCD gauge coupling can be perturbative up to a sufficiently high scale, and therefore a perturbative description for a D-brane model is valid. The full supersymmetric and soft SUSY breaking Lagrangians and the resulting renormalization group equations are given. Phenomenological aspects of the adjoint matter are also studied, including the decay and production processes. The similarity in gauge interaction between the adjoint fermion and gluino facilitates our study on these aspects. It is found that these adjoint multiplets can give detectable signals at colliders and satisfy the constraints from cosmology., Comment: 18 pages, 3 figures; minor corrections, references added
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- 2006
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75. AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
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El-Neaj, Yousef Abou, Alpigiani, Cristiano, Amairi-Pyka, Sana, Araújo, Henrique, Balaž, Antun, Bassi, Angelo, Bathe-Peters, Lars, Battelier, Baptiste, Belić, Aleksandar, Bentine, Elliot, Bernabeu, José, Bertoldi, Andrea, Bingham, Robert, Blas, Diego, Bolpasi, Vasiliki, Bongs, Kai, Bose, Sougato, Bouyer, Philippe, Bowcock, Themis, Bowden, William, Buchmueller, Oliver, Burrage, Clare, Calmet, Xavier, Canuel, Benjamin, Caramete, Laurentiu-Ioan, Carroll, Andrew, Cella, Giancarlo, Charmandaris, Vassilis, Chattopadhyay, Swapan, Chen, Xuzong, Chiofalo, Maria Luisa, Coleman, Jonathon, Cotter, Joseph, Cui, Yanou, Derevianko, Andrei, De Roeck, Albert, Djordjevic, Goran S., Dornan, Peter, Doser, Michael, Drougkakis, Ioannis, Dunningham, Jacob, Dutan, Ioana, Easo, Sajan, Elertas, Gedminas, Ellis, John, El Sawy, Mai, Fassi, Farida, Felea, Daniel, Feng, Chen-Hao, Flack, Robert, Foot, Chris, Fuentes, Ivette, Gaaloul, Naceur, Gauguet, Alexandre, Geiger, Remi, Gibson, Valerie, Giudice, Gian, Goldwin, Jon, Grachov, Oleg, Graham, Peter W., Grasso, Dario, van der Grinten, Maurits, Gündogan, Mustafa, Haehnelt, Martin G., Harte, Tiffany, Hees, Aurélien, Hobson, Richard, Hogan, Jason, Holst, Bodil, Holynski, Michael, Kasevich, Mark, Kavanagh, Bradley J., von Klitzing, Wolf, Kovachy, Tim, Krikler, Benjamin, Krutzik, Markus, Lewicki, Marek, Lien, Yu-Hung, Liu, Miaoyuan, Luciano, Giuseppe Gaetano, Magnon, Alain, Mahmoud, Mohammed Attia, Malik, Sarah, McCabe, Christopher, Mitchell, Jeremiah, Pahl, Julia, Pal, Debapriya, Pandey, Saurabh, Papazoglou, Dimitris, Paternostro, Mauro, Penning, Bjoern, Peters, Achim, Prevedelli, Marco, Puthiya-Veettil, Vishnupriya, Quenby, John, Rasel, Ernst, Ravenhall, Sean, Ringwood, Jack, Roura, Albert, Sabulsky, Dylan, Sameed, Muhammed, Sauer, Ben, Schäffer, Stefan Alaric, Schiller, Stephan, Schkolnik, Vladimir, Schlippert, Dennis, Schubert, Christian, Sfar, Haifa Rejeb, Shayeghi, Armin, Shipsey, Ian, Signorini, Carla, Singh, Yeshpal, Soares-Santos, Marcelle, Sorrentino, Fiodor, Sumner, Timothy, Tassis, Konstantinos, Tentindo, Silvia, Tino, Guglielmo Maria, Tinsley, Jonathan N., Unwin, James, Valenzuela, Tristan, Vasilakis, Georgios, Vaskonen, Ville, Vogt, Christian, Webber-Date, Alex, Wenzlawski, André, Windpassinger, Patrick, Woltmann, Marian, Yazgan, Efe, Zhan, Ming-Sheng, Zou, Xinhao, and Zupan, Jure
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- 2020
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76. Detectable gravitational wave signals from inflationary preheating
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Cui, Yanou, primary and Sfakianakis, Evangelos I., additional
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- 2023
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77. Cosmology with the Laser Interferometer Space Antenna
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A. G. Leventis Foundation, Academy of Finland, Onassis Foundation, Ministero dell'Istruzione, dell'Università e della Ricerca, Agenzia Spaziale Italiana, Comunidad de Madrid, Ministerio de Universidades (España), Eusko Jaurlaritza, Fondation Francqui, Centre National D'Etudes Spatiales (France), Ben-Gurion University of the Negev, Israel Academy of Sciences and Humanities, Council for Higher Education (Israel), Generalitat de Catalunya, Czech Science Foundation, Delta Institute for Theoretical Physics, Department of Energy (US), German Research Foundation, Ministry of Education, Youth and Sports (Czech Republic), European Commission, Foundation for Science and Technology, Fondation CFM pour la Recherche, Agence Nationale de la Recherche (France), National Fund for Scientific Research (Belgium), Fundação para a Ciência e a Tecnologia (Portugal), Generalitat Valenciana, Ministry of Research, Innovation and Science (Ontario), Japan Society for the Promotion of Science, Ministerio de Ciencia e Innovación (España), Israel Science Foundation, Kavli Foundation, Minerva Foundation, National Aeronautics and Space Administration (US), Netherlands Organization for Scientific Research, Indian Institute of Science, National Science Foundation (US), National Science Centre (Poland), Fundação de Amparo à Pesquisa do Estado de São Paulo Minas Gerais, Royal Society (UK), Shota Rustaveli National Science Foundation, Simons Foundation, Swiss National Science Foundation, Science and Technology Facilities Council (UK), Swiss Competence Center for Energy Research, Nardini, Germano [0000-0002-3523-0477], Auclair, Pierre, Bacon, David, Baker, Tessa, Barreiro, Tiago, Bartolo, Nicola, Belgacem, Enis, Bellomo, Nicola, Ben-Dayan, Ido, Bertacca, Daniele, Besancon, Marc, Blanco-Pillado, Jose J., Blas, Diego, Boileau, Guillaume, Calcagni, Gianluca, Caldwell, Robert, Caprini, Chiara, Carbone, Carmelita, Chang, Chia Feng, Chen, Hsin Yu, Christensen, Nelson, Clesse, Sebastien, Comelli, Denis, Congedo, Giuseppe, Contaldi, Carlo, Crisostomi, Marco, Croon, Djuna, Cui, Yanou, Cusin, Giulia, Cutting, Daniel, Dalang, Charles, De Luca, Valerio, Pozzo, Walter Del, Desjacques, Vincent, Dimastrogiovanni, Emanuela, Dorsch, Glauber C., Ezquiaga, Jose Maria, Fasiello, Matteo, Figueroa, Daniel G., Flauger, Raphael, Franciolini, Gabriele, Frusciante, Noemi, Fumagalli, Jacopo, García-Bellido, Juan, Gould, Oliver, Holz, Daniel, Iacconi, Laura, Jain, Rajeev Kumar, Jenkins, Alexander C., Jinno, Ryusuke, Joana, Cristian, Karnesis, Nikolaos, Konstandin, Thomas, Koyama, Kazuya, Kozaczuk, Jonathan, Kuroyanagi, Sachiko, Laghi, Danny, Lewicki, Marek, Lombriser, Lucas, Madge, Eric, Maggiore, Michele, Malhotra, Ameek, Mancarella, Michele, Mandic, Vuk, Mangiagli, Alberto, Matarrese, Sabino, Mazumdar, Anupam, Mukherjee, Suvodip, Musco, Ilia, Nardini, Germano, No, Jose Miguel, Papanikolaou, Theodoros, Peloso, Marco, Pieroni, Mauro, Pilo, Luigi, Raccanelli, Alvise, Renaux-Petel, Sébastien, Renzini, Arianna I., Ricciardone, Angelo, Riotto, Antonio, Romano, Joseph D., Rollo, Rocco, Pol, Alberto Roper, Morales, Ester Ruiz, Sakellariadou, Mairi, Saltas, Ippocratis D., Scalisi, Marco, Schmitz, Kai, Schwaller, Pedro, Sergijenko, Olga, Servant, Geraldine, Simakachorn, Peera, Sorbo, Lorenzo, Sousa, Lara, Speri, Lorenzo, Steer, Danièle A., Tamanini, Nicola, Tasinato, Gianmassimo, Torrado, Jesús, Unal, Caner, Vennin, Vincent, A. G. Leventis Foundation, Academy of Finland, Onassis Foundation, Ministero dell'Istruzione, dell'Università e della Ricerca, Agenzia Spaziale Italiana, Comunidad de Madrid, Ministerio de Universidades (España), Eusko Jaurlaritza, Fondation Francqui, Centre National D'Etudes Spatiales (France), Ben-Gurion University of the Negev, Israel Academy of Sciences and Humanities, Council for Higher Education (Israel), Generalitat de Catalunya, Czech Science Foundation, Delta Institute for Theoretical Physics, Department of Energy (US), German Research Foundation, Ministry of Education, Youth and Sports (Czech Republic), European Commission, Foundation for Science and Technology, Fondation CFM pour la Recherche, Agence Nationale de la Recherche (France), National Fund for Scientific Research (Belgium), Fundação para a Ciência e a Tecnologia (Portugal), Generalitat Valenciana, Ministry of Research, Innovation and Science (Ontario), Japan Society for the Promotion of Science, Ministerio de Ciencia e Innovación (España), Israel Science Foundation, Kavli Foundation, Minerva Foundation, National Aeronautics and Space Administration (US), Netherlands Organization for Scientific Research, Indian Institute of Science, National Science Foundation (US), National Science Centre (Poland), Fundação de Amparo à Pesquisa do Estado de São Paulo Minas Gerais, Royal Society (UK), Shota Rustaveli National Science Foundation, Simons Foundation, Swiss National Science Foundation, Science and Technology Facilities Council (UK), Swiss Competence Center for Energy Research, Nardini, Germano [0000-0002-3523-0477], Auclair, Pierre, Bacon, David, Baker, Tessa, Barreiro, Tiago, Bartolo, Nicola, Belgacem, Enis, Bellomo, Nicola, Ben-Dayan, Ido, Bertacca, Daniele, Besancon, Marc, Blanco-Pillado, Jose J., Blas, Diego, Boileau, Guillaume, Calcagni, Gianluca, Caldwell, Robert, Caprini, Chiara, Carbone, Carmelita, Chang, Chia Feng, Chen, Hsin Yu, Christensen, Nelson, Clesse, Sebastien, Comelli, Denis, Congedo, Giuseppe, Contaldi, Carlo, Crisostomi, Marco, Croon, Djuna, Cui, Yanou, Cusin, Giulia, Cutting, Daniel, Dalang, Charles, De Luca, Valerio, Pozzo, Walter Del, Desjacques, Vincent, Dimastrogiovanni, Emanuela, Dorsch, Glauber C., Ezquiaga, Jose Maria, Fasiello, Matteo, Figueroa, Daniel G., Flauger, Raphael, Franciolini, Gabriele, Frusciante, Noemi, Fumagalli, Jacopo, García-Bellido, Juan, Gould, Oliver, Holz, Daniel, Iacconi, Laura, Jain, Rajeev Kumar, Jenkins, Alexander C., Jinno, Ryusuke, Joana, Cristian, Karnesis, Nikolaos, Konstandin, Thomas, Koyama, Kazuya, Kozaczuk, Jonathan, Kuroyanagi, Sachiko, Laghi, Danny, Lewicki, Marek, Lombriser, Lucas, Madge, Eric, Maggiore, Michele, Malhotra, Ameek, Mancarella, Michele, Mandic, Vuk, Mangiagli, Alberto, Matarrese, Sabino, Mazumdar, Anupam, Mukherjee, Suvodip, Musco, Ilia, Nardini, Germano, No, Jose Miguel, Papanikolaou, Theodoros, Peloso, Marco, Pieroni, Mauro, Pilo, Luigi, Raccanelli, Alvise, Renaux-Petel, Sébastien, Renzini, Arianna I., Ricciardone, Angelo, Riotto, Antonio, Romano, Joseph D., Rollo, Rocco, Pol, Alberto Roper, Morales, Ester Ruiz, Sakellariadou, Mairi, Saltas, Ippocratis D., Scalisi, Marco, Schmitz, Kai, Schwaller, Pedro, Sergijenko, Olga, Servant, Geraldine, Simakachorn, Peera, Sorbo, Lorenzo, Sousa, Lara, Speri, Lorenzo, Steer, Danièle A., Tamanini, Nicola, Tasinato, Gianmassimo, Torrado, Jesús, Unal, Caner, and Vennin, Vincent
- Abstract
The Laser Interferometer Space Antenna (LISA) has two scientific objectives of cosmological focus: to probe the expansion rate of the universe, and to understand stochastic gravitational-wave backgrounds and their implications for early universe and particle physics, from the MeV to the Planck scale. However, the range of potential cosmological applications of gravitational-wave observations extends well beyond these two objectives. This publication presents a summary of the state of the art in LISA cosmology, theory and methods, and identifies new opportunities to use gravitational-wave observations by LISA to probe the universe.
- Published
- 2023
78. Probing the pre-BBN universe with gravitational waves from cosmic strings
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Cui, Yanou, Lewicki, Marek, Morrissey, David E., and Wells, James D.
- Published
- 2019
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79. Shining light on cosmogenic axions with neutrino experiments
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Cui, Yanou, primary, Kuo, Jui-Lin, additional, Pradler, Josef, additional, and Tsai, Yu-Dai, additional
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- 2022
- Full Text
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80. Detection of early-universe gravitational-wave signatures and fundamental physics
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Caldwell, Robert, primary, Cui, Yanou, additional, Guo, Huai-Ke, additional, Mandic, Vuk, additional, Mariotti, Alberto, additional, No, Jose Miguel, additional, Ramsey-Musolf, Michael J., additional, Sakellariadou, Mairi, additional, Sinha, Kuver, additional, Wang, Lian-Tao, additional, White, Graham, additional, Zhao, Yue, additional, An, Haipeng, additional, Bian, Ligong, additional, Caprini, Chiara, additional, Clesse, Sebastien, additional, Cline, James M., additional, Cusin, Giulia, additional, Fornal, Bartosz, additional, Jinno, Ryusuke, additional, Laurent, Benoit, additional, Levi, Noam, additional, Lyu, Kun-Feng, additional, Martinez, Mario, additional, Miller, Andrew L., additional, Redigolo, Diego, additional, Scarlata, Claudia, additional, Sevrin, Alexander, additional, Haghi, Barmak Shams Es, additional, Shu, Jing, additional, Siemens, Xavier, additional, Steer, Danièle A., additional, Sundrum, Raman, additional, Tamarit, Carlos, additional, Weir, David J., additional, Xie, Ke-Pan, additional, Yang, Feng-Wei, additional, and Zhou, Siyi, additional
- Published
- 2022
- Full Text
- View/download PDF
81. Cold atoms in space: community workshop summary and proposed road-map
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Alonso, Iván, primary, Alpigiani, Cristiano, additional, Altschul, Brett, additional, Araújo, Henrique, additional, Arduini, Gianluigi, additional, Arlt, Jan, additional, Badurina, Leonardo, additional, Balaž, Antun, additional, Bandarupally, Satvika, additional, Barish, Barry C., additional, Barone, Michele, additional, Barsanti, Michele, additional, Bass, Steven, additional, Bassi, Angelo, additional, Battelier, Baptiste, additional, Baynham, Charles F. A., additional, Beaufils, Quentin, additional, Belić, Aleksandar, additional, Bergé, Joel, additional, Bernabeu, Jose, additional, Bertoldi, Andrea, additional, Bingham, Robert, additional, Bize, Sébastien, additional, Blas, Diego, additional, Bongs, Kai, additional, Bouyer, Philippe, additional, Braitenberg, Carla, additional, Brand, Christian, additional, Braxmaier, Claus, additional, Bresson, Alexandre, additional, Buchmueller, Oliver, additional, Budker, Dmitry, additional, Bugalho, Luís, additional, Burdin, Sergey, additional, Cacciapuoti, Luigi, additional, Callegari, Simone, additional, Calmet, Xavier, additional, Calonico, Davide, additional, Canuel, Benjamin, additional, Caramete, Laurentiu-Ioan, additional, Carraz, Olivier, additional, Cassettari, Donatella, additional, Chakraborty, Pratik, additional, Chattopadhyay, Swapan, additional, Chauhan, Upasna, additional, Chen, Xuzong, additional, Chen, Yu-Ao, additional, Chiofalo, Maria Luisa, additional, Coleman, Jonathon, additional, Corgier, Robin, additional, Cotter, J. P., additional, Michael Cruise, A., additional, Cui, Yanou, additional, Davies, Gavin, additional, De Roeck, Albert, additional, Demarteau, Marcel, additional, Derevianko, Andrei, additional, Di Clemente, Marco, additional, Djordjevic, Goran S., additional, Donadi, Sandro, additional, Doré, Olivier, additional, Dornan, Peter, additional, Doser, Michael, additional, Drougakis, Giannis, additional, Dunningham, Jacob, additional, Easo, Sajan, additional, Eby, Joshua, additional, Elertas, Gedminas, additional, Ellis, John, additional, Evans, David, additional, Examilioti, Pandora, additional, Fadeev, Pavel, additional, Fanì, Mattia, additional, Fassi, Farida, additional, Fattori, Marco, additional, Fedderke, Michael A., additional, Felea, Daniel, additional, Feng, Chen-Hao, additional, Ferreras, Jorge, additional, Flack, Robert, additional, Flambaum, Victor V., additional, Forsberg, René, additional, Fromhold, Mark, additional, Gaaloul, Naceur, additional, Garraway, Barry M., additional, Georgousi, Maria, additional, Geraci, Andrew, additional, Gibble, Kurt, additional, Gibson, Valerie, additional, Gill, Patrick, additional, Giudice, Gian F., additional, Goldwin, Jon, additional, Gould, Oliver, additional, Grachov, Oleg, additional, Graham, Peter W., additional, Grasso, Dario, additional, Griffin, Paul