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Pérez de los Heros, CarlosORCID iD iconorcid.org/0000-0002-2084-5866
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Publikasjoner (10 av 291) Visa alla publikasjoner
Aartsen, M. G., Botner, O., Burgman, A., Hallgren, A., Pérez de los Heros, C., Unger, E. & Yermia, F. (2020). Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU. Physical Review D: covering particles, fields, gravitation, and cosmology, 101(3), Article ID 032006.
Åpne denne publikasjonen i ny fane eller vindu >>Combined sensitivity to the neutrino mass ordering with JUNO, the IceCube Upgrade, and PINGU
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2020 (engelsk)Inngår i: Physical Review D: covering particles, fields, gravitation, and cosmology, ISSN 2470-0010, E-ISSN 2470-0029, Vol. 101, nr 3, artikkel-id 032006Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The ordering of the neutrino mass eigenstates is one of the fundamental open questions in neutrino physics. While current-generation neutrino oscillation experiments are able to produce moderate indications on this ordering, upcoming experiments of the next generation aim to provide conclusive evidence. In this paper we study the combined performance of the two future multi-purpose neutrino oscillation experiments JUNO and the IceCube Upgrade, which employ two very distinct and complementary routes toward the neutrino mass ordering. The approach pursued by the 20 kt medium-baseline reactor neutrino experiment JUNO consists of a careful investigation of the energy spectrum of oscillated (nu) over bar (e) produced by ten nuclear reactor cores. The IceCube Upgrade, on the other hand, which consists of seven additional densely instrumented strings deployed in the center of IceCube DeepCore, will observe large numbers of atmospheric neutrinos that have undergone oscillations affected by Earth matter. In a joint fit with both approaches, tension occurs between their preferred mass-squared differences Delta m(31)(2) = m(3)(2) - m(1)(2) in within the wrong mass ordering. In the case of JUNO and the IceCube Upgrade, this allows to exclude the wrong ordering at > 5 sigma on a timescale of 3-7 years-even under circumstances that are unfavorable to the experiments individual sensitivities. For PINGU, a 26-string detector array designed as a potential low-energy extension to IceCube, the inverted ordering could be excluded within 1.5 years (3 years for the normal ordering) in a joint analysis.

sted, utgiver, år, opplag, sider
AMER PHYSICAL SOC, 2020
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-407651 (URN)10.1103/PhysRevD.101.032006 (DOI)000515060600001 ()
Forskningsfinansiär
Swedish Research CouncilKnut and Alice Wallenberg FoundationSwedish Polar Research Secretariat
Merknad

For complete list of authors see http://dx.doi.org/10.1103/PhysRevD.101.032006

Tilgjengelig fra: 2020-03-31 Laget: 2020-03-31 Sist oppdatert: 2020-03-31bibliografisk kontrollert
Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., . . . Yuan, T. (2020). Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data IceCube Collaboration. European Physical Journal C, 80(1), Article ID 9.
Åpne denne publikasjonen i ny fane eller vindu >>Development of an analysis to probe the neutrino mass ordering with atmospheric neutrinos using three years of IceCube DeepCore data IceCube Collaboration
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2020 (engelsk)Inngår i: European Physical Journal C, ISSN 1434-6044, E-ISSN 1434-6052, Vol. 80, nr 1, artikkel-id 9Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

The Neutrino Mass Ordering (NMO) remains one of the outstanding questions in the field of neutrino physics. One strategy to measure the NMO is to observe matter effects in the oscillation pattern of atmospheric neutrinos above similar to 1GeV, as proposed for several next-generation neutrino experiments. Moreover, the existing IceCube DeepCore detector can already explore this type of measurement. We present the development and application of two independent analyses to search for the signature of the NMO with three years of DeepCore data. These analyses include a full treatment of systematic uncertainties and a statistically-rigorous method to determine the significance for the NMO from a fit to the data. Both analyses show that the dataset is fully compatible with both mass orderings. For the more sensitive analysis, we observe a preference for normal ordering with a p-value of pIO=15.3% and CLs=53.3% for the inverted ordering hypothesis, while the experimental results from both analyses are consistent within their uncertainties. Since the result is independent of the value of delta CP and obtained from energies E nu greater than or similar to 5GeV, it is complementary to recent results from long-baseline experiments. These analyses set the groundwork for the future of this measurement with more capable detectors, such as the IceCube Upgrade and the proposed PINGU detector.

