Observation of inverse Compton emission from a long γ-ray burst
Abstract
Long-duration γ-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterized by an initial phase of bright and highly variable radiation in the kiloelectronvolt-to-megaelectronvolt band, which is probably produced within the jet and lasts from milliseconds to minutes, known as the prompt emission. Subsequently, the interaction of the jet with the surrounding medium generates shock waves that are responsible for the afterglow emission, which lasts from days to months and occurs over a broad energy range from the radio to the gigaelectronvolt bands. The afterglow emission is generally well explained as synchrotron radiation emitted by electrons accelerated by the external shock. Recently, intense long-lasting emission between 0.2 and 1 teraelectronvolts was observed from GRB 190114C. Here we report multi-frequency observations of GRB 190114C, and study the evolution in time of the GRB emission across 17 orders of magnitude in energy, from 5 × 10-6 to 1012 electronvolts. We find that the broadband spectral energy distribution is double-peaked, with the teraelectronvolt emission constituting a distinct spectral component with power comparable to the synchrotron component. This component is associated with the afterglow and is satisfactorily explained by inverse Compton up-scattering of synchrotron photonsmore »
- Authors:
- more »
- Publication Date:
- Research Org.:
- SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)
- Sponsoring Org.:
- USDOE; Ministry of Economic Affairs and Digital Transformation of Spain (MINECO); Academy of Finland; Spanish Centro de Excelencia; Polish National Research Centre; National Key Research and Development Program of China; National Aeronautics and Space Administration (NASA); German Research Foundation (DFG); Polish NCN MAESTRO; ASI; UK Space Agency; UK Science and Technology Facilities Council; National Science Centre, Poland; Department of Science and Technology, India; European Research Council (ERC)
- Contributing Org.:
- MAGIC Collaboration
- OSTI Identifier:
- 1596639
- Grant/Contract Number:
- AC02-76SF00515; FPA2017-87859-P; FPA2017-85668-P; FPA2017-82729-C6-2-R; FPA2017-82729-C6-6-R; FPA2017-82729-C6-5-R; AYA2015-71042-P; AYA2016-76012-C3-1-P; ESP2017-87055-C2-2-P; FPA201790566REDC; 320045; SEV-2016-0588; SEV-2015-0548; UMO-2016/22/M/ST9/00382; 2017YFA0402700; NNM11AA01A; HA 1850/28-1; 2014/14/A/ST9/00121; I/004/11/3; 2017-14-H.0; ST/P002323/1; ST/N00811/1; 2018/30/E/ST9/00208; 758638
- Resource Type:
- Accepted Manuscript
- Journal Name:
- Nature (London)
- Additional Journal Information:
- Journal Name: Nature (London); Journal Volume: 575; Journal Issue: 7783; Journal ID: ISSN 0028-0836
- Publisher:
- Nature Publishing Group
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; high-energy astrophysics; transient astrophysical phenomena
Citation Formats