F., additional, Guerlin, Christine, additional, Gündoğan, Mustafa, additional, Gupta, Ratnesh K., additional, Haehnelt, Martin, additional, Hanımeli, Ekim T., additional, Hawkins, Leonie, additional, Hees, Aurélien, additional, Henderson, Victoria A., additional, Herr, Waldemar, additional, Herrmann, Sven, additional, Hird, Thomas, additional, Hobson, Richard, additional, Hock, Vincent, additional, Hogan, Jason M., additional, Holst, Bodil, additional, Holynski, Michael, additional, Israelsson, Ulf, additional, Jeglič, Peter, additional, Jetzer, Philippe, additional, Juzeliūnas, Gediminas, additional, Kaltenbaek, Rainer, additional, Kamenik, Jernej F., additional, Kehagias, Alex, additional, Kirova, Teodora, additional, Kiss-Toth, Marton, additional, Koke, Sebastian, additional, Kolkowitz, Shimon, additional, Kornakov, Georgy, additional, Kovachy, Tim, additional, Krutzik, Markus, additional, Kumar, Mukesh, additional, Kumar, Pradeep, additional, Lämmerzahl, Claus, additional, Landsberg, Greg, additional, Le Poncin-Lafitte, Christophe, additional, Leibrandt, David R., additional, Lévèque, Thomas, additional, Lewicki, Marek, additional, Li, Rui, additional, Lipniacka, Anna, additional, Lisdat, Christian, additional, Liu, Mia, additional, Lopez-Gonzalez, J. L., additional, Loriani, Sina, additional, Louko, Jorma, additional, Luciano, Giuseppe Gaetano, additional, Lundblad, Nathan, additional, Maddox, Steve, additional, Mahmoud, M. A., additional, Maleknejad, Azadeh, additional, March-Russell, John, additional, Massonnet, Didier, additional, McCabe, Christopher, additional, Meister, Matthias, additional, Mežnaršič, Tadej, additional, Micalizio, Salvatore, additional, Migliaccio, Federica, additional, Millington, Peter, additional, Milosevic, Milan, additional, Mitchell, Jeremiah, additional, Morley, Gavin W., additional, Müller, Jürgen, additional, Murphy, Eamonn, additional, Müstecaplıoğlu, Özgür E., additional, O’Shea, Val, additional, Oi, Daniel K. L., additional, Olson, Judith, additional, Pal, Debapriya, additional, Papazoglou, Dimitris G., additional, Pasatembou, Elizabeth, additional, Paternostro, Mauro, additional, Pawlowski, Krzysztof, additional, Pelucchi, Emanuele, additional, Pereira dos Santos, Franck, additional, Peters, Achim, additional, Pikovski, Igor, additional, Pilaftsis, Apostolos, additional, Pinto, Alexandra, additional, Prevedelli, Marco, additional, Puthiya-Veettil, Vishnupriya, additional, Quenby, John, additional, Rafelski, Johann, additional, Rasel, Ernst M., additional, Ravensbergen, Cornelis, additional, Reguzzoni, Mirko, additional, Richaud, Andrea, additional, Riou, Isabelle, additional, Rothacher, Markus, additional, Roura, Albert, additional, Ruschhaupt, Andreas, additional, Sabulsky, Dylan O., additional, Safronova, Marianna, additional, Saltas, Ippocratis D., additional, Salvi, Leonardo, additional, Sameed, Muhammed, additional, Saurabh, Pandey, additional, Schäffer, Stefan, additional, Schiller, Stephan, additional, Schilling, Manuel, additional, Schkolnik, Vladimir, additional, Schlippert, Dennis, additional, Schmidt, Piet O., additional, Schnatz, Harald, additional, Schneider, Jean, additional, Schneider, Ulrich, additional, Schreck, Florian, additional, Schubert, Christian, additional, Shayeghi, Armin, additional, Sherrill, Nathaniel, additional, Shipsey, Ian, additional, Signorini, Carla, additional, Singh, Rajeev, additional, Singh, Yeshpal, additional, Skordis, Constantinos, additional, Smerzi, Augusto, additional, Sopuerta, Carlos F., additional, Sorrentino, Fiodor, additional, Sphicas, Paraskevas, additional, Stadnik, Yevgeny V., additional, Stefanescu, Petruta, additional, Tarallo, Marco G., additional, Tentindo, Silvia, additional, Tino, Guglielmo M., additional, Tinsley, Jonathan N., additional, Tornatore, Vincenza, additional, Treutlein, Philipp, additional, Trombettoni, Andrea, additional, Tsai, Yu-Dai, additional, Tuckey, Philip, additional, Uchida, Melissa A., additional, Valenzuela, Tristan, additional, Van Den Bossche, Mathias, additional, Vaskonen, Ville, additional, Verma, Gunjan, additional, Vetrano, Flavio, additional, Vogt, Christian, additional, von Klitzing, Wolf, additional, Waller, Pierre, additional, Walser, Reinhold, additional, Wille, Eric, additional, Williams, Jason, additional, Windpassinger, Patrick, additional, Wittrock, Ulrich, additional, Wolf, Peter, additional, Woltmann, Marian, additional, Wörner, Lisa, additional, Xuereb, André, additional, Yahia, Mohamed, additional, Yazgan, Efe, additional, Yu, Nan, additional, Zahzam, Nassim, additional, Zambrini Cruzeiro, Emmanuel, additional, Zhan, Mingsheng, additional, Zou, Xinhao, additional, Zupan, Jure, additional, and Zupanič, Erik, additional
- Published
- 2022
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82. Probing Leptogenesis with the Cosmological Collider
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Cui, Yanou, primary and Xianyu, Zhong-Zhi, additional
- Published
- 2022
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- View/download PDF
83. Cold atoms in space: community workshop summary and proposed road-map
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Müstecaplıoğlu, Özgür Esat (ORCID 0000-0002-9134-3951 & YÖK ID 1674), Alonso, Ivan; Alpigiani, Cristiano; Altschul, Brett; Araujo, Henrique; Arduini, Gianluigi; Arlt, Jan; Badurina, Leonardo; Balaz, Antun; Bandarupally, Satvika; Barish, Barry C.; Barone, Michele; Barsanti, Michele; Bass, Steven; Bassi, Angelo; Battelier, Baptiste; Baynham, Charles F. A.; Beaufils, Quentin; Berge, Joel; Bernabeu, Jose; Bertoldi, Andrea; Bingham, Robert; Bize, Sebastien; Blas, Diego; Bongs, Kai; Bouyer, Philippe; Braitenberg, Carla; Brand, Christian; Braxmaier, Claus; Bresson, Alexandre; Buchmueller, Oliver; Budker, Dmitry; Bugalho, Luis; Burdin, Sergey; Cacciapuoti, Luigi; Callegari, Simone; Calmet, Xavier; Calonico, Davide; Canuel, Benjamin; Caramete, Laurentiu-Ioan; Carraz, Olivier; Cassettari, Donatella; Chakraborty, Pratik; Chattopadhyay, Swapan; Chauhan, Upasna; Chen, Xuzong; Chen, Yu-Ao; Chiofalo, Maria Luisa; Coleman, Jonathon; Corgier, Robin; Cotter, J. P.; Cruise, A. Michael; Cui, Yanou; Davies, Gavin; De Roeck, Albert; Demarteau, Marcel; Derevianko, Andrei; Di Clemente, Marco; Djordjevic, Goran S.; Donadi, Sandro; Dore, Olivier; Dornan, Peter; Doser, Michael; Drougakis, Giannis; Dunningham, Jacob; Easo, Sajan; Eby, Joshua; Elertas, Gedminas; Ellis, John; Evans, David; Examilioti, Pandora; Fadeev, Pavel; Fani, Mattia; Fassi, Farida; Fattori, Marco; Fedderke, Michael A.; Felea, Daniel; Feng, Chen-Hao; Ferreras, Jorge; Flack, Robert; Flambaum, Victor V.; Forsberg, Rene; Fromhold, Mark; Gaaloul, Naceur; Garraway, Barry M.; Georgousi, Maria; Geraci, Andrew; Gibble, Kurt; Gibson, Valerie; Gill, Patrick; Giudice, GianF; Goldwin, Jon; Gould, Oliver; Grachov, Oleg; Graham, Peter W.; Grasso, Dario; Griffin, PaulF; Guerlin, Christine; Gupta, Ratnesh K.; Haehnelt, Martin; Hawkins, Leonie; Hees, Aurelien; Henderson, Victoria A.; Herr, Waldemar; Herrmann, Sven; Hird, Thomas; Hobson, Richard; Hock, Vincent; Hogan, Jason M.; Holst, Bodil; Holynski, Michael; Israelsson, Ulf; Jeglic, Peter; Jetzer, Philippe; Juzeliunas, Gediminas; Kaltenbaek, Rainer; Kamenik, College of Sciences, Department of Physics, Müstecaplıoğlu, Özgür Esat (ORCID 0000-0002-9134-3951 & YÖK ID 1674), Alonso, Ivan; Alpigiani, Cristiano; Altschul, Brett; Araujo, Henrique; Arduini, Gianluigi; Arlt, Jan; Badurina, Leonardo; Balaz, Antun; Bandarupally, Satvika; Barish, Barry C.; Barone, Michele; Barsanti, Michele; Bass, Steven; Bassi, Angelo; Battelier, Baptiste; Baynham, Charles F. A.; Beaufils, Quentin; Berge, Joel; Bernabeu, Jose; Bertoldi, Andrea; Bingham, Robert; Bize, Sebastien; Blas, Diego; Bongs, Kai; Bouyer, Philippe; Braitenberg, Carla; Brand, Christian; Braxmaier, Claus; Bresson, Alexandre; Buchmueller, Oliver; Budker, Dmitry; Bugalho, Luis; Burdin, Sergey; Cacciapuoti, Luigi; Callegari, Simone; Calmet, Xavier; Calonico, Davide; Canuel, Benjamin; Caramete, Laurentiu-Ioan; Carraz, Olivier; Cassettari, Donatella; Chakraborty, Pratik; Chattopadhyay, Swapan; Chauhan, Upasna; Chen, Xuzong; Chen, Yu-Ao; Chiofalo, Maria Luisa; Coleman, Jonathon; Corgier, Robin; Cotter, J. P.; Cruise, A. Michael; Cui, Yanou; Davies, Gavin; De Roeck, Albert; Demarteau, Marcel; Derevianko, Andrei; Di Clemente, Marco; Djordjevic, Goran S.; Donadi, Sandro; Dore, Olivier; Dornan, Peter; Doser, Michael; Drougakis, Giannis; Dunningham, Jacob; Easo, Sajan; Eby, Joshua; Elertas, Gedminas; Ellis, John; Evans, David; Examilioti, Pandora; Fadeev, Pavel; Fani, Mattia; Fassi, Farida; Fattori, Marco; Fedderke, Michael A.; Felea, Daniel; Feng, Chen-Hao; Ferreras, Jorge; Flack, Robert; Flambaum, Victor V.; Forsberg, Rene; Fromhold, Mark; Gaaloul, Naceur; Garraway, Barry M.; Georgousi, Maria; Geraci, Andrew; Gibble, Kurt; Gibson, Valerie; Gill, Patrick; Giudice, GianF; Goldwin, Jon; Gould, Oliver; Grachov, Oleg; Graham, Peter W.; Grasso, Dario; Griffin, PaulF; Guerlin, Christine; Gupta, Ratnesh K.; Haehnelt, Martin; Hawkins, Leonie; Hees, Aurelien; Henderson, Victoria A.; Herr, Waldemar; Herrmann, Sven; Hird, Thomas; Hobson, Richard; Hock, Vincent; Hogan, Jason M.; Holst, Bodil; Holynski, Michael; Israelsson, Ulf; Jeglic, Peter; Jetzer, Philippe; Juzeliunas, Gediminas; Kaltenbaek, Rainer; Kamenik, College of Sciences, and Department of Physics
- Abstract
We summarise the discussions at a virtual Community Workshop on Cold Atoms in Space concerning the status of cold atom technologies, the prospective scientific and societal opportunities offered by their deployment in space, and the developments needed before cold atoms could be operated in space. The cold atom technologies discussed include atomic clocks, quantum gravimeters and accelerometers, and atom interferometers. Prospective applications include metrology, geodesy and measurement of terrestrial mass change due to, e.g., climate change, and fundamental science experiments such as tests of the equivalence principle, searches for dark matter, measurements of gravitational waves and tests of quantum mechanics. We review the current status of cold atom technologies and outline the requirements for their space qualification, including the development paths and the corresponding technical milestones, and identifying possible pathfinder missions to pave the way for missions to exploit the full potential of cold atoms in space. Finally, we present a first draft of a possible road-map for achieving these goals, that we propose for discussion by the interested cold atom, Earth Observation, fundamental physics and other prospective scientific user communities, together with the European Space Agency (ESA) and national space and research funding agencies., We thank the CERN Quantum Technology Initiative for their support of the workshop that laid the basis for this paper.
- Published
- 2022
84. (In)direct detection of boosted dark matter
- Author
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Massachusetts Institute of Technology. Center for Theoretical Physics, Massachusetts Institute of Technology. Department of Physics, Agashe, Kaustubh, Cui, Yanou, Necib, Lina, Thaler, Jesse, Massachusetts Institute of Technology. Center for Theoretical Physics, Massachusetts Institute of Technology. Department of Physics, Agashe, Kaustubh, Cui, Yanou, Necib, Lina, and Thaler, Jesse
- Abstract
We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. These stable particles are typically a subdominant DM component, but because they are produced with a large Lorentz boost in this process, they can be detected in large volume terrestrial experiments via neutral-current-like interactions with electrons or nuclei. This novel DM signal thus combines the production mechanism associated with indirect detection experiments (i.e. galactic DM annihilation) with the detection mechanism associated with direct detection experiments (i.e. DM scattering off terrestrial targets). Such processes are generically present in multi-component DM scenarios or those with non-minimal DM stabilization symmetries. As a proof of concept, we present a model of two-component thermal relic DM, where the dominant heavy DM species has no tree-level interactions with the standard model and thus largely evades direct and indirect DM bounds. Instead, its thermal relic abundance is set by annihilation into a subdominant lighter DM species, and the latter can be detected in the boosted channel via the same annihilation process occurring today. Especially for dark sector masses in the 10 MeV-10 GeV range, the most promising signals are electron scattering events pointing toward the galactic center. These can be detected in experiments designed for neutrino physics or proton decay, in particular Super-K and its upgrade Hyper-K, as well as the PINGU/MICA extensions of IceCube. This boosted DM phenomenon highlights the distinctive signatures possible from non-minimal dark sectors. ©2014, U.S. Department of Energy (no. DE-FG02-05ER-41360), DOE Early Career research program (DE-FG02-11ER-41741)
- Published
- 2022
85. Warped dipole completed, with a tower of Higgs bosons
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Agashe, Kaustubh, Azatov, Aleksandr, Cui, Yanou, Randall, Lisa, and Son, Minho
- Published
- 2015
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86. Probing baryogenesis with displaced vertices at the LHC
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Cui, Yanou and Shuve, Brian
- Published
- 2015
- Full Text
- View/download PDF
87. The European Physical Journal C
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Abed Abud, Adam, Abi, Babak, Acciarri, Roberto, Acero, Mario, Adames, Marcio, Adamov, George, Adamowski, Mark, Adams, David, Adinolfi, Marco, Aduszkiewicz, Antoni, Aguilar, Jessica, Ahmad, Zubayer, Ahmed, Jhanzeb, Aimard, Benjamin, Ali-Mohammadzadeh, Behnam, Alion, Tyler, Allison, Kyle, Alonso Monsalve, Saul, AlRashed, Munera, Alt, Christoph, Alton, Andrew, Alvarez, Rodrigo, Amedo, Pablo, Anderson, John, Andreopoulos, Costas, Andreotti, Mirco, Andrews, Michael P., Andrianala, Fenompanirina, Andringa, Sofia, Anfimov, Nikolay, Ankowski, Artur, Antoniassi, Marcelo, Antonova, Maria, Antoshkin, Alexander, Antusch, Stefan, Aranda-Fernandez, Alfredo, Arellano, Luciano, Arnold, Lukas, Arroyave, Manuel, Asaadi, Jonathan, Asquith, Lily, Aurisano, Adam, Aushev, Vladimir, Autiero, Dario, Ayala Lara, Victor, Ayala-Torres, Marco Alberto, Azfar, Farrukh, Back, Ashley, Back, Henning, Back, John, Backhouse, Chris, Bagaturia, Iuri, Bagby, Linda, Balashov, Nikita, Balasubramanian, Supraja, Baldi, Pierre, Baller, Bruce, Bambah, Bindu, Barao, Fernando, Barenboim, Gabriela, Barham Alzas, Pablo, Barker, Gary J., Barkhouse, Wayne, Barnes, Christopher, Barr, Giles, Barranco Monarca, Juan, Barros, Adilson, Barros, Nuno, Barrow, Joshua, Basharina-Freshville, Anastasia, Bashyal, Amit, Basque, Vincent, Batchelor, Charlie, Batista das Chagas, Ewerton, Battat, J.B. R., Battisti, Federico, Bay, Fatih, Bazetto, Maria Cecilia, Bazo Alba, José Luis, Beacom, John, Bechetoille, Edouard, Behera, Biswaranjan, Beigbeder, Christophe, Bellantoni, Leo, Bellettini, Giorgio, Bellini, Vincenzo, Beltramello, Olga, Benekos, Nektarios, Benitez Montiel, Carlos, Bento Neves, Francisco, Berger, Joshua, Berkman, Sophie, Bernardini, Paolo, Berner, Roman, Bersani, Andrea, Bertolucci, Sergio, Betancourt, Minerba, Betancur Rodríguez, Amalia, Bevan, Adrian, Bezawada, Yashwanth, Bezerra, T.J. C., Bhardwaj, Akhil, Bhatnagar, Vipin, Bhattacharjee, Maharnab, Bhattarai, Devesh, Bhuller, Shyam, Bhuyan, Bipul, Biagi, Simone, Bian, Jianming, Biassoni, Matteo, Biery, Kurt, Bilki, Burak, Bishai, Mary, Bitadze, Alexander, Blake, Andrew, Blaszczyk, Flor de Maria, Blazey, Gerald