sted, utgiver, år, opplag, sider
SPRINGER, 2020
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-406913 (URN)10.1140/epjc/s10052-019-7555-0 (DOI)000511722800001 ()
Tilgjengelig fra: 2020-03-18 Laget: 2020-03-18 Sist oppdatert: 2020-03-18bibliografisk kontrollert
Colom i Bernadich, M. & Pérez de los Heros, C. (2020). Limits on Kaluza-Klein dark matter annihilation in the Sun from recent IceCube results. European Physical Journal C, 80(2), Article ID 129.
Åpne denne publikasjonen i ny fane eller vindu >>Limits on Kaluza-Klein dark matter annihilation in the Sun from recent IceCube results
2020 (engelsk)Inngår i: European Physical Journal C, ISSN 1434-6044, E-ISSN 1434-6052, Vol. 80, nr 2, artikkel-id 129Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We interpret recent IceCube results on searches for dark matter accumulated in the Sun in terms of the lightest Kaluza-Klein excitation (assumed here to be the Kaluza-Klein photon, B1), obtaining improved limits on the annihilation rate in the Sun, the resulting neutrino flux at the Earth and on the B1-proton cross-sections, for B1 masses in the range 30-3000 GeV. These results improve previous results from IceCube in its 22-string configuration by up to an order of magnitude, depending on mass, but also extend the results to B1masses as low as 30 GeV.

sted, utgiver, år, opplag, sider
SPRINGER, 2020
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-407355 (URN)10.1140/epjc/s10052-020-7708-1 (DOI)000515796800004 ()
Tilgjengelig fra: 2020-05-29 Laget: 2020-05-29 Sist oppdatert: 2020-05-29bibliografisk kontrollert
Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., . . . Yuan, T. (2020). Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data. Astroparticle physics, 116, Article ID 102392.
Åpne denne publikasjonen i ny fane eller vindu >>Neutrinos below 100 TeV from the southern sky employing refined veto techniques to IceCube data
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2020 (engelsk)Inngår i: Astroparticle physics, ISSN 0927-6505, E-ISSN 1873-2852, Vol. 116, artikkel-id 102392Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

Many Galactic sources of gamma rays, such as supernova remnants, are expected to produce neutrinos with a typical energy cutoff well below 100 TeV. For the IceCube Neutrino Observatory located at the South Pole, the southern sky, containing the inner part of the Galactic plane and the Galactic Center, is a particularly challenging region at these energies, because of the large background of atmospheric muons. In this paper, we present recent advancements in data selection strategies for track-like muon neutrino events with energies below 100 TeV from the southern sky. The strategies utilize the outer detector regions as veto and features of the signal pattern to reduce the background of atmospheric muons to a level which, for the first time, allows IceCube searching for point-like sources of neutrinos in the southern sky at energies between 100 GeV and several TeV in the muon neutrino charged current channel. No significant clustering of neutrinos above background expectation was observed in four years of data recorded with the completed IceCube detector. Upper limits on the neutrino flux for a number of spectral hypotheses are reported for a list of astrophysical objects in the southern hemisphere. 

sted, utgiver, år, opplag, sider
ELSEVIER, 2020
Emneord
Neutrinos, Point sources, Veto techniques
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-400830 (URN)10.1016/j.astropartphys.2019.102392 (DOI)000501416000004 ()
Forskningsfinansiär
Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationSwedish Polar Research Secretariat
Tilgjengelig fra: 2020-01-13 Laget: 2020-01-13 Sist oppdatert: 2020-01-13bibliografisk kontrollert
Aartsen, M. G., Botner, O., Burgman, A., Hallgren, A., Pérez de los Heros, C., Unger, E. & Zoecklein, M. (2020). Time-Integrated Neutrino Source Searches with 10 Years of IceCube Data. Physical Review Letters, 124(5), Article ID 051103.
Åpne denne publikasjonen i ny fane eller vindu >>Time-Integrated Neutrino Source Searches with 10 Years of IceCube Data
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2020 (engelsk)Inngår i: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 124, nr 5, artikkel-id 051103Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