Veres, P., Bhat, P. N., Briggs, M. S., Cleveland, W. H., Hamburg, R., Hui, C. M., Mailyan, B., Preece, R. D., Roberts, O. J., von Kienlin, A., Wilson-Hodge, C. A., Kocevski, D., Arimoto, M., Tak, D., Asano, K., Axelsson, M., Barbiellini, G., Bissaldi, E., Dirirsa, F. Fana, Gill, R., Granot, J., McEnery, J., Omodei, N., Razzaque, S., Piron, F., Racusin, J. L., Thompson, D. J., Campana, S., Bernardini, M. G., Kuin, N. P. M., Siegel, M. H., Cenko, S. B., O’Brien, P., Capalbi, M., Daì, A., De Pasquale, M., Gropp, J., Klingler, N., Osborne, J. P., Perri, M., Starling, R. L. C., Tagliaferri, G., Tohuvavohu, A., Ursi, A., Tavani, M., Cardillo, M., Casentini, C., Piano, G., Evangelista, Y., Verrecchia, F., Pittori, C., Lucarelli, F., Bulgarelli, A., Parmiggiani, N., Anderson, G. E., Anderson, J. P., Bernardi, G., Bolmer, J., Caballero-García, M. D., Carrasco, I. M., Castellón, A., Segura, N. Castro, Castro-Tirado, A. J., Cherukuri, S. V., Cockeram, A. M., D’Avanzo, P., Di Dato, A., Diretse, R., Fender, R. P., Fernández-García, E., Fynbo, J. P. U., Fruchter, A. S., Greiner, J., Gromadzki, M., Heintz, K. E., Heywood, I., van der Horst, A. J., Hu, Y. -D., Inserra, C., Izzo, L., Jaiswal, V., Jakobsson, P., Japelj, J., Kankare, E., Kann, D. A., Kouveliotou, C., Klose, S., Levan, A. J., Li, X. Y., Lotti, S., Maguire, K., Malesani, D. B., Manulis, I., Marongiu, M., Martin, S., Melandri, A., Michałowski, M. J., Miller-Jones, J. C. A., Misra, K., Moin, A., Mooley, K. P., Nasri, S., Nicholl, M., Noschese, A., Novara, G., Pandey, S. B., Peretti, E., del Pulgar, C. J. Pérez, Pérez-Torres, M. A., Perley, D. A., Piro, L., Ragosta, F., Resmi, L., Ricci, R., Rossi, A., Sánchez-Ramírez, R., Selsing, J., Schulze, S., Smartt, S. J., Smith, I. A., Sokolov, V. V., Stevens, J., Tanvir, N. R., Thöne, C. C., Tiengo, A., Tremou, E., Troja, E., de Ugarte Postigo, A., Valeev, A. F., Vergani, S. D., Wieringa, M., Woudt, P. A., Xu, D., Yaron, O., and Young, D. R. Observation of inverse Compton emission from a long γ-ray burst. United States: N. p., 2019.
Web. doi:10.1038/s41586-019-1754-6.
Veres, P., Bhat, P. N., Briggs, M. S., Cleveland, W. H., Hamburg, R., Hui, C. M., Mailyan, B., Preece, R. D., Roberts, O. J., von Kienlin, A., Wilson-Hodge, C. A., Kocevski, D., Arimoto, M., Tak, D., Asano, K., Axelsson, M., Barbiellini, G., Bissaldi, E., Dirirsa, F. Fana, Gill, R., Granot, J., McEnery, J., Omodei, N., Razzaque, S., Piron, F., Racusin, J. L., Thompson, D. J., Campana, S., Bernardini, M. G., Kuin, N. P. M., Siegel, M. H., Cenko, S. B., O’Brien, P., Capalbi, M., Daì, A., De Pasquale, M., Gropp, J., Klingler, N., Osborne, J. P., Perri, M., Starling, R. L. C., Tagliaferri, G., Tohuvavohu, A., Ursi, A., Tavani, M., Cardillo, M., Casentini, C., Piano, G., Evangelista, Y., Verrecchia, F., Pittori, C., Lucarelli, F., Bulgarelli, A., Parmiggiani, N., Anderson, G. E., Anderson, J. P., Bernardi, G., Bolmer, J., Caballero-García, M. D., Carrasco, I. M., Castellón, A., Segura, N. Castro, Castro-Tirado, A. J., Cherukuri, S. V., Cockeram, A. M., D’Avanzo, P., Di Dato, A., Diretse, R., Fender, R. P., Fernández-García, E., Fynbo, J. P. U., Fruchter, A. S., Greiner, J., Gromadzki, M., Heintz, K. E., Heywood, I., van der