C., Blucher, Edward, Boissevain, Jan, Bolognesi, Sara, Bolton, Timothy, Bomben, Luca, Bonesini, Maurizio, Bongrand, Mathieu, Bonilla-Diaz, Cesar, Bonini, Filiberto, Booth, Alexander, Boran, Fatma, Bordoni, Stefania, Borkum, Aran, Bostan, Nilay, Bour, Petr, Bourgeois, Christian, Boyden, Daniel, Bracinik, Juraj, Braga, Davide, Brailsford, Dominic, Branca, Antonio, Brandt, Andrew, Bremer, Johan, Breton, Dominique, Brew, Christopher, Brice, Stephen, Brizzolari, Claudia, Bromberg, Carl, Brooke, Jim, Bross, Alan, Brunetti, Giulia, Brunetti, Maria, Buchanan, Norman, Budd, Howard, Butorov, Ilia, Cagnoli, Irene, Cai, Tejin, Caiulo, Davide, Calabrese, Roberto, Calafiura, Paolo, Calcutt, Jacob, Calin, Marius, Calvez, Steven, Calvo, Enrique, Caminata, Alessio, Campanelli, Mario, Caratelli, David, Carber, Daniel, Carceller, J.C., Carceller, Juan Miguel, Carini, Gabriella, Carlus, Bruno, Carneiro, Mateus, Carniti, Paolo, Caro Terrazas, Ivan, Carranza, Hector, Carroll, Thomas, Castaño Forero, Javier, Castillo, Andrés, Castromonte, Cesar, Catano-Mur, Erika, Cattadori, Carla, Cavalier, Fabien, Cavallaro, Giuseppe, Cavanna, Flavio, Centro, Sandro, Cerati, Giuseppe, Cervelli, Alberto, Cervera Villanueva, Anselmo, Chalifour, Michel, Chappell, Andrew, Chardonnet, Etienne, Charitonidis, Nikolas, Chatterjee, Animesh, Chattopadhyay, Subhasish, Chavarry Neyra, Michael Steve, Chen, Hucheng, Chen, Mu-Chun, Chen, Yifan, Chen, Zheyang, Chen-Wishart, Zachary, Cheon, Yoolim, Cherdack, Daniel, Chi, Cheng-Yi, Childress, Sam, Chirco, Robert, Chiriacescu, Ana, Chisnall, Georgia, Cho, Kihyeon, Choate, Sarah, Chokheli, David, Chong, Pooi, Christensen, Anne, Christian, David, Christodoulou, Georgios, Chukanov, Artem, Chung, Moses, Church, Eric, Cicero, Valentina, Clarke, Peter, Cline, Gordon, Coan, Thomas, Cocco, Alfredo, Coelho, J.A. B., Colton, Nicole, Conley, Erin, Conley, Robert, Conrad, Janet M., Convery, Mark, Copello, Simone, Cova, Paolo, Cremaldi, Lucien, Cremonesi, Linda, Crespo-Anadón, José, Crisler, Michael, Cristaldo, Esteban, Crnkovic, Jason, Cross, Ryan, Cudd, Andrew, Cuesta, Clara, Cui, Yanou, Cussans, David, Dalager, Olivia, da Motta, Helio, da Silva Peres, Leonardo, David, Claire, David, Quentin, Davies, Gavin, Davini, Stefano, Dawson, Jaime, De, Kaushik, De, Shruti, Debbins, Paul, De Bonis, Isabelle, Decowski, M. Patrick, de Gouvea, Andre, de Holanda, Pedro, de Icaza Astiz, Iker, Deisting, Alexander, De Jong, Paul, Delbart, Alain, Delepine, David, Delgado, Maritza, Dell'Acqua, Andrea, Delmonte, Nicola, De Lurgio, Patrick, de Mello Neto, J.R. T., DeMuth, David, Dennis, Steve, Densham, Chris, Deptuch, Grzegorz, De Roeck, Albert, De Romeri, Valentina, de Souza, Greg, Devi, Ritu, Dharmapalan, Ranjan, Dias, Marco, Diaz, Felix, Diaz, Jorge S., Di Domizio, Sergio, Di Giulio, Letizia, Ding, Pengfei, Di Noto, Lea, Dirkx, Glenn, Distefano, Carla, Diurba, Richard, Diwan, Milind, Djurcic, Zelimir, Doering, Dionisio, Dolan, Stephen, Dolek, Furkan, Dolinski, Michelle J., Domine, Laura, Donon, Yann, Douglas, Daniel, Douillet, Denis, Dragone, Angelo, Drake, Gary, Drielsma, Francois, Duarte, Laura Cristina, Duchesneau, Dominique, Duffy, Kirsty, Dunne, Patrick, Dutta, Bhaskar, Duyang, Hongyue, Dvornikov, Olexiy, Dwyer, Daniel A., Dyshkant, Alexandre S., Eads, Michael, Earle, Antony, Edmunds, Daniel, Eisch, Jonathan, Emberger, Lorenz, Emery, Sandrine, Englezos, Panagiotis, Ereditato, Antonio, Erjavec, Tyler, Escobar, Carlos O., Eurin, Guillaume, Evans, Justin, Ewart, Erin, Ezeribe, Anthony, Fahey, Kevin, Falcone, Andrea, Fani', Mattia, Farnese, Christian, Farzan, Yasaman, Fedoseev, Dmitry, Felix, Julian, Feng, Yue, Fernandez-Martinez, Enrique, Fernandez Menendez, Pablo, Fernandez Morales, Miguel, Ferraro, Federico, Fields, Laura, Filip, Peter, Filthaut, Frank, Fiorini, Massimiliano, Fischer, Vincent, Fitzpatrick, Rory, Flanagan, Will, Fleming, Bonnie, Flight, Robert, Fogarty, Sam, Foreman, Will, Fowler, Jack, Fox, Walt, Franc, Jiri, Francis, Kurt, Franco, Domenico, Freeman, John, Freestone, Julian, Fried, Jack, Friedland, Alex, Fuentes Robayo, Freddy, Fuess, Stu, Furic, Ivan, Furman, Krzysztof, Furmanski, Andrew, Gabrielli, Alessandro, Gago, A.M., Gallagher, Hugh, Gallas, Alexandre, Gallego-Ros, Ana, Gallice, Niccolo, Galymov, Vyacheslav, Gamberini, Enrico, Gamble, Trevor, Ganacim, Francisco, Gandhi, Raj, Gandrajula, Reddy, Gao, Fan, Gao, Shanshan, Garcia-Gamez, Diego, García-Peris, Miguel, Gardiner, Steven, Gastler, Dan, Gauvreau, Jean-Luc, Ge, Guanqun, Geffroy, Nicolas, Gelli, Bruno, Gendotti, Adamo, Gent, Stephen, Ghorbani-Moghaddam, Zahra, Giammaria, Paola, Giammaria, Tommaso, Giangiacomi, Nico, Gibin, Daniele, Gil-Botella, Ines, Gilligan, Sean, Girerd, Claude, Giri, Anjan Kumar, Gnani, Dario, Gogota, Olga, Gold, Michael, Gollapinni, Sowjanya, Gollwitzer, Keith, Gomes, Ricardo, Gomez Bermeo, Laura Vanessa, Gomez Fajardo, L.S., Gonnella, Francesco, Gonzalez-Diaz, Diego, Gonzalez-Lopez, Manuel, Goodman, Maury, Goodwin, Owen, Goswami, Srubabati, Gotti, Claudio, Goudzovski, Evgueni, Grace, Carl, Gran, Rik, Granados, Everardo, Granger, Pierre, Grant, Alan, Grant, Christopher, Gratieri, Diego, Green, Patrick, Greenler, Leland, Greer, Joel, Grenard, Jean-Louis, Griffith, Clark, Groh, Micah, Grudzinski, James, Grzelak, Katarzyna, Gu, Wenqiang, Guardincerri, Elena, Guarino, Victor, Guarise, Marco, Guenette, Roxanne, Guerard, Eric, Guerzoni, Marco, Guffanti, Daniele, Guglielmi, Alberto, Guo, Bing, Gupta, Aseem, Gupta, Vikas, Guthikonda, K.K., Gutierrez, Rafael, Guzowski, Pawel, Guzzo, Marcelo, Gwon, Sunwoo, Ha, Chang Hyon, Haaf, Kevin, Habig, Alec, Hadavand, Haleh, Haenni, Roger, Hahn, Alan, Haiston, James, Hamacher-Baumann, Philip, Hamernik, Thomas, Hamilton, Philip, Han, Jiyeon, Harris, Deborah, Hartnell, Jeffrey, Hartnett, Trevor, Harton, John, Hasegawa, Takyua, Hasnip, Ciaran, Hatcher, Robert, Hatfield, Kaleb, Hatzikoutelis, Athanasios, Hayes, Christopher, Hayrapetyan, Karen, Hays, Jonathan, Hazen, Eric, He, Muyuan, Heavey, Anne, Heeger, Karsten, Heise, Jaret, Henry, Sarah, Hernandez Morquecho, Miguel Angel, Herner, Kenneth, Hewes, V., Hewes, Jeremy, Hilgenberg, Christopher, Hill, Tony, Hillier, Stephen, Himmel, Alexander, Hinkle, Elise, Hirsch, Luciana, Ho, Johnny, Hoff, James, Holin, Anna, Hoppe, Eric, Horton-Smith, Glenn, Hostert, Matheus, Hourlier, Adrien, Howard, Bruce, Howell, Ryan, Hoyos, Jaime, Hristova, Ivana, Hronek, Maxine, Huang, Junying, Hulcher, Zachary, Iles, Gregory, Ilic, Nikolina, Iliescu, Antoniu, Illingworth, Robert, Ingratta, Gianfranco, Ioannisian, Ara, Irwin, Burke, Isenhower, Larry, Itay, Ran, Jackson, Christopher, Jain, Vivek, James, Eric, Jang, Wooyoung, Jargowsky, Benjamin, Jediny, Filip, Jena, Deepika, Jeong, Yu Seon, Jesús-Valls, César, Ji, Xiangpan, Jiang, Libo, Jiménez, Sergio, Jipa, Alexandru, Johnson, Randy, Johnson, Walker, Johnston, Nicholas, Jones, Benjamin, Jones, Sebastian, Judah, Matthew, Jung, Chang Kee, Junk, Thomas, Jwa, Yeon-jae, Kabirnezhad, Monireh, Kaboth, Asher, Kadenko, I., Kakorin, Igor, Kalitkina, Anastasia, Kalra, Daisy, Kamiya, Felipe, Kaneshige, Nathaniel, Kaplan, Daniel, Karagiorgi, Georgia, Karaman, Gurkan, Karcher, Armin, Karolak, Mark, Karyotakis, Yannis, Kasai, Seiji, Kasetti, Siva, Kashur, Lane, Kazaryan, Narine, Kearns, Edward, Keener, Paul, Kelly, Kevin, Kemp, Ernesto, Kemularia, Otari, Ketchum, Wes, Kettell, Steve, Khabibullin, Marat, Khotjantsev, Alexei, Khvedelidze, Arsen, Kim, Doojin, King, Bonnie, Kirby, Brian, Kirby, Mike, Klein, Joshua, Klustova, Anezka, Kobilarcik, Thomas, Koehler, Kevin, Koerner, Lisa, Koh, D.H., Kohn, Sam, Koller, Patrick, Kolupaeva, Liudmila, Korablev, Denis, Kordosky, Mike, Kosc, Thomas, Kose, Umut, Kostelecky, V. Alan, Kothekar, Kunal, Kralik, Robert, Kreczko, Luke, Krennrich, Frank, Kreslo, Igor, Kropp, William, Kroupova, Tereza, Kubota, Shion, Kudenko, Yury, Kudryavtsev, Vitaly A., Kulagin, Sergey, Kumar, Jason, Kumar, Praveen, Kunze, Pablo, Kurita, Nadine, Kuruppu, Chatura, Kus, Vaclav, Kutter, Thomas, Kvasnicka, Jiri, Kwak, Donghyun, Lambert, Andrew, Land, Benjamin, Lane, Charles, Lang, Karol, Langford, Thomas, Langstaff, Mark, Larkin, Jacob, Lasorak, Pierre, Last, David, Laundrie, Andy, Laurenti, Giuliano, Lawrence, Andrew, Lazanu, Ionel, LaZur, Ryan, Lazzaroni, Massimo, Le, Trung, Leardini, Sara, Learned, John, LeBrun, Patrice, LeCompte, Thomas, Lee, Claire, Lee, Soo Yeon, Lehmann Miotto, Giovanna, Lehnert, Ralf, de Oliveira, M.A. Leigui, Leitner, Matthaeus, Lepin, Luis, Li, Shirley W., Li, Yichen, Liao, Heng-Ye, Lin, Cheng-Ju Stephen, Lin, Qing, Lin, Shih-Kai, Lineros, Roberto, Ling, Jiajie, Lister, Adam, Littlejohn, Bryce, Liu, Junze, Liu, Yinrui, Lockwitz, Sarah, Loew, Timothy, Lokajicek, Milos, Lomidze, Irakli, Long, Ken, Lord, Tom, LoSecco, John M., Louis, William, Lu, Xianguo, Luk, Kam-Biu, Lunday, Benjamin, Luo, Xiao, Luppi, Eleonora, Lux, Thorsten, Luzio, Vitor, Maalmi, Jihane, MacFarlane, David, Machado, Ana Amelia, Machado, Pedro, Macias, Christopher Thomas, Macier, Jolie R., Maddalena, Antonello, Madera, Alfonso, Madigan, Peter, Magill, Steve, Mahn, Kendall, Maio, Amélia, Major, Adryanna, Maloney, James, Mandrioli, Gianni, Mandujano, Roberto, Maneira, José, Manenti, Laura, Manly, Steve, Mann, Anthony, Manolopoulos, Konstantinos, Manrique Plata, Maria, Manyam, Venkata, Manzanillas, Luis, Marchan, Miquel, Marchionni, Alberto, Marciano, William, Marfatia, Danny, Mariani, Camillo, Maricic, Jelena, Marie, Rodolphe, Marinho, Franciole, Marino, Alysia, Marsden, David, Marshak, Marvin, Marshall, Chris, Marshall, John, Marteau, Jacques, Martin-Albo, Justo, Martinez, Norman, Martinez Caicedo, David, Martínez Miravé, Pablo, Martynenko, Sergey, Mascagna, Valerio, Mason, Katie, Mastbaum, Andrew, Matichard, Fabrice, Matsuno, Shigenobu, Matthews, James, Mauger, Christopher, Mauri, Nicoletta, Mavrokoridis, Konstantinos, Mawby, Isobel, Mazza, Roberto, Mazzacane, Anna, Mazzucato, Edoardo, McAskill, Tracy, McCluskey, Elaine, McConkey, Nicola, McFarland, Kevin, McGrew, Clark, McNab, Andrew, Mefodiev, Alexander, Mehta, Poonam, Melas, Pantelis, Mena, Olga, Mendez, Hector, Mendez, Patricia, Méndez, Diana, Menegolli, A., Meng, Guang, Messier, Mark, Metcalf, William, Mettler, Thomas, Mewes, Matthew, Meyer, Holger, Miao, Ting, Michna, Gregory, Miedema, Thijs, Mikola, Veera, Milincic, Radovan, Miller, Graham, Miller, William, Mills, Joshua, Mineev, Oleg, Minotti, Alessandro, Miranda, Omar, Miryala, Sandeep, Mishra, C. Shekhar, Mishra, Sanjib R., Mislivec, Aaron, Mitchell, Mote, Mladenov, Dimitar, Mocioiu, Irina, Moffat, Kristian, Moggi, Niccolo, Mohanta, Rukmani, Mohayai, Tanaz, Mokhov, Nikolai, Molina, Jorge, Molina Bueno, Laura, Montagna, Elisabetta, Montanari, Alessandro, Montanari, Claudio, Montanari, David, Zetina, L.M. Montañno, Moon, Seok Ho, Mooney, Michael, Moor, Alexandra, Moreno, Deywis, Moretti, Davide, Morris, Casandra, Mossey, Chris, Mitchell Mote, Motuk, Erdem, Moura, Célio, Mousseau, Joel, Mouster, Gwenn, Mu, Wei, Mualem, Leon, Mueller, Justin, Muether, Mathew, Mufson, Stuart, Muheim, Franz, Muir, Alan, Mulhearn, Mike, Munford, Donnie, Muramatsu, Hajime, Murphy, Sebastien, Musser, Jim, Nachtman, Jane, Nagu, Srishti, Nalbandyan, Mikayel, Nandakumar, Raja, Naples, Donna, Narita, Shinya, Nath, Atanu, Navrer-Agasson, Anyssa, Nayak, Nitish, Nebot-Guinot, Miquel, Negishi, Kentaro, Nelson, Jeff, Nesbit, Jake, Nessi, Marzio, Newbold, David, Newcomer, Mitch, Newton, Hannah, Nichol, Ryan, Nicolas-Arnaldos, Francisco, Nikolica, Adrian, Niner, Evan, Nishimura, Kurtis, Norman, Andrew, Norrick, Anne, Northrop, Rich, Novella, Pau, Nowak, Jaroslaw, Oberling, Michael, Ochoa-Ricoux, Juan Pedro, Olivier, Andrew, Olshevskiy, Alexander, Onel, Yasar, Onishchuk, Yuriy, Ott, Jordan, Pagani, Luca, Palacio, Guillermo, Palamara, Ornella, Palestini, Sandro, Paley, Jonathan, Pallavicini, Marco, Palomares, Carmen, Panduro Vazquez, William, Pantic, Emilija, Paolone, Vittorio, Papadimitriou, Vaia, Papaleo, Riccardo, Papanestis, Antonis, Paramesvaran, Sudarshan, Parke, Stephen, Parozzi, Elisabetta, Parsa, Zohreh, Parvu, Mihaela, Pascoli, Silvia, Pasqualini, Laura, Pasternak, Jaroslaw, Pater, Joleen, Patrick, Cheryl, Patrizii, Laura, Patterson, Ryan, Patton, Simon John, Patzak, Thomas, Paudel, Ajib, Paulos, Bob, Paulucci, Laura, Pavlovic, Zarko, Pawloski, Greg, Payne, David, Pec, Viktor, Peeters, S.J. M., Pena Perez, Aldo, Pennacchio, Elisabetta, Penzo, Aldo, Peres, Orlando, Perry, James, Pershey, Daniel, Pessina, Gianluigi, Petrillo, Gianluca, Petta, Catia, Petti, Roberto, Valerio Pia, Piastra, Francesco, Pickering, Luke, Pietropaolo, Francesco, Pimentel, Vinicius, Pinaroli, Giovanni, Plows, Komninos-John, Plunkett, Robert, Poling, Ronald, Pompa, Federica, Pons, Xavier, Poonthottathil, Navaneeth, Poppi, Francesco, Pordes, Stephen, Porter, Joshua, Potekhin, Maxim, Potenza, Renato, Potukuchi, B.V. K.S., Pozimski, Juergen, Pozzato, Michele, Prakash, Suprabh, Prakash, Tarun, Prest, Michela, Prince, Sebastien, Psihas, Fernanda, Pugnere, Denis, Qian, Xin, Raaf, Jennifer L., Radeka, Veljko, Rademacker, Jonas, Radics, Balint, Rafique, Aleena, Raguzin, Eric, Rai, Mousam, Rajaoalisoa, Miriama, Rakhno, Igor, Rakotonandrasana, Andrianjafy Michaël, Rakotondravohitra, Laza, Rameika, Regina, Ramirez Delgado, Manuel Alejandro, Ramson, Bryan, Rappoldi, A., Raselli, G.L., Ratoff, Peter, Raut, Sanil, Razakamiandra, Rado Fanantenana, Rea, Eran, Real, Jean-Sebastien, Rebel, Brian, Rechenmacher, Ronald, Reggiani-Guzzo, Marina, Reichenbacher, Juergen, Reitzner, S.D., Rejeb Sfar, Haifa, Renshaw, Andrew, Rescia, Sergio, Resnati, Filippo, Ribas, Marlos, Riboldi, Stefano, Riccio, Ciro, Riccobene, Giorgio, Rice, L.C. J., Ricol, Jean-Stephane, Rigamonti, Alberto, Rigaut, Yann-Axel, Rincón, Edgar, Ritchie-Yates, Harrison, Rivera, David, Robert, Arnaud, Rochester, Leon, Roda, Marco, Rodrigues, Philip, Rodriguez Alonso, Manuel, Rodriguez Bonilla, Engelver, Rodriguez Rondon, Jairo, Rosauro-Alcaraz, Salvador, Rosenberg, Matt, Rosier, Philippe, Roskovec, Bedrich, Rossella, Massimo, Rossi, Marco, Rout, Jogesh, Roy, Palash, Rubbia, Andre, Rubbia, Carlo, Russell, Brooke, Ruterbories, Daniel, Rybnikov, Arseniy, Saa-Hernandez, Angela, Saakyan, Ruben, Sacerdoti, Sabrina, Safford, Twymun, Sahu, Narendra, Sakashita, Ken, Sala, Paola, Samios, Nicholas, Samoylov, Oleg, Sanchez, Mayly, Sandberg, Vern, Sanders, David, Sankey, David, Santana, Samuel, Santos-Maldonado, Marvin, Saoulidou, Niki, Sapienza, Piera, Sarasty, Carlos, Sarcevic, Ina, Savage, Geoffrey, Savinov, Vladimir, Scaramelli, Alberto, Scarff, Andrew, Scarpelli, Andrea, Schefke, Tristan, Schellman, Heidi, Schifano, Sebastiano, Schlabach, Philip, Schmitz, David, Schneider, Austin, Scholberg, Kate, Schukraft, Anne, Segreto, Ettore, Selyunin, Alexander, Senise, C.R., Senise Jr, Carlos, Sensenig, Jon, Sergi, Antonino, Sgalaberna, Davide, Shaevitz, Michael H., Shafaq, Sheeba, Shaker, Fady, Shamma, Michael, Sharankova, Ralitsa, Sharma, Hans, Sharma, Rahul, Sharma, Rajeev, Shaw, Terri, Shchablo, Konstantin, Shepherd-Themistocleous, Claire, Sheshukov, Andrey, Shin, Seodong, Shoemaker, Ian, Shooltz, Dean, Shrock, Robert, Siegel, Harrison, Simard, Laurent, Sinclair, James, Sinev, Gleb, Singh, Jaydip, Singh, Jyotsna, Singh, Lakwinder, Singh, Prabhjot, Singh, Venktesh, Sipos, Roland, Sippach, F.W., Sirri, Gabriele, Sitraka, Andriaseta, Siyeon, Kim, Skarpaas, Knut, Smith, Andrew, Smith, Erica, Smith, Paul, Smolik, Jan, Smy, Michael, Snider, E.L., Snopok, Pavel, Snowden-Ifft, Daniel, Soares Nunes, Mônica, Sobel, Henry, Soderberg, Mitch, Sokolov, Sergei, Solano Salinas, Carlos, Söldner-Rembold, Stefan, Soleti, Stefano Roberto, Solomey, Nicholas, Solovov, Vladimir, Sondheim, Walter, Sorel, Michel, Sotnikov, Albert, Soto-Oton, Jose, Soto Ugaldi, Fidel Antonio, Sousa, Alexandre, Soustruznik, Karel, Spagliardi, Fabio, Spanu, Maura, Spitz, Joshua, Spooner, N.J. C., Spurgeon, Kyle, Stancari, Michelle, Stanco, Luca, Stanford, Chris, Stein, Raul, Steiner, Herbert M., Steklain Lisbôa, André, Stewart, James, Stillwell, Ben, Stock, Jason, Stocker, Francesca, Stokes, Tyler, Strait, Matthew, Strauss, Thomas, Strigari, Louis, Stuart, Alexander, Suarez, Juan, Suárez Sunción, Juan Martín, Sullivan, Hunter, Summers, Don, Surdo, Antonio, Susic, Vasja, Suter, Louise, Sutera, Concetta Maria, Svoboda, Robert, Szczerbinska, Barbara, Szelc, Andrzej, Tanaka, Hirohisa, Tang, Shaochun, Tapia, Alex, Tapia