This Letter presents the results from pointlike neutrino source searches using ten years of IceCube data collected between April 6, 2008 and July 10, 2018. We evaluate the significance of an astrophysical signal from a pointlike source looking for an excess of clustered neutrino events with energies typically above similar to 1 TeV among the background of atmospheric muons and neutrinos. We perform a full-sky scan, a search within a selected source catalog, a catalog population study, and three stacked Galactic catalog searches. The most significant point in the northern hemisphere from scanning the sky is coincident with the Seyfert II galaxy NGC 1068, which was included in the source catalog search. The excess at the coordinates of NGC 1068 is inconsistent with background expectations at the level of 2.9 sigma after accounting for statistical trials from the entire catalog. The combination of this result along with excesses observed at the coordinates of three other sources, including TXS 0506 + 056, suggests that, collectively, correlations with sources in the northern catalog are inconsistent with background at 3.3 sigma significance. The southern catalog is consistent with background. These results, all based on searches for a cumulative neutrino signal integrated over the 10 years of available data, motivate further study of these and similar sources, including time-dependent analyses, multimessenger correlations, and the possibility of stronger evidence with coming upgrades to the detector.

sted, utgiver, år, opplag, sider
AMER PHYSICAL SOC, 2020
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-406734 (URN)10.1103/PhysRevLett.124.051103 (DOI)000511450000004 ()32083934 (PubMedID)
Forskningsfinansiär
Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationSwedish Polar Research Secretariat
Merknad

For complete list of authors see http://dx.doi.org/10.1103/PhysRevLett.124.051103

Tilgjengelig fra: 2020-03-12 Laget: 2020-03-12 Sist oppdatert: 2020-03-12bibliografisk kontrollert
Betti, M. G., Biasotti, M., Bosca, A., Calle, F., Carabe-Lopez, J., Cavoto, G., . . . Zurek, K. M. (2019). A design for an electromagnetic filter for precision energy measurements at the tritium endpoint. Progress in Particle and Nuclear Physics, 106, 120-131
Åpne denne publikasjonen i ny fane eller vindu >>A design for an electromagnetic filter for precision energy measurements at the tritium endpoint
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2019 (engelsk)Inngår i: Progress in Particle and Nuclear Physics, ISSN 0146-6410, E-ISSN 1873-2224, Vol. 106, s. 120-131Artikkel, forskningsoversikt (Fagfellevurdert) Published
Abstract [en]

We present a detailed description of the electromagnetic filter for the PTOLEMY project to directly detect the Cosmic Neutrino Background (CNB). Starting with an initial estimate for the orbital magnetic moment, the higher-order drift process of E x B is configured to balance the gradient-B drift motion of the electron in such a way as to guide the trajectory into the standing voltage potential along the mid-plane of the filter. As a function of drift distance along the length of the filter, the filter zooms in with exponentially increasing precision on the transverse velocity component of the electron kinetic energy. This yields a linear dimension for the total filter length that is exceptionally compact compared to previous techniques for electromagnetic filtering. The parallel velocity component of the electron kinetic energy oscillates in an electrostatic harmonic trap as the electron drifts along the length of the filter. An analysis of the phase-space volume conservation validates the expected behavior of the filter from the adiabatic invariance of the orbital magnetic moment and energy conservation following Liouville's theorem for Hamiltonian systems. (C) 2019 Elsevier B.V. All rights reserved.