Horst, A. J., Hu, Y. -D., Inserra, C., Izzo, L., Jaiswal, V., Jakobsson, P., Japelj, J., Kankare, E., Kann, D. A., Kouveliotou, C., Klose, S., Levan, A. J., Li, X. Y., Lotti, S., Maguire, K., Malesani, D. B., Manulis, I., Marongiu, M., Martin, S., Melandri, A., Michałowski, M. J., Miller-Jones, J. C. A., Misra, K., Moin, A., Mooley, K. P., Nasri, S., Nicholl, M., Noschese, A., Novara, G., Pandey, S. B., Peretti, E., del Pulgar, C. J. Pérez, Pérez-Torres, M. A., Perley, D. A., Piro, L., Ragosta, F., Resmi, L., Ricci, R., Rossi, A., Sánchez-Ramírez, R., Selsing, J., Schulze, S., Smartt, S. J., Smith, I. A., Sokolov, V. V., Stevens, J., Tanvir, N. R., Thöne, C. C., Tiengo, A., Tremou, E., Troja, E., de Ugarte Postigo, A., Valeev, A. F., Vergani, S. D., Wieringa, M., Woudt, P. A., Xu, D., Yaron, O., & Young, D. R. Observation of inverse Compton emission from a long γ-ray burst. United States. https://doi.org/10.1038/s41586-019-1754-6
Veres, P., Bhat, P. N., Briggs, M. S., Cleveland, W. H., Hamburg, R., Hui, C. M., Mailyan, B., Preece, R. D., Roberts, O. J., von Kienlin, A., Wilson-Hodge, C. A., Kocevski, D., Arimoto, M., Tak, D., Asano, K., Axelsson, M., Barbiellini, G., Bissaldi, E., Dirirsa, F. Fana, Gill, R., Granot, J., McEnery, J., Omodei, N., Razzaque, S., Piron, F., Racusin, J. L., Thompson, D. J., Campana, S., Bernardini, M. G., Kuin, N. P. M., Siegel, M. H., Cenko, S. B., O’Brien, P., Capalbi, M., Daì, A., De Pasquale, M., Gropp, J., Klingler, N., Osborne, J. P., Perri, M., Starling, R. L. C., Tagliaferri, G., Tohuvavohu, A., Ursi, A., Tavani, M., Cardillo, M., Casentini, C., Piano, G., Evangelista, Y., Verrecchia, F., Pittori, C., Lucarelli, F., Bulgarelli, A., Parmiggiani, N., Anderson, G. E., Anderson, J. P., Bernardi, G., Bolmer, J., Caballero-García, M. D., Carrasco, I. M., Castellón, A., Segura, N. Castro, Castro-Tirado, A. J., Cherukuri, S. V., Cockeram, A. M., D’Avanzo, P., Di Dato, A., Diretse, R., Fender, R. P., Fernández-García, E., Fynbo, J. P. U., Fruchter, A. S., Greiner, J., Gromadzki, M., Heintz, K. E., Heywood, I., van der Horst, A. J., Hu, Y. -D., Inserra, C., Izzo, L., Jaiswal, V., Jakobsson, P., Japelj, J., Kankare, E., Kann, D. A., Kouveliotou, C., Klose, S., Levan, A. J., Li, X. Y., Lotti, S., Maguire, K., Malesani, D. B., Manulis, I., Marongiu, M., Martin, S., Melandri, A., Michałowski, M. J., Miller-Jones, J. C. A., Misra, K., Moin, A., Mooley, K. P., Nasri, S., Nicholl, M., Noschese, A., Novara, G., Pandey, S. B., Peretti, E., del Pulgar, C. J. Pérez, Pérez-Torres, M. A., Perley, D. A., Piro, L., Ragosta, F., Resmi, L., Ricci, R., Rossi, A., Sánchez-Ramírez, R., Selsing, J., Schulze, S., Smartt, S. J., Smith, I. A., Sokolov, V. V., Stevens, J., Tanvir, N. R., Thöne, C. C., Tiengo, A., Tremou, E., Troja, E., de Ugarte Postigo, A., Valeev, A. F., Vergani, S. D., Wieringa, M., Woudt, P. A., Xu, D., Yaron, O., and Young, D. R. Wed .
"Observation of inverse Compton emission from a long γ-ray burst". United States. https://doi.org/10.1038/s41586-019-1754-6. https://www.osti.gov/servlets/purl/1596639.