Oregui, Beatriz, Tapper, Alexander, Tariq, Salman, Tarpara, Eaglekumar, Tata, Neeraj, Tatar, Tayloe, Rex, Teklu, Abraham Meles, Tennessen, Peter, Tenti, Matteo, Terao, Kazuhiro, Ternes, Christoph, Terranova, Francesco, Testera, Gemma, Thakore, Tarak, Thea, Alessandro, Thompson, Joshua, Thorn, Craig, Timm, Steven C., Tishchenko, Vladimir, Tomassetti, Luca, Tonazzo, Alessandra, Torbunov, Dmitri, Torti, Marta, Tortola, Mariam, Tortorici, Francesco, Tosi, Nicolo, Totani, Dante, Toups, Matthew, Touramanis, Christos, Travaglini, Riccardo, Trevor, Jason, Trilov, Stoyan, Trzaska, Wladyslaw, Tsai, Yu-Dai, Tsai, Yun-Tse, Tsamalaidze, Zviadi, Tsang, Ka Vang, Tsverava, Nikolozi, Tufanli, Serhan, Tull, Craig, Tyley, E., Tzanov, Martin, Uboldi, Lorenzo, Uchida, Melissa, Urheim, Jon, Usher, Tracy, Uzunyan, Sergey, Vagins, Mark, Vahle, Patricia, Valder, Sammy, Valdiviesso, Gustavo, Valencia, Edgar, Valentim, Rodolfo, Vallari, Zoya, Vallazza, Erik, Valle, J.W. F., Vallecorsa, Sofia, Van Berg, Rick, Van de Water, Richard, Vanegas Forero, David, Vannerom, David, Varanini, Filippo, Vargas, Danaisis, Varner, Gary, Vasel, Justin, Vasina, Svetlana, Vasseur, Georges, Vaughan, Noah, Vaziri, Kamran, Ventura, Sandro, Verdugo, Antonio, Vergani, Stefano, Vermeulen, Milo, Verzocchi, Marco, Vicenzi, Matteo, Vieira de Souza, Henrique, Vignoli, Chiara, Vilela, Cristovao, Viren, Brett, Vrba, Tomas, Wachala, Tomasz, Waldron, Abigail, Wallbank, Michael, Wallis, Connor, Wang, Hanguo, Wang, Jingbo, Wang, Li, Wang, M.H. L.S., Wang, Xiaoran, Wang, Yi, Wang, Yue, Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Wawrowska, Klaudia, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Alexander, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wisniewski, William, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Anthony, Wood, Kevin, Worcester, Elizabeth, Worcester, Matthew, Wresilo, Karolina, Wret, Clarence, Wu, Wanwei, Wu, Wenjie, Xiao, Yiwen, Xie, Fang, Yaeggy, Barbara, Yandel, Erin, Yang, Guang, Yang, Kang, Yang, Tingjun, Yankelevich, Alejandro, Yershov, Nikolai, Yonehara, Katsuya, Yoon, Young Soo, Young, Tim, Yu, Bo, Yu, Haiwang, Yu, Hongzhao, Yu, Jae, Yu, Yiding, Yuan, Wenlong, Zaki, Rowan, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeller, Geralyn, Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhang, Shuaixiang, Zhang, Yuze, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zimmerman, Eric, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, UK Research and Innovation, XENON (IHEF, IoP, FNWI), Other Research IHEF (IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IoP (FNWI), DUNE Collaboration, Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, Apollo - University of Cambridge Repository, Abud, A Abed, Abi, B, Acciarri, R, Acero, M A, Adames, M R, Adamov, G, Adamowski, M, Adams, D, Adinolfi, M, Aduszkiewicz, A, Aguilar, J, Ahmad, Z, Ahmed, J, Aimard, B, Ali-Mohammadzadeh, B, Alion, T, Allison, K, Monsalve, S Alonso, AlRashed, M, Alt, C, Alton, A, Alvarez, R, Amedo, P, Anderson, J, Andreopoulos, C, Andreotti, M, Andrews, M, Andrianala, F, Andringa, S, Anfimov, N, Ankowski, A, Antoniassi, M, Antonova, M, Antoshkin, A, Antusch, S, Aranda-Fernandez, A, Arellano, L, Arnold, L O, Arroyave, M A, Asaadi, J, Asquith, L, Aurisano, A, Aushev, V, Autiero, D, Lara, V Ayala, Ayala-Torres, M, Azfar, F, Back, A, Back, H, Back, J J, Backhouse, C, Bagaturia, I, Bagby, L, Balashov, N, Balasubramanian, S, Baldi, P, Baller, B, Bambah, B, Barao, F, Barenboim, G, Alzas, P Barham, Barker, G, Barkhouse, W, Barnes, C, Barr, G, Monarca, J Barranco, Barros, A, Barros, N, Barrow, J L, Basharina-Freshville, A, Bashyal, A, Basque, V, Batchelor, C, Chagas, E Batista da, Battat, J B R, Battisti, F, Bay, F, Bazetto, M C Q, Alba, J L L Bazo, Beacom, J F, Bechetoille, E, Behera, B, Beigbeder, C, 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Physics - Instrumentation and Detectors ,Science & Technology ,Physics and Astronomy (miscellaneous) ,Regular Article - Experimental Physics ,Physics::Instrumentation and Detectors ,530 Physics ,Physics ,Settore FIS/01 - Fisica Sperimentale ,FOS: Physical sciences ,neutrino detector, dual phase liquid argon TPC, scintillation light ,Instrumentation and Detectors (physics.ins-det) ,Nuclear & Particles Physics ,Settore FIS/04 - Fisica Nucleare e Subnucleare ,Physics, Particles & Fields ,neutrino ,DUNE Collaboration ,Physical Sciences ,SIMULATION ,0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,High Energy Physics ,Detectors and Experimental Techniques ,Engineering (miscellaneous) ,physics.ins-det ,0206 Quantum Physics - Abstract
Funder: Ministerio de Ciencia e Innovación; doi: http://dx.doi.org/10.13039/501100004837, Funder: Xunta de Galicia; doi: http://dx.doi.org/10.13039/501100010801, Funder: Conselho Nacional de Desenvolvimento Científico e Tecnológico; doi: http://dx.doi.org/10.13039/501100003593, Funder: Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; doi: http://dx.doi.org/10.13039/501100004586, Funder: Instituto Nazionale di Fisica Nucleare; doi: http://dx.doi.org/10.13039/501100004007, Funder: Fundação Amazônia Paraense de Amparo à Pesquisa; doi: http://dx.doi.org/10.13039/501100005288, Funder: Junta de Andalucia-FEDER, Funder: Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada; doi: http://dx.doi.org/10.13039/501100002790, Funder: “la Caixa” Foundation; doi: http://dx.doi.org/10.13039/100010434, Funder: Canada Foundation for Innovation; doi: http://dx.doi.org/10.13039/501100000196, Funder: UK Research and Innovation; doi: http://dx.doi.org/10.13039/100014013, Funder: Royal Society; doi: http://dx.doi.org/10.13039/501100000288, Funder: IPP, Funder: Centre National de la Recherche Scientifique; doi: http://dx.doi.org/10.13039/501100004794, Funder: CEA, Funder: National Science Foundation; doi: http://dx.doi.org/10.13039/100000001, Funder: Türkiye Bilimsel ve Teknolojik Arastirma Kurumu; doi: http://dx.doi.org/10.13039/501100004410, Funder: MSMT, Funder: CERN; doi: http://dx.doi.org/10.13039/100012470, Funder: Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; doi: http://dx.doi.org/10.13039/501100001711, Funder: Comunidad de Madrid; doi: http://dx.doi.org/10.13039/100012818, Funder: Fundação de Amparo à Pesquisa do Estado de Goiá s; doi: http://dx.doi.org/10.13039/501100005285, Funder: FCT, Funder: National Research Foundation; doi: http://dx.doi.org/10.13039/501100001321, Funder: U.S. Department of Energy; doi: http://dx.doi.org/10.13039/100000015, Funder: Marie Sklodowska-Curie Actions; doi: http://dx.doi.org/10.13039/100018694, Funder: Science and Technology Facilities Council; doi: http://dx.doi.org/10.13039/501100000271, Funder: European Regional Development Fund; doi: http://dx.doi.org/10.13039/501100008530, DUNE is a dual-site experiment for long-baseline neutrino oscillation studies, neutrino astrophysics and nucleon decay searches. ProtoDUNE Dual Phase (DP) is a 6 × 6 × 6 m 3 liquid argon time-projection-chamber (LArTPC) that recorded cosmic-muon data at the CERN Neutrino Platform in 2019-2020 as a prototype of the DUNE Far Detector. Charged particles propagating through the LArTPC produce ionization and scintillation light. The scintillation light signal in these detectors can provide the trigger for non-beam events. In addition, it adds precise timing capabilities and improves the calorimetry measurements. In ProtoDUNE-DP, scintillation and electroluminescence light produced by cosmic muons in the LArTPC is collected by photomultiplier tubes placed up to 7 m away from the ionizing track. In this paper, the ProtoDUNE-DP photon detection system performance is evaluated with a particular focus on the different wavelength shifters, such as PEN and TPB, and the use of Xe-doped LAr, considering its future use in giant LArTPCs. The scintillation light production and propagation processes are analyzed and a comparison of simulation to data is performed, improving understanding of the liquid argon properties.
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- 2022
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88. Unraveling the Dirac neutrino with cosmological and terrestrial detectors
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Adshead, Peter, Cui, Yanou, Long, Andrew J., and Shamma, Michael
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- 2021
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89. Impact of a midband gravitational wave experiment on detectability of cosmological stochastic gravitational wave backgrounds
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Barish, Barry C., primary, Bird, Simeon, additional, and Cui, Yanou, additional
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- 2021
- Full Text
- View/download PDF
90. Deep Underground Neutrino Experiment (DUNE) Near Detector Conceptual Design Report
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Mislivec, Aaron, Mladenov, Dimitar, Mocioiu, Irina, Moffat, Kristian, Moggi, Niccolo, Mohanta, Rukmani, Mohayai, Tanaz, Mokhov, Nikolai, Molina, Jorge, Molina Bueno, Laura, Montanari, Alessandro, Montanari, Claudio, Montanari, David, Montagna, E., Montano Zetina, Luis, Moon, Jarrett, Mooney, Michael, Moor, Alexandra, Moreno, Deywis, Morris, Casandra, Mossey, Chris, Motuk, Erdem, Moura, Célio, Mousseau, Joel, Mu, Wei, Mualem, Leon, Mueller, Justin, Muether, Mathew, Mufson, Stuart, Muheim, Franz, Muir, Alan, Mulhearn, Mike, Munford, Donnie, Muramatsu, Hajime, Murphy, Sebastien, Musser, Jim, Nachtman, Jane, Nagu, Srishti, Nalbandyan, Mikayel, Nandakumar, Raja, Naples, Donna, Narita, Shinya, Navas-Nicolás, Diana, Navrer-Agasson, Anyssa, Nayak, Nitish, Nebot-Guinot, Miquel, Negishi, Kentaro, Nelson, Jeff, Nesbit, Jake, Nessi, Marzio, Newbold, David, Newcomer, Mitch, Newhart, Duane, Newton, Hannah, Niccolo, M., Nichol, Ryan, Nicolas-Arnaldos, Francisco, Nicoletta, M., Niner, Evan, Nishimura, 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C., Groh, M., Grudzinski, J., Grzelak, K., Gu, W., Guarino, V., Guenette, R., Guerard, E., Guerzoni, M., Guglielmi, A., Guo, B., Guthikonda, K. K., Gutierrez, R., Guzowski, P., Guzzo, M. M., Gwon, S., Habig, A., Hadavand, H., Haenni, R., Hahn, A., Haiston, J., Hamacher-Baumann, P., Hamernik, T., Hamilton, P., Han, J., Harris, D. A., Hartnell, J., Harton, J., Hasegawa, T., Hasnip, C., Hatcher, R., Hatfield, K. W., Hatzikoutelis, A., Hayes, C., Hazen, E., Heavey, A., Heeger, K. M., Heise, J., Hennessy, K., Henry, S., Hernandez Morquecho, M. A., Herner, K., Hertel, L., Hewes, J., Higuera, A., Hill, T., Hillier, S. J., Himmel, A., Hoff, J., Hohl, C., Holin, A., Hoppe, E., Horton-Smith, G. A., Hostert, M., Hourlier, A., Howard, B., Howell, R., Huang, J., Hugon, J., Iles, G., Ilic, N., Iliescu, A. M., Illingworth, R., Ingratta, G., Ioannisian, A., Isenhower, L., Itay, R., Izmaylov, A., Jackson, S., Jain, V., James, E., Jargowsky, B., Jediny, F., Jena, D., Jeong, Y. S., Jesus-Valls, C., Ji, X., Jiang, L., Jimenez, S., Jipa, A., Johnson, R., Johnston, N., Jones, B., Jones, S. B., Judah, M., Jung, C. K., Junk, T., Jwa, Y., Kabirnezhad, M., Kaboth, A., Kadenko, I., Kakorin, I., Kamiya, F., Kaneshige, N., Karagiorgi, G., Karaman, G., Karcher, A., Karolak, M., Karyotakis, Y., Kasai, S., Kasetti, S. P., Kashur, L., Kazaryan, N., Kearns, E., Keener, P., Kelly, K. J., Kemp, E., Kemularia, O., Ketchum, W., Kettell, S. H., Khabibullin, M., Khotjantsev, A., Khvedelidze, A., Kim, D., King, B., Kirby, B., Kirby, M., Klein, J., Koehler, K., Koerner, L. W., Kohn, S., Koller, P. P., Kolupaeva, L., Kordosky, M., Kosc, T., Kose, U., Kostelecky, V. A., Kothekar, K., Krennrich, F., Kreslo, I., Kudenko, Y., Kudryavtsev, V. A., Kulagin, S., Kumar, J., Kumar, P., Kumar, R., Kunze, P., Kurita, N., Kuruppu, C., Kus, V., Kutter, T., Lambert, A., Land, B., Lande, K., Lane, C. 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A., Mokhov, N., Molina, J., Molina Bueno, L., Montanari, A., Montanari, C., Montanari, D., Montagna, E., Montano Zetina, L. M., Moon, J., Mooney, M., Moor, A. F., Moreno, D., Morris, C., Mossey, C., Motuk, E., Moura, C. A., Mousseau, J., Mu, W., Mualem, L., Mueller, J., Muether, M., Mufson, S., Muheim, F., Muir, A., Mulhearn, M., Munford, D., Muramatsu, H., Murphy, S., Musser, J., Nachtman, J., Nagu, S., Nalbandyan, M., Nandakumar, R., Naples, D., Narita, S., Navas-Nicolas, D., Navrer-Agasson, A., Nayak, N., Nebot-Guinot, M., Negishi, K., Nelson, J. K., Nesbit, J., Nessi, M., Newbold, D., Newcomer, M., Newhart, D., Newton, H., Niccolo, M., Nichol, R., Nicolas-Arnaldos, F., Nicoletta, M., Niner, E., Nishimura, K., Norman, A., Norrick, A., Northrop, R., Novella, P., Nowak, J. A., Oberling, M., Ochoa-Ricoux, J. P., Olivares Del Campo, A., Olivier, A., Olshevskiy, A., Onel, Y., Onishchuk, Y., Ott, J., Pagani, L., Pakvasa, S., Palacio, G., Palamara, O., Palestini, S., Paley, J. M., Pallavicini, M., Palomares, C., Palomino-Gallo, J. L., Pantic, E., Paolone, V., Papadimitriou, V., Papaleo, R., Papanestis, A., Paramesvaran, S., Parke, S., Parsa, Z., Parvu, M., Pascoli, S., Pasqualini, L., Pasternak, J., Pater, J., Patrick, C., Patrizii, L., Patterson, R. B., Patton, S. J., Patzak, T., Paudel, A., Paulos, B., Paulucci, L., Pavlovic, Z., Pawloski, G., Payne, D., Pec, V., Peeters, S. J. M., Pennacchio, E., Penzo, A., Peres, O. L. G., Perry, J., Pershey, D., Pessina, G., Petrillo, G., Petta, C., Petti, R., Piastra, F., Pickering, L., Pietropaolo, F., Plunkett, R., Poling, R., Pons, X., Poonthottathil, N., Poppi, F., Pordes, S., Porter, J., Potekhin, M., Potenza, R., Potukuchi, B. V. K. S., Pozimski, J., Pozzato, M., Prakash, S., Prakash, T., Prince, S., Pugnere, D., Qian, X., Queiroga Bazetto, M. C., Raaf, J. L., Radeka, V., Rademacker, J., Radics, B., Rafique, A., Raguzin, E., Rai, M., Rajaoalisoa, M., Rakhno, I., Rakotonandrasana, A., Rakotondravohitra, L., Ramachers, Y. A., Rameika, R., Ramirez Delgado, M. A., Ramson, B., Rappoldi, A., Raselli, G., Ratoff, P., Raut, S., Razakamiandra, R. F., Real, J. S., Rebel, B., Reggiani-Guzzo, M., Rehak, T., Reichenbacher, J., Reitzner, S. D., Rejeb Sfar, H., Renshaw, A., Rescia, S., Resnati, F., Reynolds, A., Riccio, C., Riccobene, G., Rice, L. C. J., Ricol, J., Rigamonti, A., Rigaut, Y., Rivera, D., Rochester, L., Roda, M., Rodrigues, P., Rodriguez Alonso, M. J., Rodriguez Bonilla, E., Rodriguez Rondon, J., Rosauro-Alcaraz, S., Rosenberg, M., Rosier, P., Roskovec, B., Rossella, M., Rout, J., Roy, P., Roy, S., Rubbia, A., Rubbia, C., Rubio, F. C., Russell, B., Ruterbories, D., Saakyan, R., Sacerdoti, S., Safford, T., Sahay, R., Sahu, N., Sala, P., Samios, N., Samoylov, O., Sanchez, M. C., Sanders, D. A., Sankey, D., Santana, S., Santos-Maldonado, M., Saoulidou, N., Sapienza, P., Sarasty, C., Sarcevic, I., Savage, G., Savinov, V., Scaramelli, A., Scarff, A., Scarpelli, A., Schaffer, T., Schellman, H., Schlabach, P., Schmitz, D., Scholberg, K., Schukraft, A., Segreto, E., Sensenig, J., Seong, I., Sergi, A., Sgalaberna, D., Shaevitz, M. H., Shafaq, S., Shamma, M., Sharankova, R., Sharma, H. R., Sharma, R., Shaw, T., Shepherd-Themistocleous, C., Shin, S., Shooltz, D., Shrock, R., Simard, L., Simon, F., Simos, N., Sinclair, J., Sinev, G., Singh, J., Singh, V., Sipos, R., Sippach, F. W., Sirri, G., Sitraka, A., Siyeon, K., Skarpaas, K., Smith, A., Smith, E., Smith, P., Smolik, J., Smy, M., Snider, E. L., Snopok, P., Soares Nunes, M., Sobel, H., Soderberg, M., Solano Salinas, C. J., Soldner-Rembold, S., Soleti, S., Solomey, N., Solovov, V., Sondheim, W. E., Sorel, M., Soto-Oton, J., Sousa, A., Soustruznik, K., Spagliardi, F., Spanu, M., Spitz, J., Spooner, N. J. C., Spurgeon, K., Staley, R., Stancari, M., Stanco, L., Stanley, R., Stein, R., Steiner, H. M., Stewart, J., Stillwell, B., Stock, J., Stocker, F., Stokes, T., Strait, M., Strauss, T., Striganov, S., Stuart, A., Suarez, J. G., Sullivan, H., Summers, D., Surdo, A., Susic, V., Suter, L., Sutera, C. M., Svoboda, R., Szczerbinska, B., Szelc, A. M., Talaga, R., Tanaka, H. A., Oregui, B. T., Tapper, A., Tariq, S., Tatar, E., Tayloe, R., Teklu, A. M., Tenti, M., Terao, K., Ternes, C. A., Terranova, F., Testera, G., Thea, A., Thompson, J. L., Thorn, C., Timm, S. C., Todd, J., Tonazzo, A., Torbunov, D., Torti, M., Tortola, M., Tortorici, F., Totani, D., Toups, M., Touramanis, C., Tosi, N., Travaglini, R., Trevor, J., Trilov, S., Trzaska, W. H., Tsai, Y. T., Tsamalaidze, Z., Tsang, K. V., Tsverava, N., Tufanli, S., Tull, C., Tyley, E., Tzanov, M., Uchida, M. A., Urheim, J., Usher, T., Uzunyan, S., Vagins, M. R., Vahle, P., Valdiviesso, G. A., Valencia, E., Valerio, P., Vallari, Z., Valle, J. W. F., Vallecorsa, S., Van Berg, R., Van De Water, R. G., Varanini, F., Vargas, D., Varner, G., Vasel, J., Vasina, S., Vasseur, G., Vaughan, N., Vaziri, K., Ventura, S., Verdugo, A., Vergani, S., Vermeulen, M. A., Verzocchi, M., Vicenzi, M., Vieira De Souza, H., Vignoli, C., Vilela, C., Viren, B., Vrba, T., Wachala, T., Waldron, A. V., Wallbank, M., Wang, H., Wang, J., Wang, L., Wang, M. H. L. S., Wang, Y., Warburton, K., Warner, D., Wascko, M., Waters, D., Watson, A., Weatherly, P., Weber, A., Weber, M., Wei, H., Weinstein, A., Wenman, D., Wetstein, M., White, A., Whitehead, L. H., Whittington, D., Wilking, M. J., Wilkinson, C., Williams, Z., Wilson, F., Wilson, R. 