sted, utgiver, år, opplag, sider
ELSEVIER SCIENCE BV, 2019
Emneord
PTOLEMY, Relic neutrino, Cosmic Neutrino Background, CNB, Neutrino mass, Transverse drift filter
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-383047 (URN)10.1016/j.ppnp.2019.02.004 (DOI)000464490900003 ()
Tilgjengelig fra: 2019-05-13 Laget: 2019-05-13 Sist oppdatert: 2019-05-13bibliografisk kontrollert
Abeysekara, A. U., Botner, O., Burgman, A., Hallgren, A., Pérez de los Heros, C., Unger, E. & Yuan, T. (2019). All-sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field. Astrophysical Journal, 871(1), Article ID 96.
Åpne denne publikasjonen i ny fane eller vindu >>All-sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field
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2019 (engelsk)Inngår i: Astrophysical Journal, ISSN 0004-637X, E-ISSN 1538-4357, Vol. 871, nr 1, artikkel-id 96Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We present the first full-sky analysis of the cosmic ray arrival direction distribution with data collected by the High-Altitude Water Cherenkov and IceCube observatories in the northern and southern hemispheres at the same median primary particle energy of 10 TeV. The combined sky map and angular power spectrum largely eliminate biases that result from partial sky coverage and present a key to probe into the propagation properties of TeV cosmic rays through our local interstellar medium and the interaction between the interstellar and heliospheric magnetic fields. From the map, we determine the horizontal dipole components of the anisotropy delta(0h) = 9.16 x 10(-4) and delta(6h) = 7.25 x 10(-4) (+/- 0.04 x 10(-4)). In addition, we infer the direction (229 degrees.2 +/- 3 degrees.5 R.A., 11 degrees.4 +/- 3 degrees.0 decl.) of the interstellar magnetic field from the boundary between large-scale excess and deficit regions from which we estimate the missing corresponding vertical dipole component of the large-scale anisotropy to be delta(N) similar to -3.97(-2.0)(+1.0) x 10(-4).

Emneord
astroparticle physics, cosmic rays, ISM: magnetic fields
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-377359 (URN)10.3847/1538-4357/aaf5cc (DOI)000456837000045 ()
Forskningsfinansiär
German Research Foundation (DFG)Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationDanish National Research Foundation
Merknad

IceCube collaboration, for complete list of authors and funding information see http://dx.doi.org/10.3847/1538-4357/aaf5cc

Tilgjengelig fra: 2019-02-19 Laget: 2019-02-19 Sist oppdatert: 2019-05-21bibliografisk kontrollert
Backstrom, A., Catena, R. & Pérez de los Heros, C. (2019). Assessing the sensitivity of PINGU to effective dark matter-nucleon interactions. Journal of Cosmology and Astroparticle Physics (5), Article ID 023.
Åpne denne publikasjonen i ny fane eller vindu >>Assessing the sensitivity of PINGU to effective dark matter-nucleon interactions
2019 (engelsk)Inngår i: Journal of Cosmology and Astroparticle Physics, ISSN 1475-7516, E-ISSN 1475-7516, nr 5, artikkel-id 023Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We calculate the sensitivity of next generation neutrino telescopes to the 28 (isoscalar and isovector) coupling constants defining the non-relativistic effective theory of (spin 1/2) dark matter (DM)-nucleon interactions. We take as a benchmark detector the proposed Precision IceCube Next Generation Upgrade (PINGU), although our results are valid for any other neutrino telescope of similar effective volume. We express PINGU's sensitivity in terms of 5 sigma sensitivity contours in the DM mass-coupling constant plane, and compare our sensitivity contours with the 90% C.L. exclusion limits on the same coupling constants that we obtain from a reanalysis of the null result of current DM searches at IceCube/DeepCore. We find that PINGU can effectively probe not only the canonical spin-independent and spin-dependent DM-nucleon interactions, but also some of the velocity-dependent or momentum-dependent interactions that generate DM-nucleus scattering cross sections scaling like the number of nucleons squared. We also find that PINGU's 5 sigma sensitivity contours are significantly below current IceCube/DeepCore 90% C.L. exclusion limits when b (b) over bar is the leading DM annihilation channel. This result shows the importance of lowering the experimental energy threshold when probing models that generate soft neutrino energy spectra, and holds true independently of the assumed DM-nucleon interaction and for all DM masses tested here. When DM primarily annihilates into tau(tau) over bar, a PINGU-like detector will improve upon current exclusion limits for DM masses below 30 GeV, independently of the assumed DM-nucleon interaction.

