Search NASA⌕ Search

DOE OSTI · 2498352

Probing the Connection between IceCube Neutrinos and MOJAVE AGN

Abbasi, R.·Ackermann, M. (ORCID:000000018952588X)·Adams, J.·Agarwalla, S. K. (ORCID:0000000297148866)·Aguilar, J. A. (ORCID:0000000322529514)·Ahlers, M. (ORCID:0000000307095631)·Alameddine, J. M. (ORCID:0000000295349189)·Amin, N. M.·Andeen, K. (ORCID:0000000193940007)·Argüelles, C. (ORCID:0000000341864182)·Ashida, Y.·Athanasiadou, S.·Ausborm, L.·Axani, S. N. (ORCID:0000000188663826)·Bai, X. (ORCID:0000000218279121)·Balagopal V., A. (ORCID:0000000153678876)·Baricevic, M.·Barwick, S. W. (ORCID:0000000320506714)·Bash, S.·Basu, V. (ORCID:0000000295282009)·Bay, R.·Beatty, J. J. (ORCID:0000000304814952)·Becker Tjus, J. (ORCID:0000000217487367)·Beise, J. (ORCID:0000000274484189)·Bellenghi, C. (ORCID:0000000185257515)·Benning, C.·BenZvi, S. (ORCID:0000000155374710)·Berley, D.·Bernardini, E. (ORCID:0000000331081141)·Besson, D. Z. (ORCID:000000016733963X)·Blaufuss, E. (ORCID:0000000154501757)·Bloom, L. (ORCID:0009000599383164)·Blot, S. (ORCID:0000000310893001)·Bontempo, F.·Book Motzkin, J. Y. (ORCID:0000000166875959)·Boscolo Meneguolo, C. (ORCID:0000000183254329)·Böser, S. (ORCID:0000000259184890)·Botner, O. (ORCID:0000000185887306)·Böttcher, J. (ORCID:0000000233874236)·Braun, J.·Brinson, B. (ORCID:0000000191281159)·Brostean-Kaiser, J.·Brusa, L.·Burley, R. T.·Butterfield, D.·Campana, M. A. (ORCID:0000000341625739)·Caracas, I.·Carloni, K.·Carpio, J. (ORCID:0000000306676557)·Chattopadhyay, S.·Chau, N.·Chen, Z. (ORCID:0000000228137688)·Chirkin, D. (ORCID:0000000349111345)·Choi, S.·Clark, B. A. (ORCID:0000000340892245)·Coleman, A. (ORCID:0000000315101712)·Collin, G. H.·Connolly, A.·Conrad, J. M. (ORCID:0000000263930438)·Corley, R.·Cowen, D. F. (ORCID:0000000347380787)·Dave, P. (ORCID:0000000238795115)·De Clercq, C. (ORCID:0000000152667059)·DeLaunay, J. J. (ORCID:0000000152291995)·Delgado, D. (ORCID:0000000243068828)·Deng, S.·Desai, A. (ORCID:0000000174059994)·Desiati, P. (ORCID:0000000197681858)·de Vries, K. D. (ORCID:0000000298424068)·de Wasseige, G. (ORCID:0000000210105100)·DeYoung, T. (ORCID:0000000348733783)·Diaz, A. (ORCID:0000000172068336)·Díaz-Vélez, J. C. (ORCID:0000000200870693)·Dierichs, P.·Dittmer, M.·Domi, A.·Draper, L.·Dujmovic, H. (ORCID:0000000318910718)·Durnford, D. (ORCID:0000000266087650)·Dutta, K.·DuVernois, M. A. (ORCID:0000000229879691)·Ehrhardt, T.·Eidenschink, L.·Eimer, A.·Eller, P. (ORCID:0000000163545209)·Ellinger, E.·El Mentawi, S.·Elsässer, D. (ORCID:0000000167963205)·Engel, R.·Erpenbeck, H. (ORCID:0000000163192108)·Evans, J.·Evenson, P. A. (ORCID:000000017929810X)·Fan, K. L. (ORCID:0000000282464751)·Fang, K.·Farrag, K.·Fazely, A. R. (ORCID:0000000269078020)·Fedynitch, A. (ORCID:0000000328373477)·Feigl, N.·Fiedlschuster, S.·Finley, C. (ORCID:000000033350390X)

Abstract

Active galactic nuclei (AGN) are prime candidate sources of the high-energy, astrophysical neutrinos detected by IceCube. This is demonstrated by the real-time multimessenger detection of the blazar TXS 0506+056 and the recent evidence of neutrino emission from NGC 1068 from a separate time-averaged study. However, the production mechanism of the astrophysical neutrinos in AGN is not well established, which can be resolved via correlation studies with photon observations. For neutrinos produced due to photohadronic interactions in AGN, in addition to a correlation of neutrinos with high-energy photons, there would also be a correlation of neutrinos with photons emitted at radio wavelengths. In this work, we perform an in-depth stacking study of the correlation between 15 GHz radio observations of AGN reported in the MOJAVE XV catalog, and 10 yr of neutrino data from IceCube. We also use a time-dependent approach, which improves the statistical power of the stacking analysis. No significant correlation was found for both analyses, and upper limits are reported. When compared to the IceCube diffuse flux, at 100 TeV and for a spectral index of 2.5, the upper limits derived are ~3% and ~9% for the time-averaged and time-dependent cases, respectively.