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D., Zito, M., Zucchelli, S., Zuklin, J., Zutshi, V., Zwaska, R., Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de Physique des 2 Infinis Irène Joliot-Curie (IJCLab), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Saclay-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), DUNE, XENON (IHEF, IoP, FNWI), Other Research IHEF (IoP, FNWI), ATLAS (IHEF, IoP, FNWI), IHEF (IoP, FNWI), Abud A.A., Abi B., Acciarri R., Acero M.A., Adamov G., Adams D., Adinolfi M., Aduszkiewicz A., Ahmad Z., Ahmed J., Alion T., Monsalve S.A., Alrashed M., Alt C., Alton A., Amedo P., Anderson J., Andreopoulos C., Andrews M.P., Andrianala F., Andringa S., Anfimov N., Ankowski A., Antonova M., Antusch S., Aranda-Fernandez A., Ariga A., Arnold L.O., Arroyave M.A., Asaadi J., Aurisano A., Aushev V., Autiero D., Ayala-Torres M., Azfar F., Back A., Back H., Back J.J., Backhouse C., Baesso P., Bagaturia I., Bagby L., Balasubramanian S., Baldi P., Baller B., Bambah B., Barao F., Barenboim G., Barker G.J., Barkhouse W., Barnes C., Barr G., Monarca J.B., Barros N., Barrow J.L., Basharina-Freshville A., Bashyal A., Basque V., Belchior E., Battat J.B.R., Battisti F., Bay F., Alba J.L.B., Beacom J.F., Bechetoille E., Behera B., Bellantoni L., Bellettini G., Bellini V., Beltramello O., Belver D., Benekos N., Neves 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Papadimitriou V., Papaleo R., Papanestis A., Paramesvaran S., Parke S., Parsa Z., Parvu M., Pascoli S., Pasqualini L., Pasternak J., Pater J., Patrick C., Patrizii L., Patterson R.B., Patton S.J., Patzak T., Paudel A., Paulos B., Paulucci L., Pavlovic Z., Pawloski G., Payne D., Pec V., Peeters S.J.M., Pennacchio E., Penzo A., Peres O.L.G., Perry J., Pershey D., Pessina G., Petrillo G., Petta C., Petti R., Piastra F., Pickering L., Pietropaolo F., Plunkett R., Poling R., Pons X., Poonthottathil N., Poppi F., Pordes S., Porter J., Potekhin M., Potenza R., Potukuchi B.V.K.S., Pozimski J., Pozzato M., Prakash S., Prakash T., Prince S., Pugnere D., Qian X., Queiroga Bazetto M.C., Raaf J.L., Radeka V., Rademacker J., Radics B., Rafique A., Raguzin E., Rai M., Rajaoalisoa M., Rakhno I., Rakotonandrasana A., Rakotondravohitra L., Ramachers Y.A., Rameika R., Ramirez Delgado M.A., Ramson B., Rappoldi A., Raselli G., Ratoff P., Raut S., Razakamiandra R.F., Real J.S., Rebel B., Reggiani-Guzzo M., Rehak T., Reichenbacher J., Reitzner S.D., Rejeb Sfar H., Renshaw A., Rescia S., Resnati F., Reynolds A., Riccio C., Riccobene G., Rice L.C.J., Ricol J., Rigamonti A., Rigaut Y., Rivera D., Rochester L., Roda M., Rodrigues P., Rodriguez Alonso M.J., Rodriguez Bonilla E., Rodriguez Rondon J., Rosauro-Alcaraz S., Rosenberg M., Rosier P., Roskovec B., Rossella M., Rout J., Roy P., Roy S., Rubbia A., Rubbia C., Rubio F.C., Russell B., Ruterbories D., Saakyan R., Sacerdoti S., Safford T., Sahay R., Sahu N., Sala P., Samios N., Samoylov O., Sanchez M.C., Sanders D.A., Sankey D., Santana S., Santos-Maldonado M., Saoulidou N., Sapienza P., Sarasty C., Sarcevic I., Savage G., Savinov V., Scaramelli A., Scarff A., Scarpelli A., Schaffer T., Schellman H., Schlabach P., Schmitz D., Scholberg K., Schukraft A., Segreto E., Sensenig J., Seong I., Sergi A., Sgalaberna D., Shaevitz M.H., Shafaq S., Shamma M., Sharankova R., Sharma H.R., Sharma R., Shaw T., Shepherd-Themistocleous C., Shin S., Shooltz D., Shrock R., Simard L., Simon F., Simos N., Sinclair J., Sinev G., Singh J., Singh V., Sipos R., Sippach F.W., Sirri G., Sitraka A., Siyeon K., Skarpaas K., Smith A., Smith E., Smith P., Smolik J., Smy M., Snider E.L., Snopok P., Soares Nunes M., Sobel H., Soderberg M., Solano Salinas C.J., Soldner-Rembold S., Soleti S., Solomey N., Solovov V., Sondheim W.E., Sorel M., Soto-Oton J., Sousa A., Soustruznik K., Spagliardi F., Spanu M., Spitz J., Spooner N.J.C., Spurgeon K., Staley R., Stancari M., Stanco L., Stanley R., Stein R., Steiner H.M., Stewart J., Stillwell B., Stock J., Stocker F., Stokes T., Strait M., Strauss T., Striganov S., Stuart A., Suarez J.G., Sullivan H., Summers D., Surdo A., Susic V., Suter L., Sutera C.M., Svoboda R., Szczerbinska B., Szelc A.M., Talaga R., Tanaka H.A., Oregui B.T., Tapper A., Tariq S., Tatar E., Tayloe R., Teklu A.M., Tenti M., Terao K., Ternes C.A., Terranova F., Testera G., Thea A., Thompson J.L., Thorn C., Timm S.C., Todd J., Tonazzo A., Torbunov D., Torti M., Tortola M., Tortorici F., Totani D., Toups M., Touramanis C., Tosi N., Travaglini R., Trevor J., Trilov S., Trzaska W.H., Tsai Y.T., Tsamalaidze Z., Tsang K.V., Tsverava N., Tufanli S., Tull C., Tyley E., Tzanov M., Uchida M.A., Urheim J., Usher T., Uzunyan S., Vagins M.R., Vahle P., Valdiviesso G.A., Valencia E., Valerio P., Vallari Z., Valle J.W.F., Vallecorsa S., Van Berg R., Van De Water R.G., Varanini F., Vargas D., Varner G., Vasel J., Vasina S., Vasseur G., Vaughan N., Vaziri K., Ventura S., Verdugo A., Vergani S., Vermeulen M.A., Verzocchi M., Vicenzi M., Vieira De Souza H., Vignoli C., Vilela C., Viren B., Vrba T., Wachala T., Waldron A.V., Wallbank M., Wang H., Wang J., Wang L., Wang M.H.L.S., Wang Y., Warburton K., Warner D., Wascko M., Waters D., Watson A., Weatherly P., Weber A., Weber M., Wei H., Weinstein A., Wenman D., Wetstein M., White A., Whitehead L.H., Whittington D., Wilking M.J., Wilkinson C., Williams Z., Wilson F., Wilson R.J., Wolcott J., Wongjirad T., Wood A., Wood K., Worcester E., Worcester M., Wret C., Wu W., Xiao Y., Yandel E., Yang G., Yang K., Yang S., Yang T., Yankelevich A., Yershov N., Yonehara K., Young T., Yu B., Yu H., Yu J., Yuan W., Zaki R., Zalesak J., Zambelli L., Zamorano B., Zani A., Zazueta L., Zeit G., Zeller G.P., Zennamo J., Zeug K., Zhang C., Zhao M., Zhivun E., Zhu G., Zilberman P., Zimmerman E.D., Zito M., Zucchelli S., Zuklin J., Zutshi V., Zwaska R., Zeller, Geralyn, Collaboration, DUNE, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Abud, A, Abi, B, Acciarri, R, Acero, M, Adamov, G, Adams, D, Adinolfi, M, Aduszkiewicz, A, Ahmad, Z, Ahmed, J, Alion, T, Monsalve, S, Alrashed, M, Alt, C, Alton, A, Amedo, P, Anderson, J, Andreopoulos, C, Andrews, M, Andrianala, F, Andringa, S, Anfimov, N, Ankowski, A, Antonova, M, Antusch, S, Aranda-Fernandez, A, Ariga, A, Arnold, L, Arroyave, M, Asaadi, J, Aurisano, A, Aushev, V, Autiero, D, Ayala-Torres, M, Azfar, F, Back, A, Back, H, Back, J, Backhouse, C, Baesso, P, Bagaturia, I, Bagby, L, Balasubramanian, S, Baldi, P, Baller, B, Bambah, B, Barao, F, Barenboim, G, Barker, G, Barkhouse, W, Barnes, C, Barr, G, Monarca, J, Barros, N, Barrow, J, Basharina-Freshville, A, Bashyal, A, Basque, V, Belchior, E, Battat, J, Battisti, F, Bay, F, Alba, J, Beacom, J, Bechetoille, E, Behera, B, Bellantoni, L, Bellettini, G, Bellini, V, Beltramello, O, Belver, D, Benekos, N, Neves, F, Berkman, S, Bernardini, P, Berner, R, Berns, H, Bertolucci, S, Betancourt, M, Rodriguez, A, Bhattacharjee, M, Bhuller, S, Bhuyan, B, Biagi, S, Bian, J, Biassoni, M, Biery, K, Bilki, B, Bishai, M, Bitadze, A, Blake, A, Blaszczyk, F, Blazey, G, Blucher, E, Boissevain, J, Bolognesi, S, Bolton, T, Bomben, L, Bonesini, M, Bongrand, M, Bonini, F, Booth, A, Booth, C, Bordoni, S, Borkum, A, Boschi, T, Bostan, N, Bour, P, Bourgeois, C, Boyd, S, Boyden, D, Bracinik, J, Braga, D, Brailsford, D, Brandt, A, Bremer, J, Brew, C, Brianne, E, Brice, S, Brizzolari, C, Bromberg, C, Brooijmans, G, Brooke, J, Bross, A, Brunetti, G, Brunetti, M, Buchanan, N, Budd, H, Cagnoli, I, Caiulo, D, Calafiura, P, Calcutt, J, Calin, M, Calvez, S, Calvo, E, Caminata, A, Campanelli, M, Cankocak, K, Caratelli, D, Carini, G, Carlus, B, Carniti, P, Terrazas, I, Carranza, H, Carroll, T, Castano Forero, J, Castillo, A, Castromonte, C, Catano-Mur, E, Cattadori, C, Cavalier, F, Cavanna, F, Centro, S, Cerati, G, Cervelli, A, Villanueva, A, Chalifour, M, Chappell, A, Chardonnet, E, Charitonidis, N, Chatterjee, A, Chattopadhyay, S, Chen, H, Chen, M, Chen, Y, Chen, Z, Cherdack, D, Chi, C, Childress, S, Chiriacescu, A, Chisnall, G, Cho, K, Choate, S, Chokheli, D, Choubey, S, Christensen, A, Christian, D, Christodoulou, G, Chukanov, A, Church, E, Cicero, V, Clarke, P, Coan, T, Cocco, A, Coelho, J, Conley, E, Conley, R, Conrad, J, Convery, M, Copello, S, Corwin, L, Cremaldi, L, Cremonesi, L, Crespo-Anadon, J, Cristaldo, E, Cross, R, Cudd, A, Cuesta, C, Cui, Y, Cussans, D, Dabrowski, M, Dalager, O, Da Motta, H, Da Silva Peres, L, David, C, David, Q, Davies, G, Davini, S, Dawson, J, De, K, De Almeida, R, Debbins, P, De Bonis, I, Decowski, M, De Gouvea, A, De Holanda, P, De Icaza Astiz, I, Deisting, A, De Jong, P, Delbart, A, Delepine, D, Delgado, M, Dell'Acqua, A, De Lurgio, P, De Mello Neto, J, De Muth, D, Dennis, S, Densham, C, Deptuch, G, De Roeck, A, De Romeri, V, De Souza, G, Dharmapalan, R, Diaz, F, Diaz, J, Di Domizio, S, Di Giulio, L, Ding, P, Di Noto, L, Distefano, C, Diurba, R, Diwan, M, Djurcic, Z, Dokania, N, Dolan, S, Dolinski, M, Domine, L, Douglas, D, Douillet, D, Drake, G, Drielsma, F, Duchesneau, D, Duffy, K, Dunne, P, Durkin, T, Duyang, H, Dvornikov, O, Dwyer, D, Dyshkant, A, Eads, M, Earle, A, Edmunds, D, Eisch, J, Emberger, L, Emery, S, Ereditato, A, Escobar, C, Eurin, G, Evans, J, Ewart, E, Ezeribe, A, Fahey, K, Falcone, A, Farnese, C, Farzan, Y, Felix, J, Carneiro Da Silva, M, Fernandez-Martinez, E, Fernandez Menendez, P, Ferraro, F, Fields, L, Filthaut, F, Fiorentini, A, Fitzpatrick, R, Flanagan, W, Fleming, B, Flight, R, Forero, D, Fowler, J, Fox, W, Franc, J, Francis, K, Franco, D, Freeman, J, Freestone, J, Fried, J, Friedland, A, Fuess, S, Furic, I, Furmanski, A, Gabrielli, A, Gago, A, Gallagher, H, Gallas, A, Gallego-Ros, A, Gallice, N, Galymov, V, Gamberini, E, Gamble, T, Gandhi, R, Gandrajula, R, Gao, F, Gao, S, Garcia-Gamez, D, Garcia-Peris, M, Gardiner, S, Gastler, D, Ge, G, Gelli, B, Gendotti, A, Gent, S, Ghorbani-Moghaddam, Z, Gibin, D, Gil-Botella, I, Gilligan, S, Girerd, C, Giri, A, Gnani, D, Gogota, O, Gold, M, Gollapinni, S, Gollwitzer, K, Gomes, R, Gomez Bermeo, L, Gomez Fajardo, L, Gonnella, F, Gonzalez-Cuevas, J, Gonzalez-Diaz, D, Gonzalez-Lopez, M, Goodman, M, Goodwin, O, Goswami, S, Gotti, C, Goudzovski, E, Grace, C, Graham, M, Gran, R, Granados, E, Granger, P, Grant, A, Grant, C, Gratieri, D, Green, P, Greenler, L, Greer, J, Griffith, W, Groh, M, Grudzinski, J, Grzelak, K, Gu, W, Guarino, V, Guenette, R, Guerard, E, Guerzoni, M, Guglielmi, A, Guo, B, Guthikonda, K, Gutierrez, R, Guzowski, P, Guzzo, M, Gwon, S, Habig, A, Hadavand, H, Haenni, R, Hahn, A, Haiston, J, Hamacher-Baumann, P, Hamernik, T, Hamilton, P, Han, J, Harris, D, Hartnell, J, Harton, J, Hasegawa, T, Hasnip, C, Hatcher, R, Hatfield, K, Hatzikoutelis, A, Hayes, C, Hazen, E, Heavey, A, Heeger, K, Heise, J, Hennessy, K, Henry, S, Hernandez Morquecho, M, Herner, K, Hertel, L, Hewes, J, Higuera, A, Hill, T, Hillier, S, Himmel, A, Hoff, J, Hohl, C, Holin, A, Hoppe, E, Horton-Smith, G, Hostert, M, Hourlier, A, Howard, B, Howell, R, Huang, J, Hugon, J, Iles, G, Ilic, N, Iliescu, A, Illingworth, R, Ingratta, G, Ioannisian, A, Isenhower, L, Itay, R, Izmaylov, A, Jackson, S, Jain, V, James, E, Jargowsky, B, Jediny, F, Jena, D, Jeong, Y, Jesus-Valls, C, Ji, X, Jiang, L, Jimenez, S, Jipa, A, Johnson, R, Johnston, N, Jones, B, Jones, S, Judah, M, Jung, C, Junk, T, Jwa, Y, Kabirnezhad, M, Kaboth, A, Kadenko, I, Kakorin, I, Kamiya, F, Kaneshige, N, Karagiorgi, G, Karaman, G, Karcher, A, Karolak, M, Karyotakis, Y, Kasai, S, Kasetti, S, Kashur, L, Kazaryan, N, Kearns, E, Keener, P, Kelly, K, Kemp, E, Kemularia, O, Ketchum, W, Kettell, S, Khabibullin, M, Khotjantsev, A, Khvedelidze, A, Kim, D, King, B, Kirby, B, Kirby, M, Klein, J, Koehler, K, Koerner, L, Kohn, S, Koller, P, Kolupaeva, L, Kordosky, M, Kosc, T, Kose, U, Kostelecky, V, Kothekar, K, Krennrich, F, Kreslo, I, Kudenko, Y, Kudryavtsev, V, Kulagin, S, Kumar, J, Kumar, P, Kumar, R, Kunze, P, Kurita, N, Kuruppu, C, Kus, V, Kutter, T, Lambert, A, Land, B, Lande, K, Lane, C, Lang, K, Langford, T, Larkin, J, Lasorak, P, Last, D, Lastoria, C, Laundrie, A, Laurenti, G, Lawrence, A, Lazanu, I, Lazur, R, Le, T, Leardini, S, Learned, J, Lebrun, P, Lecompte, T, Lehmann Miotto, G, Lehnert, R, Leigui De Oliveira, M, Leitner, M, Li, L, Li, S, Li, T, Li, Y, Liao, H, Lin, C, Lin, Q, Lin, S, Lister, A, Littlejohn, B, Liu, J, Lockwitz, S, Loew, T, Lokajicek, M, Lomidze, I, Long, K, Loo, K, Lorca, D, Lord, T, Losecco, J, Louis, W, Lu, X, Luk, K, Luo, X, Lurkin, N, Lux, T, Luzio, V, Macfarlane, D, Machado, A, Machado, P, Macias, C, Macier, J, Maddalena, A, Madera, A, Madigan, P, Magill, S, Mahn, K, Maio, A, Major, A, Maloney, J, Mandrioli, G, Mandujano, R, Maneira, J, Manenti, L, Manly, S, Mann, A, Manolopoulos, K, Manrique Plata, M, Manyam, V, Manzanillas, L, Marchan, M, Marchionni, A, Marciano, W, Marfatia, D, Mariani, C, Maricic, J, Marie, R, Marinho, F, Marino, A, Marsden, D, Marshak, M, Marshall, C, Marshall, J, Marteau, J, Martin-Albo, J, Martinez, N, Martinez Caicedo, D, Martynenko, S, Mason, K, Mastbaum, A, Masud, M, Matsuno, S, Matthews, J, Mauger, C, Mauri, N, Mavrokoridis, K, Mawby, I, Mazza, R, Mazzacane, A, Mazzucato, E, Mcaskill, T, Mccluskey, E, Mcconkey, N, Mcfarland, K, Mcgrew, C, Mcnab, A, Mefodiev, A, Mehta, P, Melas, P, Mena, O, Menary, S, Mendez, H, Mendez, D, Menegolli, A, Meng, G, Messier, M, Metcalf, W, Mettler, T, Mewes, M, Meyer, H, Miao, T, Michna, G, Miedema, T, Migenda, J, Mikola, V, Milincic, R, Miller, W, Mills, J, Milne, C, Mineev, O, Miranda, O, Miryala, S, Mishra, C, Mishra, S, Mislivec, A, Mladenov, D, Mocioiu, I, Moffat, K, Moggi, N, Mohanta, R, Mohayai, T, Mokhov, N, Molina, J, Molina Bueno, L, Montanari, A, Montanari, C, Montanari, D, Montagna, E, Montano Zetina, L, Moon, J, Mooney, M, Moor, A, Moreno, D, Morris, C, Mossey, C, Motuk, E, Moura, C, Mousseau, J, Mu, W, Mualem, L, Mueller, J, Muether, M, Mufson, S, Muheim, F, Muir, A, Mulhearn, M, Munford, D, Muramatsu, H, Murphy, S, Musser, J, Nachtman, J, Nagu, S, Nalbandyan, M, Nandakumar, R, Naples, D, Narita, S, Navas-Nicolas, D, Navrer-Agasson, A, Nayak, N, Nebot-Guinot, M, Negishi, K, Nelson, J, Nesbit, J, Nessi, M, Newbold, D, Newcomer, M, Newhart, D, Newton, H, Niccolo, M, Nichol, R, Nicolas-Arnaldos, F, Nicoletta, M, Niner, E, Nishimura, K, Norman, A, Norrick, A, Northrop, R, Novella, P, Nowak, J, Oberling, M, Ochoa-Ricoux, J, Olivares Del Campo, A, Olivier, A, Olshevskiy, A, Onel, Y, Onishchuk, Y, Ott, J, Pagani, L, Pakvasa, S, Palacio, G, Palamara, O, Palestini, S, Paley, J, Pallavicini, M, Palomares, C, Palomino-Gallo, J, Pantic, E, Paolone, V, Papadimitriou, V, Papaleo, R, Papanestis, A, Paramesvaran, S, Parke, S, Parsa, Z, Parvu, M, Pascoli, S, Pasqualini, L, Pasternak, J, Pater, J, Patrick, C, Patrizii, L, Patterson, R, Patton, S, Patzak, T, Paudel, A, Paulos, B, Paulucci, L, Pavlovic, Z, Pawloski, G, Payne, D, Pec, V, Peeters, S, Pennacchio, E, Penzo, A, Peres, O, Perry, J, Pershey, D, Pessina, G, Petrillo, G, Petta, C, Petti, R, Piastra, F, Pickering, L, Pietropaolo, F, Plunkett, R, Poling, R, Pons, X, Poonthottathil, N, Poppi, F, Pordes, S, Porter, J, Potekhin, M, Potenza, R, Potukuchi, B, Pozimski, J, Pozzato, M, Prakash, S, Prakash, T, Prince, S, Pugnere, D, Qian, X, Queiroga