Emneord
dark matter theory, dark matter experiments
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-387297 (URN)10.1088/1475-7516/2019/05/023 (DOI)000467933500003 ()
Forskningsfinansiär
Knut and Alice Wallenberg Foundation
Tilgjengelig fra: 2019-06-24 Laget: 2019-06-24 Sist oppdatert: 2019-06-24bibliografisk kontrollert
Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., . . . Yuan, T. (2019). Constraints on Minute-Scale Transient Astrophysical Neutrino Sources. Physical Review Letters, 122(5), Article ID 051102.
Åpne denne publikasjonen i ny fane eller vindu >>Constraints on Minute-Scale Transient Astrophysical Neutrino Sources
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2019 (engelsk)Inngår i: Physical Review Letters, ISSN 0031-9007, E-ISSN 1079-7114, Vol. 122, nr 5, artikkel-id 051102Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

High-energy neutrino emission has been predicted for several short-lived astrophysical transients including gamma-ray bursts (GRBs), core-collapse supernovae with choked jets, and neutron star mergers. IceCube's optical and x-ray follow-up program searches for such transient sources by looking for two or more muon neutrino candidates in directional coincidence and arriving within 100 s. The measured rate of neutrino alerts is consistent with the expected rate of chance coincidences of atmospheric background events and no likely electromagnetic counterparts have been identified in Swift follow-up observations. Here, we calculate generic bounds on the neutrino flux of short-lived transient sources. Assuming an E-2.5 neutrino spectrum, we find that the neutrino flux of rare sources, like long gamma-ray bursts, is constrained to < 5% of the detected astrophysical flux and the energy released in neutrinos (100 GeV to 10 PeV) by a median bright GRB-like source is < 10(52.5) erg. For a harder E-2.13 neutrino spectrum up to 30% of the flux could be produced by GRBs and the allowed median source energy is < 10(52) erg. A hypothetical population of transient sources has to be more common than 10(-5) Mpc(-3) yr(-1) (5 x 10(-8) Mpc(-3) yr(-1) for the E-2.13 spectrum) to account for the complete astrophysical neutrino flux.

sted, utgiver, år, opplag, sider
AMER PHYSICAL SOC, 2019
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-378535 (URN)10.1103/PhysRevLett.122.051102 (DOI)000458147300005 ()
Forskningsfinansiär
German Research Foundation (DFG)Swedish Research CouncilSwedish National Infrastructure for Computing (SNIC)Knut and Alice Wallenberg FoundationAustralian Research Council
Tilgjengelig fra: 2019-03-22 Laget: 2019-03-22 Sist oppdatert: 2019-05-21bibliografisk kontrollert
Aartsen, M. G., Ackermann, M., Adams, J., Aguilar, J. A., Ahlers, M., Ahrens, M., . . . Zoecklein, M. (2019). Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube. Physical Review D: covering particles, fields, gravitation, and cosmology, 100(8), Article ID 082002.
Åpne denne publikasjonen i ny fane eller vindu >>Cosmic ray spectrum and composition from PeV to EeV using 3 years of data from IceTop and IceCube
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2019 (engelsk)Inngår i: Physical Review D: covering particles, fields, gravitation, and cosmology, ISSN 2470-0010, E-ISSN 2470-0029, Vol. 100, nr 8, artikkel-id 082002Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We report on measurements of the all-particle cosmic ray energy spectrum and composition in the PeV to EeV energy range using 3 years of data from the IceCube Neutrino Observatory. The IceTop detector measures cosmic ray induced air showers on the surface of the ice, from which the energy spectrum of cosmic rays is determined by making additional assumptions about the mass composition. A separate measurement is performed when IceTop data are analyzed in coincidence with the high-energy muon energy loss information from the deep in-ice IceCube detector. In this measurement, both the spectrum and the mass composition of the primary cosmic rays are simultaneously reconstructed using a neural network trained on observables from both detectors. The performance and relative advantages of these two distinct analyses are discussed, including the systematic uncertainties and the dependence on the hadronic interaction models, and both all-particle spectra as well as individual spectra for elemental groups are presented.

sted, utgiver, år, opplag, sider
AMER PHYSICAL SOC, 2019
HSV kategori
Identifikatorer
urn:nbn:se:uu:diva-397044 (URN)10.1103/PhysRevD.100.082002 (DOI)000491993600001 ()
Tilgjengelig fra: 2019-11-19 Laget: 2019-11-19 Sist oppdatert: 2019-11-19bibliografisk kontrollert
Organisasjoner
Identifikatorer
ORCID-id: ORCID iD iconorcid.org/0000-0002-2084-5866