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Abbasi, R., Ackermann, M. (ORCID:000000018952588X), Adams, J., Agarwalla, S. K. (ORCID:0000000297148866), Aguilar, J. A. (ORCID:0000000322529514), Ahlers, M. (ORCID:0000000307095631), Alameddine, J. M. (ORCID:0000000295349189), Amin, N. M., Andeen, K. (ORCID:0000000193940007), Argüelles, C. (ORCID:0000000341864182), Ashida, Y., Athanasiadou, S., Ausborm, L., Axani, S. N. (ORCID:0000000188663826), Bai, X. (ORCID:0000000218279121), Balagopal V., A. (ORCID:0000000153678876), Baricevic, M., Barwick, S. W. (ORCID:0000000320506714), Bash, S., Basu, V. (ORCID:0000000295282009), Bay, R., Beatty, J. J. (ORCID:0000000304814952), Becker Tjus, J. (ORCID:0000000217487367), Beise, J. (ORCID:0000000274484189), Bellenghi, C. (ORCID:0000000185257515), Benning, C., BenZvi, S. (ORCID:0000000155374710), Berley, D., Bernardini, E. (ORCID:0000000331081141), Besson, D. Z. (ORCID:000000016733963X), Blaufuss, E. (ORCID:0000000154501757), Bloom, L. (ORCID:0009000599383164), Blot, S. (ORCID:0000000310893001), Bontempo, F., Book Motzkin, J. Y. (ORCID:0000000166875959), Boscolo Meneguolo, C. (ORCID:0000000183254329), Böser, S. (ORCID:0000000259184890), Botner, O. (ORCID:0000000185887306), Böttcher, J. (ORCID:0000000233874236), Braun, J., Brinson, B. (ORCID:0000000191281159), Brostean-Kaiser, J., Brusa, L., Burley, R. T., Butterfield, D., Campana, M. A. (ORCID:0000000341625739), Caracas, I., Carloni, K., Carpio, J. (ORCID:0000000306676557), Chattopadhyay, S., Chau, N., Chen, Z. (ORCID:0000000228137688), Chirkin, D. (ORCID:0000000349111345), Choi, S., Clark, B. A. (ORCID:0000000340892245), Coleman, A. (ORCID:0000000315101712), Collin, G. H., Connolly, A., Conrad, J. M. (ORCID:0000000263930438), Corley, R., Cowen, D. F. (ORCID:0000000347380787), Dave, P. (ORCID:0000000238795115), De Clercq, C. (ORCID:0000000152667059), DeLaunay, J. J. (ORCID:0000000152291995), Delgado, D. (ORCID:0000000243068828), Deng, S., Desai, A. (ORCID:0000000174059994), Desiati, P. (ORCID:0000000197681858), de Vries, K. D. (ORCID:0000000298424068), de Wasseige, G. (ORCID:0000000210105100), DeYoung, T. (ORCID:0000000348733783), Diaz, A. (ORCID:0000000172068336), Díaz-Vélez, J. C. (ORCID:0000000200870693), Dierichs, P., Dittmer, M., Domi, A., Draper, L., Dujmovic, H. (ORCID:0000000318910718), Durnford, D. (ORCID:0000000266087650), Dutta, K., DuVernois, M. A. (ORCID:0000000229879691), Ehrhardt, T., Eidenschink, L., Eimer, A., Eller, P. (ORCID:0000000163545209), Ellinger, E., El Mentawi, S., Elsässer, D. (ORCID:0000000167963205), Engel, R., Erpenbeck, H. (ORCID:0000000163192108), Evans, J., Evenson, P. A. (ORCID:000000017929810X), Fan, K. L. (ORCID:0000000282464751), Fang, K., Farrag, K., Fazely, A. R. (ORCID:0000000269078020), Fedynitch, A. (ORCID:0000000328373477), Feigl, N., Fiedlschuster, S., Finley, C. (ORCID:000000033350390X). 2024-09-25. Probing the Connection between IceCube Neutrinos and MOJAVE AGN. https://doi.org/10.3847/1538-4357%2Fad643d

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related reports

Dust Survival in Galactic Winds

This repository contains three-dimensional volumetric data from an Eulerian hydrodynamical simulation (conducted on a uniform Cartesian grid) generated by the Cholla hydrodynamics code. The datasets contain snapshots (full-grid, projections, and slices) in the HDF5 format of a multi-phase medium in which a hot, diffuse, dust-free background wind accelerates a cool, dense cloud of gas and dust. This scenario is intended to represent a supernova-driven galactic outflow, in which hot supernova winds are thought to accelerate cool interstellar medium material out of the galactic disk into the surrounding circumgalactic medium. There are three separate datasets for simulations corresponding to three cloud evolutionary scenarios: long-term cloud survival (surv), marginal cloud survival (disr), and cloud destruction (dest). Projection and slice images of the simulations are also included in this repository.

79 ASTRONOMY AND ASTROPHYSICS↗

Unraveling TeV halos with the Cherenkov Telescope Array

Pulsars are observed to emit bright and spatially extended gamma-ray emission at multi-TeV energies. These so-called "TeV halos" are now understood to be a nearly universal feature of middle-aged pulsars. However, many of the key physical processes that govern these systems, particularly those affecting particle diffusion, remain poorly constrained. We aim to evaluate the ability of the Cherenkov Telescope Array (CTA) to probe the physical properties of TeV halos, with a focus on the nearby and well-studied case of the Geminga pulsar. We simulate gamma-ray emission from various TeV halo models, incorporating different assumptions for the injected electron spectrum, spin-down evolution, and energy-dependent diffusion. These models are then used to forecast CTA's sensitivity to spectral and spatial differences, based on realistic mock observations and instrument response simulations. We find that CTA will be able to distinguish between a wide range of TeV halo models that are currently consistent with existing data. In particular, CTA observations can constrain the normalization, energy dependence, and spatial extent of the diffusion coefficient surrounding Geminga, as well as the spectral shape of the injected electron population.

79 ASTRONOMY AND ASTROPHYSICS↗