Bazetto, M, Raaf, J, Radeka, V, Rademacker, J, Radics, B, Rafique, A, Raguzin, E, Rai, M, Rajaoalisoa, M, Rakhno, I, Rakotonandrasana, A, Rakotondravohitra, L, Ramachers, Y, Rameika, R, Ramirez Delgado, M, Ramson, B, Rappoldi, A, Raselli, G, Ratoff, P, Raut, S, Razakamiandra, R, Real, J, Rebel, B, Reggiani-Guzzo, M, Rehak, T, Reichenbacher, J, Reitzner, S, Rejeb Sfar, H, Renshaw, A, Rescia, S, Resnati, F, Reynolds, A, Riccio, C, Riccobene, G, Rice, L, Ricol, J, Rigamonti, A, Rigaut, Y, Rivera, D, Rochester, L, Roda, M, Rodrigues, P, Rodriguez Alonso, M, Rodriguez Bonilla, E, Rodriguez Rondon, J, Rosauro-Alcaraz, S, Rosenberg, M, Rosier, P, Roskovec, B, Rossella, M, Rout, J, Roy, P, Roy, S, Rubbia, A, Rubbia, C, Rubio, F, Russell, B, Ruterbories, D, Saakyan, R, Sacerdoti, S, Safford, T, Sahay, R, Sahu, N, Sala, P, Samios, N, Samoylov, O, Sanchez, M, Sanders, D, Sankey, D, Santana, S, Santos-Maldonado, M, Saoulidou, N, Sapienza, P, Sarasty, C, Sarcevic, I, Savage, G, Savinov, V, Scaramelli, A, Scarff, A, Scarpelli, A, Schaffer, T, Schellman, H, Schlabach, P, Schmitz, D, Scholberg, K, Schukraft, A, Segreto, E, Sensenig, J, Seong, I, Sergi, A, Sgalaberna, D, Shaevitz, M, Shafaq, S, Shamma, M, Sharankova, R, Sharma, H, Sharma, R, Shaw, T, Shepherd-Themistocleous, C, Shin, S, Shooltz, D, Shrock, R, Simard, L, Simon, F, Simos, N, Sinclair, J, Sinev, G, Singh, J, Singh, V, Sipos, R, Sippach, F, Sirri, G, Sitraka, A, Siyeon, K, Skarpaas, K, Smith, A, Smith, E, Smith, P, Smolik, J, Smy, M, Snider, E, Snopok, P, Soares Nunes, M, Sobel, H, Soderberg, M, Solano Salinas, C, Soldner-Rembold, S, Soleti, S, Solomey, N, Solovov, V, Sondheim, W, Sorel, M, Soto-Oton, J, Sousa, A, Soustruznik, K, Spagliardi, F, Spanu, M, Spitz, J, Spooner, N, Spurgeon, K, Staley, R, Stancari, M, Stanco, L, Stanley, R, Stein, R, Steiner, H, Stewart, J, Stillwell, B, Stock, J, Stocker, F, Stokes, T, Strait, M, Strauss, T, Striganov, S, Stuart, A, Suarez, J, Sullivan, H, Summers, D, Surdo, A, Susic, V, Suter, L, Sutera, C, Svoboda, R, Szczerbinska, B, Szelc, A, Talaga, R, Tanaka, H, Oregui, B, Tapper, A, Tariq, S, Tatar, E, Tayloe, R, Teklu, A, Tenti, M, Terao, K, Ternes, C, Terranova, F, Testera, G, Thea, A, Thompson, J, Thorn, C, Timm, S, Todd, J, Tonazzo, A, Torbunov, D, Torti, M, Tortola, M, Tortorici, F, Totani, D, Toups, M, Touramanis, C, Tosi, N, Travaglini, R, Trevor, J, Trilov, S, Trzaska, W, Tsai, Y, Tsamalaidze, Z, Tsang, K, Tsverava, N, Tufanli, S, Tull, C, Tyley, E, Tzanov, M, Uchida, M, Urheim, J, Usher, T, Uzunyan, S, Vagins, M, Vahle, P, Valdiviesso, G, Valencia, E, Valerio, P, Vallari, Z, Valle, J, Vallecorsa, S, Van Berg, R, Van De Water, R, Varanini, F, Vargas, D, Varner, G, Vasel, J, Vasina, S, Vasseur, G, Vaughan, N, Vaziri, K, Ventura, S, Verdugo, A, Vergani, S, Vermeulen, M, Verzocchi, M, Vicenzi, M, Vieira De Souza, H, Vignoli, C, Vilela, C, Viren, B, Vrba, T, Wachala, T, Waldron, A, Wallbank, M, Wang, H, Wang, J, Wang, L, Wang, M, Wang, Y, Warburton, K, Warner, D, Wascko, M, Waters, D, Watson, A, Weatherly, P, Weber, A, Weber, M, Wei, H, Weinstein, A, Wenman, D, Wetstein, M, White, A, Whitehead, L, Whittington, D, Wilking, M, Wilkinson, C, Williams, Z, Wilson, F, Wilson, R, Wolcott, J, Wongjirad, T, Wood, A, Wood, K, Worcester, E, Worcester, M, Wret, C, Wu, W, Xiao, Y, Yandel, E, Yang, G, Yang, K, Yang, S, Yang, T, Yankelevich, A, Yershov, N, Yonehara, K, Young, T, Yu, B, Yu, H, Yu, J, Yuan, W, Zaki, R, Zalesak, J, Zambelli, L, Zamorano, B, Zani, A, Zazueta, L, Zeit, G, Zeller, G, Zennamo, J, Zeug, K, Zhang, C, Zhao, M, Zhivun, E, Zhu, G, Zilberman, P, Zimmerman, E, Zito, M, Zucchelli, S, Zuklin, J, Zutshi, V, Zwaska, R, and The DUNE Collaboration
- Subjects
Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,Physics beyond the Standard Model ,far detector ,QC770-798 ,7. Clean energy ,01 natural sciences ,High Energy Physics - Experiment ,design [detector] ,Near detector ,High Energy Physics - Experiment (hep-ex) ,neutrino ,Conceptual design ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,antimatter ,Detectors and Experimental Techniques ,Instrumentation ,physics.ins-det ,QC ,media_common ,QB ,Physics ,new physics ,Neutrino oscillations ,Detector ,Instrumentation and Detectors (physics.ins-det) ,oscillation ,Antimatter ,beam ,Neutrino ,Particle Physics - Experiment ,performance ,Neutrino oscillation ,530 Physics ,Deep Underground Neutrino Experiment ,DUNE ,media_common.quotation_subject ,QC1-999 ,FOS: Physical sciences ,interaction ,near detector ,Nuclear and particle physics. Atomic energy. Radioactivity ,0103 physical sciences ,supernova ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,010306 general physics ,detector: design ,activity report ,neutrino oscillations ,010308 nuclear & particles physics ,hep-ex ,Astronomy ,Universe ,High Energy Physics::Experiment - Abstract
FERMILAB-PUB-21-067-E-LBNF-PPD-SCD-T This document was prepared by the DUNE collaboration using the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under Contract No. DE-AC02-07CH11359. This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America. This research used resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231., This work was supported by CNPq, FAPERJ, FAPEG and FAPESP, Brazil; CFI, IPP and NSERC, Canada; CERN; MŠMT, Czech Republic; ERDF, H2020-EU and MSCA, European Union; CNRS/IN2P3 and CEA, France; INFN, Italy; FCT, Portugal; NRF, South Korea; CAM, Fundación “La Caixa”, MICINN, GVA, Xunta de Galicia and AEI, Spain; SERI and SNSF, Switzerland; TÜBİTAK, Turkey; The Royal Society and UKRI/STFC, United Kingdom; DOE and NSF, United States of America., The Deep Underground Neutrino Experiment (DUNE) is an international, world-class experiment aimed at exploring fundamental questions about the universe that are at the forefront of astrophysics and particle physics research. DUNE will study questions pertaining to the preponderance of matter over antimatter in the early universe, the dynamics of supernovae, the subtleties of neutrino interaction physics, and a number of beyond the Standard Model topics accessible in a powerful neutrino beam. A critical component of the DUNE physics program involves the study of changes in a powerful beam of neutrinos, i.e., neutrino oscillations, as the neutrinos propagate a long distance. The experiment consists of a near detector, sited close to the source of the beam, and a far detector, sited along the beam at a large distance. This document, the DUNE Near Detector Conceptual Design Report (CDR), describes the design of the DUNE near detector and the science program that drives the design and technology choices. The goals and requirements underlying the design, along with projected performance are given. It serves as a starting point for a more detailed design that will be described in future documents., Fermi Research Alliance, LLC DE-AC02-07CH11359, H2020-EU, TÜBİTAK, National Science Foundation, U.S. Department of Energy DE-AC02-05CH11231, Multiple Sclerosis Center of Atlanta, CERN, UK Research and Innovation, Natural Sciences and Engineering Research Council of Canada, Science and Technology Facilities Council, Royal Society, European Commission, Singapore Eye Research Institute, Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung, Fundação de Amparo à Pesquisa do Estado de São Paulo, Ministerstvo Školství, Mládeže a Tělovýchovy, Fundação para a Ciência e a Tecnologia, Generalitat Valenciana, Conselho Nacional de Desenvolvimento Científico e Tecnológico, National Research Foundation of Korea, Instituto Nazionale di Fisica Nucleare, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Centre National de la Recherche Scientifique, Ministerio de Ciencia e Innovación, Fundação de Amparo à Pesquisa do Estado de Goiás, Commissariat à l'Énergie Atomique et aux Énergies Alternatives, European Regional Development Fund, Xunta de Galicia, Agencia Estatal de Investigación, Institut National de Physique Nucléaire et de Physique des Particules
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- 2021
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91. (In)direct detection of boosted dark matter
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Massachusetts Institute of Technology. Center for Theoretical Physics, Massachusetts Institute of Technology. Department of Physics, Agashe, Kaustubh, Cui, Yanou, Necib, Lina, Thaler, Jesse, Massachusetts Institute of Technology. Center for Theoretical Physics, Massachusetts Institute of Technology. Department of Physics, Agashe, Kaustubh, Cui, Yanou, Necib, Lina, and Thaler, Jesse
- Abstract
We initiate the study of novel thermal dark matter (DM) scenarios where present-day annihilation of DM in the galactic center produces boosted stable particles in the dark sector. These stable particles are typically a subdominant DM component, but because they are produced with a large Lorentz boost in this process, they can be detected in large volume terrestrial experiments via neutral-current-like interactions with electrons or nuclei. This novel DM signal thus combines the production mechanism associated with indirect detection experiments (i.e. galactic DM annihilation) with the detection mechanism associated with direct detection experiments (i.e. DM scattering off terrestrial targets). Such processes are generically present in multi-component DM scenarios or those with non-minimal DM stabilization symmetries. As a proof of concept, we present a model of two-component thermal relic DM, where the dominant heavy DM species has no tree-level interactions with the standard model and thus largely evades direct and indirect DM bounds. Instead, its thermal relic abundance is set by annihilation into a subdominant lighter DM species, and the latter can be detected in the boosted channel via the same annihilation process occurring today. Especially for dark sector masses in the 10 MeV-10 GeV range, the most promising signals are electron scattering events pointing toward the galactic center. These can be detected in experiments designed for neutrino physics or proton decay, in particular Super-K and its upgrade Hyper-K, as well as the PINGU/MICA extensions of IceCube. This boosted DM phenomenon highlights the distinctive signatures possible from non-minimal dark sectors. ©2014, U.S. Department of Energy (no. DE-FG02-05ER-41360), DOE Early Career research program (DE-FG02-11ER-41741)
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- 2021
92. Long-Lived Particles at the Energy Frontier: The MATHUSLA Physics Case
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Massachusetts Institute of Technology. Department of Physics, Curtin, David, Drewes, Marco, McCullough, Matthew, Meade, Patrick, Mohapatra, Rabindra N, Shelton, Jessie, Shuve, Brian, Accomando, Elena, Alpigiani, Cristiano, Antusch, Stefan, Carlos Arteaga-Velázquez, Juan, Batell, Brian, Bauer, Martin, Blinov, Nikita, Salomé Caballero-Mora, Karen, Hyeok Chang, Jae, Chun, Eung Jin, Co, Raymond T, Cohen, Timothy, Cox, Peter, Craig, Nathaniel, Csáki, Csaba, Cui, Yanou, D’Eramo, Francesco, Delle Rose, Luigi, Bhupal Dev, P S, Dienes, Keith R, Dror, Jeff A, Essig, Rouven, Evans, Jared A, Evans, Jason L, Fernández Tellez, Arturo, Fischer, Oliver, Flacke, Thomas, Fradette, Anthony, Frugiuele, Claudia, Fuchs, Elina, Gherghetta, Tony, Giudice, Gian F, Gorbunov, Dmitry, Gupta, Rick S, Hagedorn, Claudia, Hall, Lawrence J, Harris, Philip, Carlos Helo, Juan, Hirsch, Martin, Hochberg, Yonit, Hook, Anson, Ibarra, Alejandro, Ipek, Seyda, Jung, Sunghoon, Knapen, Simon, Kuflik, Eric, Liu, Zhen, Lombardo, Salvator, Lubatti, H J, McKeen, David, Molinaro, Emiliano, Moretti, Stefano, Nagata, Natsumi, Neubert, Matthias, Miguel No, Jose, Olaiya, Emmanuel, Perez, Gilad, Peskin, Michael E, Pinner, David, Pospelov, Maxim, Reece, Matthew, Robinson, Dean J, Rodríguez Cahuantzi, Mario, Santonico, Rinaldo, Schlaffer, Matthias, Shepherd-Themistocleous, Claire H, Spray, Andrew, Stolarski, Daniel, Subieta Vasquez, Martin A, Sundrum, Raman, Thamm, Andrea, Thomas, Brooks, Tsai, Yuhsin, Tweedie, Brock, West, Stephen M, Young, Charles, Yu, Felix, Zaldivar, Bryan, Zhang, Yongchao, Zurek, Kathryn, Zurita, José, Massachusetts Institute of Technology. Department of Physics, Curtin, David, Drewes, Marco, McCullough, Matthew, Meade, Patrick, Mohapatra, Rabindra N, Shelton, Jessie, Shuve, Brian, Accomando, Elena, Alpigiani, Cristiano, Antusch, Stefan, Carlos Arteaga-Velázquez, Juan, Batell, Brian, Bauer, Martin, Blinov, Nikita, Salomé Caballero-Mora, Karen, Hyeok Chang, Jae, Chun, Eung Jin, Co, Raymond T, Cohen, Timothy, Cox, Peter, Craig, Nathaniel, Csáki, Csaba, Cui, Yanou, D’Eramo, Francesco, Delle Rose, Luigi, Bhupal Dev, P S, Dienes, Keith R, Dror, Jeff A, Essig, Rouven, Evans, Jared A, Evans, Jason L, Fernández Tellez, Arturo, Fischer, Oliver, Flacke, Thomas, Fradette, Anthony, Frugiuele, Claudia, Fuchs, Elina, Gherghetta, Tony, Giudice, Gian F, Gorbunov, Dmitry, Gupta, Rick S, Hagedorn, Claudia, Hall, Lawrence J, Harris, Philip, Carlos Helo, Juan, Hirsch, Martin, Hochberg, Yonit, Hook, Anson, Ibarra, Alejandro, Ipek, Seyda, Jung, Sunghoon, Knapen, Simon, Kuflik, Eric, Liu, Zhen, Lombardo, Salvator, Lubatti, H J, McKeen, David, Molinaro, Emiliano, Moretti, Stefano, Nagata, Natsumi, Neubert, Matthias, Miguel No, Jose, Olaiya, Emmanuel, Perez, Gilad, Peskin, Michael E, Pinner, David, Pospelov, Maxim, Reece, Matthew, Robinson, Dean J, Rodríguez Cahuantzi, Mario, Santonico, Rinaldo, Schlaffer, Matthias, Shepherd-Themistocleous, Claire H, Spray, Andrew, Stolarski, Daniel, Subieta Vasquez, Martin A, Sundrum, Raman, Thamm, Andrea, Thomas, Brooks, Tsai, Yuhsin, Tweedie, Brock, West, Stephen M, Young, Charles, Yu, Felix, Zaldivar, Bryan, Zhang, Yongchao, Zurek, Kathryn, and Zurita, José
- Abstract
© 2019 IOP Publishing Ltd. We examine the theoretical motivations for long-lived particle (LLP) signals at the LHC in a comprehensive survey of standard model (SM) extensions. LLPs are a common prediction of a wide range of theories that address unsolved fundamental mysteries such as naturalness, dark matter, baryogenesis and neutrino masses, and represent a natural and generic possibility for physics beyond the SM (BSM). In most cases the LLP lifetime can be treated as a free parameter from the m scale up to the Big Bang Nucleosynthesis limit of m. Neutral LLPs with lifetimes above 100 m are particularly difficult to probe, as the sensitivity of the LHC main detectors is limited by challenging backgrounds, triggers, and small acceptances. MATHUSLA is a proposal for a minimally instrumented, large-volume surface detector near ATLAS or CMS. It would search for neutral LLPs produced in HL-LHC collisions by reconstructing displaced vertices (DVs) in a low-background environment, extending the sensitivity of the main detectors by orders of magnitude in the long-lifetime regime. We study the LLP physics opportunities afforded by a MATHUSLA-like detector at the HL-LHC, assuming backgrounds can be rejected as expected. We develop a model-independent approach to describe the sensitivity of MATHUSLA to BSM LLP signals, and compare it to DV and missing energy searches at ATLAS or CMS. We then explore the BSM motivations for LLPs in considerable detail, presenting a large number of new sensitivity studies. While our discussion is especially oriented towards the long-lifetime regime at MATHUSLA, this survey underlines the importance of a varied LLP search program at the LHC in general. By synthesizing these results into a general discussion of the top-down and bottom-up motivations for LLP searches, it is our aim to demonstrate the exceptional strength and breadth of the physics case for the construction of the MATHUSLA detector.
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- 2021
93. A WIMPy baryogenesis miracle
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Cui, Yanou, Randall, Lisa, and Shuve, Brian
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- 2012
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94. Prospects for detecting boosted dark matter in DUNE through hadronic interactions
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Berger, Joshua, primary, Cui, Yanou, additional, Graham, Mathew, additional, Necib, Lina, additional, Petrillo, Gianluca, additional, Stocks, Dane, additional, Tsai, Yun-Tse, additional, and Zhao, Yue, additional
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- 2021
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95. Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume I Introduction to DUNE
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Abi, Babak, Acciarri, Roberto, Acero, Mario, Adamov, Giorge, Adams, David, Adinolfi, Marco, Ahmad, Zubayer, Ahmed, Jhanzeb, Alion, Tyler, Alonso Monsalve, Saul, Alt, Christoph, Anderson, John, Andreopoulos, Costas, Andrews, Michael P, Andriamirado, Manoa, Andrianala, Fenompanirina, Andringa, Sofia, Ankowski, Artur, Anthony, Jack, Antoniu, Iliescu, Antonova, Maria, Antusch, Stefan, Aranda Fernandez, Alfredo, Ariga, Akitaka, Arnold, Lukas, Arroyave, Manuel, Asaadi, Jonathan, Aurisano, Adam, Aushev, Vladimir, Autiero, Dario, Azfar, Farrukh, Back, Ashley, Back, Henning, Back, John, Backhouse, Chris, Baesso, Paolo, Bagby, Linda, Bajou, Raphael, Balasubramanian, Supraja, Baldi, Pierre, Bambah, Bindu, Barao, Fernando, Barenboim, Gabriela, Barker, Gary J, Barkhouse, Wayne, Barnes, Christopher, Barr, Giles, Barranco Monarca, Juan, Barros, Nuno, Barrow, Joshua, Bashyal, Amit, Basque, Vincent, Bay, Fatih, Bazo Alba, J.L., Beacom, John, Bechetoille, Edouard, Behera, Biswaranjan, Bellantoni, Leo, Bellettini, Giorgio, Bellini, Vincenzo, Beltramello, Olga, Belver, D., Benekos, Nektarios, Bento Neves, Francisco, Berger, Joshua, Berkman, Sophie, Bernardini, Paolo, Berner, Roman, Berns, Hans-Gerd, Bertolucci, Sergio, Betancourt, Minerba, Bezawada, Y., Bhattacharjee, maharnab, Bhuyan, Bipul, Biagi, Simone, Bian, Jianming, Biassoni, Matteo, Biery, Kurt, Bilki, Burak, Bishai, Mary, Bitadze, Alexander, Blake, Andrew, Blanco Siffert, Beatriz, Blaszczyk, Flor de Maria, Blazey, Gerald C, Blucher, Edward, Boissevain, Jan, Bolognesi, Sara, Bolton, Timothy, Bonesini, Maurizio, Bongrand, Mathieu, Bonini, Filiberto, Booth, Alexander, Booth, Chris, Bordoni, Stefania, Borkum, Aran, Boschi, Tommaso, Bostan, Nilay, Bour, Petr, Boyd, Steve B, Boyden, Daniel, Bracinik, Juraj, Braga, Davide, Brailsford, Dominic, Brandt, Andrew, Bremer, Johan, Brew, Chris, Brianne, Eldwan, Brice, Stephen, Brizzolari, Claudia, Bromberg, Carl, Brooijmans, Gustaaf, Brooke, Jim, Bross, Alan, Brunetti, Giulia, Buchanan, Norman, Budd, Howard, Caiulo, Davide, Calafiura, Paolo, Calcutt, Jacob, Calin, Marius, Calvez, Steven, Calvo, Enrique, Camilleri, Leslie, Caminata, Alessio, Campanelli, Mario, Caratelli, David, Carini, Gabriella, Carlus, Bruno, Carniti, Paolo, Caro Terrazas, Ivan, Carranza, Hector, Castillo, Andrés, Castromonte, Cesar, Cattadori, Carla, Cavalier, Fabien, Cavanna, Flavio, Centro, Sandro, Cerati, Giuseppe, Cervelli, Alberto, Cervera Villanueva, Anselmo, Chalifour, Michel, Chang, C., Chardonnet, Etienne, Chatterjee, Animesh, Chattopadhyay, Subhasish, Chaves, Jorge, Chen, Hucheng, Chen, Mu-Chun, Chen, Yifan, Cherdack, Daniel, Chi, Cheng-Yi, Childress, Sam, Chiriacescu, Ana, Cho, Kihyeon, Choubey, Sandhya, Christensen, Anne, Christian, David, Christodoulou, Georgios, Church, Eric, Clarke, Peter, Coan, Thomas, Cocco, Alfredo, Coelho, Joao, Conley, Erin, Conrad, Janet M, Convery, Mark, Corwin, Luke, Cotte, Philippe, Cremaldi, Lucien, Cremonesi, Linda, Crespo-Anadón, Jose I, Cristaldo, Esteban, Cross, Ryan, Cuesta, Clara, Cui, Yanou, Cussans, David, Dabrowski, Mieczyslaw, Da Motta, Helio, Peres, L. Da Silva, David, Quentin, Davies, Gavin, Davini, Stefano, Dawson, Jaime, De, Kaushik, de Almeida, Rogerio, Debbins, Paul, De Bonis, Isabelle, Decowski, M Patrick, de Gouvea, Andre, de Holanda, Pedro, de Icaza Astiz, Iker, Deisting, Alexander, De Jong, Paul, Delbart, Alain, Delepine, David, Delgado, Maritza, Dell'Acqua, Andrea, De Lurgio, Patrick, Ewart, Kevin, Grant, Nick, Hernandez Morquecho, Miguel Angel, Hewes, Jeremy, Huang, Junting, Huang, Junying, Leigui de Oliveira, M A, Li, Shaorui, Li, Shirley W, Ramirez Delgado, Manuel Alejandro, Singh, Jaydip, Singh, Jyotsna, Smith, Adryanna, Smith, Andrew, Todd, Jacob, Torres de Mello Neto, Joao, DeMuth, David, Dennis, Steve, Densham, Chris, Gregor Recalde, Derlis, De Roeck, Albert, De Romeri, Valentina, Jan De Vries, Joris, Dharmapalan, Ranjan, Diaz, Felix, Diaz, Jorge S, Di Domizio, Sergio, Di Giulio, Letizia, Ding, Pengfei, Di Noto, Lea, Distefano, Carla, Diurba, Richard, Diwan, Milind, Djurcic, Zelimir, Dokania, Neha, Dolinski, Michelle J, Domine, Laura, Douglas, Daniel, Drielsma, Francois, Duchesneau, Dominique, Duffy, Kirsty, Dunne, Patrick, Durkin, Tim, Duyang, Hongyue, Dvornikov, Olexiy, Dwyer, Daniel A, Dyshkant, Alexandre S, Eads, Michael, Edmunds, Daniel, Eisch, Jonathan, Emery, Sandrine, Ereditato, Antonio, Escobar, Carlos O, Escudero Sanchez, Lorena, Evans, Justin, Ewart, E., Ezeribe, Anthony, Fahey, Kevin, Falcone, Andrea, Farnese, Christian, Farzan, Yasaman, Felix, Julian, Fernandez-Martinez, Enrique, Fernandez Menendez, Pablo, Ferraro, Federico, Fields, Laura, Filkins, A., Filthaut, Frank, Fitzpatrick, Rory, Flanagan, Will, Fleming, Bonnie, Flight, Robert, Fowler, Jack, Fox, Walt, Franc, Jiri, Francis, Kurt, Franco, Domenico, Freeman, John, Freestone, Julian, Fried, Jack, Friedland, Alex, Fuess, Stu, Furic, Ivan, Furmanski, Andrew, Gago, A., Gallagher, Hugh, Gallego-Ros, Ana, Gallice, Niccolo, Galymov, Vyacheslav, Gamberini, Enrico, Gamble, Trevor, Gandhi, Raj, Gandrajula, Reddy, Gao, Shanshan, Garcia-Gamez, Diego, García-Peris, Miguel, Gardiner, Steven, Gastler, Dan, Ge, Guanqun, Gelli, Bruno, Gendotti, Adamo, Gent, Stephen, Ghorbani-Moghaddam, Zahra, Gibin, Daniele, Gil-Botella, Ines, Girerd, Claude, Giri, Anjan Kumar, Gnani, D., Gogota, Olga, Gold, Michael, Gollapinni, Sowjanya, Gollwitzer, Keith, Gomes, Ricardo, Gomez Bermeo, Laura Vanessa, Gomez Fajardo, Luz, Gonnella, Francesco, Gonzalez-Cuevas, Juan Alberto, Goodman, Maury, Goodwin, Owen, Goswami, Srubabati, Gotti, Claudio, Goudzovski, Evgueni, Grace, Carl, Graham, Mathew, Gramellini, E., Gran, Rik, Granados, Everardo, Grant, Alan, Grant, Christopher, Gratieri, Diego, Green, Patrick, Green, Steven, Greenler, Leland, Greenwood, M., Greer, Joel, Griffith, Clark, Groh, Micah, Grudzinski, James, Grzelak, Katarzyna, Gu, Wenqiang, Guarino, Victor, Guenette, Roxanne, Guglielmi, Alberto, Guo, Bing, Guthikonda, K K, Gutierrez, Rafael, Guzowski, Pawel, Guzzo, Marcelo, Gwon, Sunwoo, Habig, Alec, Hackenburg, A., Hadavand, Haleh, Haenni, Roger, Hahn, Alan, Haigh, Jennifer, Haiston, James, Hamernik, Thomas, Hamilton, Philip, Han, Jiyeon, Harder, Kristian, Harris, Debbie, Hartnell, Jeffrey, Hasegawa, Takyua, Hatcher, Robert, Hazen, Eric, Heavey, Anne, Heeger, Karsten, Hennessy, Karol, Henry, Sarah, Herner, Kenneth, Hertel, Lars, Hewes, V., Higuera Pichardo, Aaron, Hill, Tony, Hillier, Stephen, Himmel, Alexander, Hoff, James, Hohl, Christian, Holin, Anna, Hoppe, Eric, Horton-Smith, Glenn, Hostert, Matheus, Hourlier, Adrien, Howard, Bruce, Howell, Ryan, Hugon, Justin, Iles, Gregory, Illingworth, Robert, Ioannisian, Ara, Itay, Ran, Izmaylov, Alexander, James, Eric, Jargowsky, B., Jediny, Filip, Jesús-Valls, César, Ji, Xiangpan, Jiang, L., Jiménez, Sergio, Jipa, Alexandru, Johnson, Connor, Johnson, Randy, Jones, Benjamin, Jones, Sebastian, Jung, Chang Kee, Junk, Thomas, Jwa, Yeon-jae, Kabirnezhad, Monireh, Kaboth, Asher, Kadenko, I, Kamiya, Felipe, Karagiorgi, Georgia, Karcher, A., Karolak, Mark, Karyotakis, Yannis, Kasai, Seiji, Kasetti, Siva, Kashur, Lane, Kazaryan, Narine, Kearns, Edward, Keener, Paul, Kelly, Kevin, Kemp, Ernesto, Ketchum, Wes, Kettell, Steve H, Khabibullin, Marat, Khotjantsev, Alexei, Khvedelidze, Arsen, Kim, D., King, Bonnie, Kirby, Brian, Kirby, Mike, Klein, Joshua, Koehler, Kevin, Koerner, Lisa, Kohn, Sam, Koller, Patrick, Kordosky, Mike, Kosc, Thomas, Kose, Umut, Kostelecky, V Alan, Kothekar, Kunal, Krennrich, Frank, Kreslo, Igor, Kudenko, Yury, Kudryavtsev, Vitaly A, Kulagin, Sergey, Kumar, Jason, KUMAR, Rajeev, Kuruppu, Chatura, Kus, Vaclav, Kutter, Thomas, Lambert, A., Lande, Kenneth, Lane, Charles, Lang, Karol, Langford, Thomas, Lasorak, Pierre, Last, David, Lastoria, Chiara, Laundrie, Andy, Lawrence, A., Lazanu, Ionel, LaZur, Ryan, Le, Trung, Learned, John, LeBrun, Patrice, Lehmann Miotto, Giovanna, Lehnert, Ralf, Leitner, M., Leyton, Michael, Li, Lingge, Li, Teng, Li, Yichen, Liao, Heng-Ye, Lin, Cheng-Ju Stephen, Lin, Shih-Kai, Lister, Adam, Littlejohn, Bryce, Liu, J., Lockwitz, Sarah, Loew, Timothy, Lokajicek, Milos, Lomidze, Irakli, Long, Ken, Loo, Kai, Lorca, David, Lord, Tom, LoSecco, John M, Louis, William, Luk, Kam-Biu, Luo, Xiao, Lurkin, Nicolas, Lux, Thorsten, Luzio, Vitor Prestes, MacFarlane, David, Machado, Ana Amelia, Machado, Pedro, Macias, Christopher Thomas, Macier, Jolie R, Maddalena, Antonello, Madigan, Peter, Magill, Steve, Mahn, Kendall, Maio, Amélia, Maloney, James, Mandrioli, Gianni, Maneira, José, Manenti, Laura, Manly, Steve, Mann, Anthony, Manolopoulos, Konstantinos, Manrique Plata, Maria, Marchionni, Alberto, Marciano, William, Marfatia, Danny, Mariani, Camillo, Maricic, Jelena, Marinho, Franciole, Marino, Alysia, Marshak, Marvin, Marshall, Chris, Marshall, John, Marteau, Jacques, Martin-Albo, Justo, Martinez, Norman, Martinez Caicedo, David, Martynenko, Sergey, Mason, Katie, Mastbaum, Andrew, Masud, Mehedi, Matsuno, Shigenobu, Matthews, James, Mauger, Christopher, Mauri, Nicoletta, Mavrokoridis, Konstantinos, Mazza, Roberto, Mazzacane, Anna, Mazzucato, Edoardo, McCluskey, Elaine, McConkey, Nicola, McFarland, Kevin, McGrew, Clark, McNab, Andrew, Mefodiev, Alexander, Mehta, Poonam, Melas, Pantelis, Mellinato, Michele, Mena, Olga, Menary, Scott, Mendes Santos, Lucas, Mendez, Hector, Menegolli, A, Meng, Guang, Messier, Mark, Metcalf, William, Mewes, Matthew, Meyer, Holger, Miao, Ting, Michna, Gregory, Miedema, Thijs, Migenda, Jost, Milincic, Radovan, Miller, William, Mills, Joshua, Milne, Cody, Mineev, Oleg, Miranda, Omar, Miryala, Sandeep, Mishra, C Shekhar, Mishra, Sanjib R, Mislivec, Aaron, Mladenov, Dimitar, Mocioiu, Irina, Moffat, Kristian, Moggi, Niccolo, Mohanta, Rukmani, Mohayai, Tanaz, Mokhov, Nikolai, Molina, Jorge, Molina Bueno, Laura, Montanari, Alessandro, Montanari, Claudio, Montanari, David, Montano Zetina, Luis, Moon, Jarrett, Mooney, Michael, Moreno, Deywis, Morgan, Ben, Morris, Casandra, Mossey, Chris, Motuk, Erdem, Moura, Célio, Mousseau, Joel, Mu, Wei, Mualem, Leon, Mueller, Justin, Muether, Mathew, Mufson, Stuart, Muheim, Franz, Muir, Alan, Mulhearn, Mike, Muramatsu, Hajime, Murphy, Sebastien, Musser, Jim, Nachtman, Jane, Nagu, S., Nalbandyan, Mikayel, Nandakumar, Raja, Naples, Donna, Narita, Shinya, Navas-Nicolas, D., Nayak, Nitish, Nebot-Guinot, Miquel, Necib, Lina, Negishi, Kentaro, Nelson, Jeff, Nesbit, Jake, Nessi, Marzio, Newbold, David, Newcomer, Mitch, Newhart, Duane, Nichol, Ryan, Niner, Evan, Nishimura, Kurtis, Norman, Andrew, Northrop, Rich, Novella, Pau, Nowak, Jaroslaw, Oberling, Michael, Olivares Del Campo, Andres, Olivier, Andrew, Onel, Yasar, Onishchuk, Yuriy, Ott, Jordan, Pagani, Luca, Pakvasa, Sandip, Palamara, Ornella, Palestini, Sandro, Paley, Jonathan, Pallavicini, Marco, Palomares, Carmen, Pantic, Emilija, Paolone, Vittorio, Papadimitriou, Vaia, Papaleo, Riccardo, Papanestis, Antonis, Paramesvaran, Sudarshan, Parke, Stephen, Parsa, Zohreh, Parvu, Mihaela, Pascoli, Silvia, Pasqualini, Laura, Pasternak, Jaroslaw, Pater, Joleen, Patrick, Cheryl, Patrizii, Laura, Patterson, Ryan, Patton, Simon John, Patzak, Thomas, Paudel, Ajib, Paulos, Bob, Paulucci, Laura, Pavlovic, Zarko, Pawloski, Greg, Payne, David, Pec, Viktor, Peeters, Simon, Penichot, Yves, Pennacchio, Elisabetta, Penzo, Aldo, Peres, Orlando, Perry, James, Pershey, Daniel, Pessina, Gianluigi, Petrillo, Gianluca, Petta, Catia, Petti, Roberto, Piastra, Francesco, Pickering, Luke, Pietropaolo, Francesco, Pillow, James, Plunkett, Robert, Poling, Ronald, Pons, Xavier, Poonthottathil, Navaneeth, Pordes, Stephen, Potekhin, Maxim, Potenza, Renato, Potukuchi, B.V.K.S., Pozimski, Juergen, Pozzato, Michele, Prakash, Suprabh, Prakash, Tarun, Prince, Sebastien, Pugnere, Denis, Qi, K., Qian, Xin, Raaf, Jennifer L, Raboanary, R., Radeka, Veljko, Rademacker, Jonas, Radics, Balint, Rafique, Aleena, Raguzin, Eric, Rai, Mousam, Rajaoalisoa, Miriama, Rakhno, Igor, Rakotondramanana, H.T., Rakotondravohitra, Laza, Ramachers, Yorck A, Rameika, Regina, Ramson, Bryan, Rappoldi, A, Raselli, GL, Ratoff, Peter, Ravat, Sylvain, Razafinime, H., Real, Jean-Sebastien, Rebel, Brian, Redondo, David, Reggiani-Guzzo, Marina, Rehak, Tyler, Reichenbacher, Juergen, Reitzner, S, Renshaw, Andrew, Rescia, Sergio, Resnati, Filippo, Reynolds, Aidan, Riccobene, Giorgio, Rice, Logan, Rielage, Keith, Rigaut, Yann-Axel, Rivera, David, Rochester, Leon, Roda, Marco, Rodrigues, Philip, Rodriguez Alonso, Manual Jesus, Rodriguez Rondon, Jairo, Roeth, Alison J, Rogers, Hannah, Rosauro-Alcaraz, Salvador, Rossella, M, Rout, Jogesh, Roy, Samiran, Rubbia, Andre, Rubbia, Carlo, Russell, Brooke, Russell, James, Ruterbories, Daniel, Saakyan, Ruben, Sacerdoti, Sabrina, Safford, Twymun, Sahu, Narendra, Sala, Paola, Samios, Nicholas, Sanchez, Mayly, Sanders, David, Sankey, David, Santana, Samuel, Santos-Maldonado, Marvin, Saoulidou, Niki, Sapienza, Piera, Sarasty, Carlos, Sarcevic, Ina, Savage, Geoffrey, Savinov, Vladimir, Scaramelli, Alberto, Scarff, Andrew, Scarpelli, Andrea, Schaffer, Tom, Schellman, Heidi, Schlabach, Philip, Schmitz, David, Scholberg, Kate, Schukraft, Anne, Segreto, Ettore, Sensenig, Jon, Seong, Ilsoo, Sergi, Antonino, Sergiampietri, F., Sgalaberna, Davide, Shaevitz, Michael H, Shafaq, Sheeba, Shamma, M., Sharma, Hans, Sharma, Rahul, Shaw, Terri, Shepherd-Themistocleous, Claire, Shin, Seodong, Shooltz, Dean, Shrock, Robert, Simard, Laurent, Simos, Nikolaos, Sinclair, James, Sinev, Gleb, Sipos, Roland, Sippach, F W, Sirri, Gabriele, Sitraka, Andriaseta, Siyeon, Kim, Smargianaki, D., Smith, Erica, Smith, Paul, Smolik, Jan, Smy, Michael, Snopok, Pavel, Soares Nunes, Mônica, Sobel, Henry, Soderberg, Mitch, Solano Salinas, Carlos, Söldner-Rembold, Stefan, Solomey, Nicholas, Solovov, Vladimir, Sondheim, Walter, Sorel, Michel, Soto-Oton, Jose, Sousa, Alexandre, Soustruznik, Karel, Spagliardi, Fabio, Spanu, Maura, Spitz, Joshua, Spooner, Neil JC, Spurgeon, Kyle, Staley, Richard, Stancari, Michelle, Stanco, Luca, Steiner, Herbert M, Stewart, James, Stillwell, Ben, Stock, Jason, Stocker, Francesca, Stokes, Tyler, Strait, Matthew, Strauss, Thomas, Striganov, Sergei, Stuart, Alexander, Summers, Don, Surdo, Antonio, Susic, Vasja, Suter, Louise, Sutera, Concetta Maria, Svoboda, Robert, Szczerbinska, Barbara, Szelc, Andrzej, Talaga, Richard, Tanaka, Hirohisa, Tapia Oregui, Beatriz, Tapper, Alexander, Tariq, Salman, Tatar, E., Tayloe, Rex, Teklu, Abraham Meles, Tenti, Matteo, Terao, Kazuhiro, Ternes, Christoph, Terranova, Francesco, Testera, Gemma, Thea, Alessandro, Thompson, Joshua, Thorn, Craig, Timm, Steven C, Tonazzo, Alessandra, Torti, Marta, Tortola, Mariam, Tortorici, Francesco, Totani, Dante, Toups, Matthew, Touramanis, Christos, Trevor, Jason, Trzaska, Wladyslaw, Tsai, Yun-Tse, Tsamalaidze, Zviadi, Tsang, Ka Vang, Tsverava, Nikolozi, Tufanli, Serhan, Tull, Craig, Tyley, E., Tzanov, Martin, Uchida, Melissa, Urheim, Jon, Usher, Tracy, Vagins, Mark R, Vahle, Patricia, Valdiviesso, Gustavo, Valencia, E., Vallari, Zoya, Valle, Jose, Vallecorsa, Sofia, Van Berg, Rick, Van de Water, Richard, Vanegas Forero, David, Varanini, Filippo, Vargas, Danaisis, Varner, Gary, Vasel, Justin, Vasseur, Georges, Vaziri, Kamran, Ventura, Sandro, Verdugo, Antonio, Vergani, Stefano, Vermeulen, Milo, Verzocchi, Marco, Vieira de Souza, Henrique, Vignoli, Chiara, Vilela, Cristovao, Viren, Brett, Vrba, Tomas, Wachala, Tomasz, Waldron, Abigail, Wallbank, Michael, Wang, Hanguo, Wang, Jingbo, Wang, Yi, Wang, Yue, Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, Yang, Shaokai, Zeller, Geralyn (Sam), While, M.R., White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Kevin, Wood, Lynn, Worcester, Elizabeth, Worcester, Matthew, Wret, Clarence, Wu, Wanwei, Xiao, Y., Yang, Guang, Yang, Tingjun, Yershov, Nikolai, Yonehara, Katsuya, Young, Tim, Yu, Bo, Yu, Jae, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeller, G.P., Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zimmerman, Eric, Zito, Marco, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
detector: technology ,Physics - Instrumentation and Detectors ,hep-ex ,Physics::Instrumentation and Detectors ,far detector ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,time projection chamber: liquid argon ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,neutrino: deep underground detector ,near detector ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,High Energy Physics::Experiment ,data management ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,activity report ,detector: design - Abstract
The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay -- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. This TDR is intended to justify the technical choices for the far detector that flow down from the high-level physics goals through requirements at all levels of the Project. Volume I contains an executive summary that introduces the DUNE science program, the far detector and the strategy for its modular designs, and the organization and management of the Project. The remainder of Volume I provides more detail on the science program that drives the choice of detector technologies and on the technologies themselves. It also introduces the designs for the DUNE near detector and the DUNE computing model, for which DUNE is planning design reports. Volume II of this TDR describes DUNE's physics program in detail. Volume III describes the technical coordination required for the far detector design, construction, installation, and integration, and its organizational structure. Volume IV describes the single-phase far detector technology. A planned Volume V will describe the dual-phase technology., Comment: Minor corrections made for JINST submission; 244 pages, 114 figures
- Published
- 2020
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96. Deep Underground Neutrino Experiment (DUNE), Far Detector Technical Design Report, Volume III: DUNE Far Detector Technical Coordination
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A, Raselli, GL, Ratoff, Peter, Ravat, Sylvain, Razafinime, H., Real, Jean-Sebastien, Rebel, Brian, Redondo, David, Reggiani-Guzzo, Marina, Rehak, Tyler, Reichenbacher, Juergen, Reitzner, S, Renshaw, Andrew, Rescia, Sergio, Resnati, Filippo, Reynolds, Aidan, Riccobene, Giorgio, Rice, Logan, Rielage, Keith, Rigaut, Yann-Axel, Rivera, David, Rochester, Leon, Roda, Marco, Rodrigues, Philip, Rodriguez Alonso, Manual Jesus, Rodriguez Rondon, Jairo, Roeth, Alison J, Rogers, Hannah, Rosauro-Alcaraz, Salvador, Rossella, M, Rout, Jogesh, Roy, Samiran, Rubbia, Andre, Rubbia, Carlo, Russell, Brooke, Russell, James, Ruterbories, Daniel, Saakyan, Ruben, Sacerdoti, Sabrina, Safford, Twymun, Sahu, Narendra, Sala, Paola, Samios, Nicholas, Sanchez, Mayly, Sanders, David, Sankey, David, Santana, Samuel, Santos-Maldonado, Marvin, Saoulidou, Niki, Sapienza, Piera, Sarasty, Carlos, Sarcevic, Ina, Savage, Geoffrey, Savinov, Vladimir, Scaramelli, Alberto, Scarff, Andrew, Scarpelli, Andrea, Schaffer, Tom, Schellman, Heidi, Schlabach, Philip, Schmitz, David, Scholberg, Kate, Schukraft, Anne, Segreto, Ettore, Sensenig, Jon, Seong, Ilsoo, Sergi, Antonino, Sergiampietri, F., Sgalaberna, Davide, Shaevitz, Michael H, Shafaq, Sheeba, Shamma, M., Sharma, Hans, Sharma, Rahul, Shaw, Terri, Shepherd-Themistocleous, Claire, Shin, Seodong, Shooltz, Dean, Shrock, Robert, Simard, Laurent, Simos, Nikolaos, Sinclair, James, Sinev, Gleb, Sipos, Roland, Sippach, F W, Sirri, Gabriele, Sitraka, Andriaseta, Siyeon, Kim, Smargianaki, D., Smith, Erica, Smith, Paul, Smolik, Jan, Smy, Michael, Snopok, Pavel, Soares Nunes, Mônica, Sobel, Henry, Soderberg, Mitch, Solano Salinas, Carlos, Söldner-Rembold, Stefan, Solomey, Nicholas, Solovov, Vladimir, Sondheim, Walter, Sorel, Michel, Soto-Oton, Jose, Sousa, Alexandre, Soustruznik, Karel, Spagliardi, Fabio, Spanu, Maura, Spitz, Joshua, Spooner, Neil JC, Spurgeon, Kyle, Staley, Richard, Stancari, Michelle, Stanco, Luca, Steiner, Herbert M, Stewart, James, Stillwell, Ben, Stock, Jason, Stocker, Francesca, Stokes, Tyler, Strait, Matthew, Strauss, Thomas, Striganov, Sergei, Stuart, Alexander, Summers, Don, Surdo, Antonio, Susic, Vasja, Suter, Louise, Sutera, Concetta Maria, Svoboda, Robert, Szczerbinska, Barbara, Szelc, Andrzej, Talaga, Richard, Tanaka, Hirohisa, Tapia Oregui, Beatriz, Tapper, Alexander, Tariq, Salman, Tatar, E., Tayloe, Rex, Teklu, Abraham Meles, Tenti, Matteo, Terao, Kazuhiro, Ternes, Christoph, Terranova, Francesco, Testera, Gemma, Thea, Alessandro, Thompson, Joshua, Thorn, Craig, Timm, Steven C, Tonazzo, Alessandra, Torti, Marta, Tortola, Mariam, Tortorici, Francesco, Totani, Dante, Toups, Matthew, Touramanis, Christos, Trevor, Jason, Trzaska, Wladyslaw, Tsai, Yun-Tse, Tsamalaidze, Zviadi, Tsang, Ka Vang, Tsverava, Nikolozi, Tufanli, Serhan, Tull, Craig, Tyley, E., Tzanov, Martin, Uchida, Melissa, Urheim, Jon, Usher, Tracy, Vagins, Mark R, Vahle, Patricia, Valdiviesso, Gustavo, Valencia, E., Vallari, Zoya, Valle, Jose, Vallecorsa, Sofia, Van Berg, Rick, Van de Water, Richard, Vanegas Forero, David, Varanini, Filippo, Vargas, Danaisis, Varner, Gary, Vasel, Justin, Vasseur, Georges, Vaziri, Kamran, Ventura, Sandro, Verdugo, Antonio, Vergani, Stefano, Vermeulen, Milo, Verzocchi, Marco, Vieira de Souza, Henrique, Vignoli, Chiara, Vilela, Cristovao, Viren, Brett, Vrba, Tomas, Wachala, Tomasz, Waldron, Abigail, Wallbank, Michael, Wang, Hanguo, Wang, Jingbo, Wang, Yi, Wang, Yue, Warburton, Karl, Warner, David, Wascko, Morgan, Waters, David, Watson, Alan, Weatherly, Pierce, Weber, Alfons, Weber, Michele, Wei, Hanyu, Weinstein, Amanda, Wenman, Dan, Wetstein, Matthew, Yang, Shaokai, Zeller, Geralyn (Sam), While, M.R., White, Andy, Whitehead, Leigh, Whittington, Denver, Wilking, Michael, Wilkinson, Callum, Williams, Zachary, Wilson, Fergus, Wilson, Robert, Wolcott, Jeremy, Wongjirad, Taritree, Wood, Kevin, Wood, Lynn, Worcester, Elizabeth, Worcester, Matthew, Wret, Clarence, Wu, Wanwei, Xiao, Y., Yang, Guang, Yang, Tingjun, Yershov, Nikolai, Yonehara, Katsuya, Young, Tim, Yu, Bo, Yu, Jae, Zalesak, Jaroslav, Zambelli, Laura, Zamorano, Bruno, Zani, Andrea, Zazueta, Luis, Zeller, G.P., Zennamo, Joseph, Zeug, Kyle, Zhang, Chao, Zhao, Manhong, Zhivun, Elena, Zhu, Guanying, Zimmerman, Eric, Zito, Marco, Zucchelli, Stefano, Zuklin, Josef, Zutshi, Vishnu, Zwaska, Robert, Institut de Physique des 2 Infinis de Lyon (IP2I Lyon), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Recherches sur les lois Fondamentales de l'Univers (IRFU), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris-Saclay, Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire d'Annecy de Physique des Particules (LAPP), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Savoie Mont Blanc (USMB [Université de Savoie] [Université de Chambéry])-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), DUNE, Université Claude Bernard Lyon 1 (UCBL), Université de Lyon-Université de Lyon-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), and Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)
- Subjects
safety ,Neutrino Oscillations. Neutrino detectors ,Physics - Instrumentation and Detectors ,hep-ex ,Physics::Instrumentation and Detectors ,engineering ,far detector ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,fabrication ,time projection chamber: liquid argon ,High Energy Physics - Experiment ,High Energy Physics - Experiment (hep-ex) ,neutrino: deep underground detector ,quality ,[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex] ,High Energy Physics::Experiment ,[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det] ,Detectors and Experimental Techniques ,physics.ins-det ,Particle Physics - Experiment ,activity report - Abstract
The preponderance of matter over antimatter in the early universe, the dynamics of the supernovae that produced the heavy elements necessary for life, and whether protons eventually decay -- these mysteries at the forefront of particle physics and astrophysics are key to understanding the early evolution of our universe, its current state, and its eventual fate. The Deep Underground Neutrino Experiment (DUNE) is an international world-class experiment dedicated to addressing these questions as it searches for leptonic charge-parity symmetry violation, stands ready to capture supernova neutrino bursts, and seeks to observe nucleon decay as a signature of a grand unified theory underlying the standard model. The DUNE far detector technical design report (TDR) describes the DUNE physics program and the technical designs of the single- and dual-phase DUNE liquid argon TPC far detector modules. Volume III of this TDR describes how the activities required to design, construct, fabricate, install, and commission the DUNE far detector modules are organized and managed. This volume details the organizational structures that will carry out and/or oversee the planned far detector activities safely, successfully, on time, and on budget. It presents overviews of the facilities, supporting infrastructure, and detectors for context, and it outlines the project-related functions and methodologies used by the DUNE technical coordination organization, focusing on the areas of integration engineering, technical reviews, quality assurance and control, and safety oversight. Because of its more advanced stage of development, functional examples presented in this volume focus primarily on the single-phase (SP) detector module., Minor corrections made for JINST submission, 209 pages, 55 figures (updated typos in Table A.5; corrected errors in author list)
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- 2020
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97. AEDGE:Atomic Experiment for Dark Matter and Gravity Exploration in Space
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El-Neaj, Yousef Abou, Alpigiani, Cristiano, Amairi-Pyka, Sana, Araujo, Henrique, Balaz, Antun, Belic, Aleksandar, Bentine, Elliot, Bernabeu, Jose, Bingham, Robert, Bolpasi, Vasiliki, Bowden, William, Buchmueller, Oliver, Burrage, Clare, Calmet, Xavier, Canuel, Benjamin, Charmandaris, Vassilis, Chen, Xuzong, Coleman, Jonathon, Cotter, Joseph, Cui, Yanou, Derevianko, Andrei, De Roeck, Albert, Drougkakis, Ioannis, Dutan, Ioana, Elertas, Gedminas, Ellis, John, El Sawy, Mai, Fassi, Farida, Felea, Daniel, Feng, Chen-Hao, Flack, Robert, Foot, Chris, Fuentes, Ivette, Gaaloul, Naceur, Gauguet, Alexandre, Geiger, Remi, Gibson, Valerie, Giudice, Gian, Goldwin, Jon, Grachov, Oleg, Graham, Peter W., Grasso, Dario, Van der Grinten, Maurits, Guendogan, Mustafa, Haehnelt, Martin G., Harte, Tiffany, Hees, Aurelien, Hobson, Richard, Hogan, Jason, Holst, Bodil, Holynski, Michael, Kasevich, Mark, Kavanagh, Bradley J., Von Klitzing, Wolf, Kovachy, Tim, Krikler, Benjamin, Krutzik, Markus, Lewicki, Marek, Lien, Yu-Hung, Liu, Miaoyuan, Luciano, Giuseppe Gaetano, Pandey, Saurabh, Paternostro, Mauro, Penning, Bjoern, Peters, Achim, Prevedelli, Marco, Puthiya-Veettil, Vishnupriya, Quenby, John, Rasel, Ernst, Roura, Albert, Sabulsky, Dylan, Sameed, Muhammed, Sauer, Ben, Schaffer, Stefan Alaric, Schiller, Stephan, Schkolnik, Vladimir, Schlippert, Dennis, Schubert, Christian, Sfar, Haifa Rejeb, Shayeghi, Armin, Soares-Santos, Marcelle, Vasilakis, Georgios, Vaskonen, Ville, Vogt, Christian, Webber-Date, Alex, Windpassinger, Patrick, Woltmann, Marian, Yazgan, Efe, Zupan, Jure, El-Neaj, Yousef Abou, Alpigiani, Cristiano, Amairi-Pyka, Sana, Araujo, Henrique, Balaz, Antun, Belic, Aleksandar, Bentine, Elliot, Bernabeu, Jose, Bingham, Robert, Bolpasi, Vasiliki, Bowden, William, Buchmueller, Oliver, Burrage, Clare, Calmet, Xavier, Canuel, Benjamin, Charmandaris, Vassilis, Chen, Xuzong, Coleman, Jonathon, Cotter, Joseph, Cui, Yanou, Derevianko, Andrei, De Roeck, Albert, Drougkakis, Ioannis, Dutan, Ioana, Elertas, Gedminas, Ellis, John, El Sawy, Mai, Fassi, Farida, Felea, Daniel, Feng, Chen-Hao, Flack, Robert, Foot, Chris, Fuentes, Ivette, Gaaloul, Naceur, Gauguet, Alexandre, Geiger, Remi, Gibson, Valerie, Giudice, Gian, Goldwin, Jon, Grachov, Oleg, Graham, Peter W., Grasso, Dario, Van der Grinten, Maurits, Guendogan, Mustafa, Haehnelt, Martin G., Harte, Tiffany, Hees, Aurelien, Hobson, Richard, Hogan, Jason, Holst, Bodil, Holynski, Michael, Kasevich, Mark, Kavanagh, Bradley J., Von Klitzing, Wolf, Kovachy, Tim, Krikler, Benjamin, Krutzik, Markus, Lewicki, Marek, Lien, Yu-Hung, Liu, Miaoyuan, Luciano, Giuseppe Gaetano, Pandey, Saurabh, Paternostro, Mauro, Penning, Bjoern, Peters, Achim, Prevedelli, Marco, Puthiya-Veettil, Vishnupriya, Quenby, John, Rasel, Ernst, Roura, Albert, Sabulsky, Dylan, Sameed, Muhammed, Sauer, Ben, Schaffer, Stefan Alaric, Schiller, Stephan, Schkolnik, Vladimir, Schlippert, Dennis, Schubert, Christian, Sfar, Haifa Rejeb, Shayeghi, Armin, Soares-Santos, Marcelle, Vasilakis, Georgios, Vaskonen, Ville, Vogt, Christian, Webber-Date, Alex, Windpassinger, Patrick, Woltmann, Marian, Yazgan, Efe, and Zupan, Jure
- Abstract
We propose in this White Paper a concept for a space experiment using cold atoms to search for ultra-light dark matter, and to detect gravitational waves in the frequency range between the most sensitive ranges of LISA and the terrestrial LIGO/Virgo/KAGRA/INDIGO experiments. This interdisciplinary experiment, called Atomic Experiment for Dark Matter and Gravity Exploration (AEDGE), will also complement other planned searches for dark matter, and exploit synergies with other gravitational wave detectors. We give examples of the extended range of sensitivity to ultra-light dark matter offered by AEDGE, and how its gravitational-wave measurements could explore the assembly of super-massive black holes, first-order phase transitions in the early universe and cosmic strings. AEDGE will be based upon technologies now being developed for terrestrial experiments using cold atoms, and will benefit from the space experience obtained with, e.g., LISA and cold atom experiments in microgravity. KCL-PH-TH/2019-65, CERN-TH-2019-126
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- 2020
98. WIMP cogenesis for asymmetric dark matter and the baryon asymmetry
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Cui, Yanou, primary and Shamma, Michael, additional
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- 2020
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99. Gravitational Wave Bursts as Harbingers of Cosmic Strings Diluted by Inflation
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Cui, Yanou, primary, Lewicki, Marek, additional, and Morrissey, David E., additional
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- 2020
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100. Cosmic filaments from cosmic strings
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Fernandez, M. A., primary, Bird, Simeon, additional, and Cui, Yanou, additional
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- 2020
- Full Text
- View/download PDF
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