@article{osti_1596639,
title = {Observation of inverse Compton emission from a long γ-ray burst},
author = {Veres, P. and Bhat, P. N. and Briggs, M. S. and Cleveland, W. H. and Hamburg, R. and Hui, C. M. and Mailyan, B. and Preece, R. D. and Roberts, O. J. and von Kienlin, A. and Wilson-Hodge, C. A. and Kocevski, D. and Arimoto, M. and Tak, D. and Asano, K. and Axelsson, M. and Barbiellini, G. and Bissaldi, E. and Dirirsa, F. Fana and Gill, R. and Granot, J. and McEnery, J. and Omodei, N. and Razzaque, S. and Piron, F. and Racusin, J. L. and Thompson, D. J. and Campana, S. and Bernardini, M. G. and Kuin, N. P. M. and Siegel, M. H. and Cenko, S. B. and O’Brien, P. and Capalbi, M. and Daì, A. and De Pasquale, M. and Gropp, J. and Klingler, N. and Osborne, J. P. and Perri, M. and Starling, R. L. C. and Tagliaferri, G. and Tohuvavohu, A. and Ursi, A. and Tavani, M. and Cardillo, M. and Casentini, C. and Piano, G. and Evangelista, Y. and Verrecchia, F. and Pittori, C. and Lucarelli, F. and Bulgarelli, A. and Parmiggiani, N. and Anderson, G. E. and Anderson, J. P. and Bernardi, G. and Bolmer, J. and Caballero-García, M. D. and Carrasco, I. M. and Castellón, A. and Segura, N. Castro and Castro-Tirado, A. J. and Cherukuri, S. V. and Cockeram, A. M. and D’Avanzo, P. and Di Dato, A. and Diretse, R. and Fender, R. P. and Fernández-García, E. and Fynbo, J. P. U. and Fruchter, A. S. and Greiner, J. and Gromadzki, M. and Heintz, K. E. and Heywood, I. and van der Horst, A. J. and Hu, Y. -D. and Inserra, C. and Izzo, L. and Jaiswal, V. and Jakobsson, P. and Japelj, J. and Kankare, E. and Kann, D. A. and Kouveliotou, C. and Klose, S. and Levan, A. J. and Li, X. Y. and Lotti, S. and Maguire, K. and Malesani, D. B. and Manulis, I. and Marongiu, M. and Martin, S. and Melandri, A. and Michałowski, M. J. and Miller-Jones, J. C. A. and Misra, K. and Moin, A. and Mooley, K. P. and Nasri, S. and Nicholl, M. and Noschese, A. and Novara, G. and Pandey, S. B. and Peretti, E. and del Pulgar, C. J. Pérez and Pérez-Torres, M. A. and Perley, D. A. and Piro, L. and Ragosta, F. and Resmi, L. and Ricci, R. and Rossi, A. and Sánchez-Ramírez, R. and Selsing, J. and Schulze, S. and Smartt, S. J. and Smith, I. A. and Sokolov, V. V. and Stevens, J. and Tanvir, N. R. and Thöne, C. C. and Tiengo, A. and Tremou, E. and Troja, E. and de Ugarte Postigo, A. and Valeev, A. F. and Vergani, S. D. and Wieringa, M. and Woudt, P. A. and Xu, D. and Yaron, O. and Young, D. R.},
abstractNote = {Long-duration γ-ray bursts (GRBs) originate from ultra-relativistic jets launched from the collapsing cores of dying massive stars. They are characterized by an initial phase of bright and highly variable radiation in the kiloelectronvolt-to-megaelectronvolt band, which is probably produced within the jet and lasts from milliseconds to minutes, known as the prompt emission. Subsequently, the interaction of the jet with the surrounding medium generates shock waves that are responsible for the afterglow emission, which lasts from days to months and occurs over a broad energy range from the radio to the gigaelectronvolt bands. The afterglow emission is generally well explained as synchrotron radiation emitted by electrons accelerated by the external shock. Recently, intense long-lasting emission between 0.2 and 1 teraelectronvolts was observed from GRB 190114C. Here we report multi-frequency observations of GRB 190114C, and study the evolution in time of the GRB emission across 17 orders of magnitude in energy, from 5 × 10-6 to 1012 electronvolts. We find that the broadband spectral energy distribution is double-peaked, with the teraelectronvolt emission constituting a distinct spectral component with power comparable to the synchrotron component. This component is associated with the afterglow and is satisfactorily explained by inverse Compton up-scattering of synchrotron photons by high-energy electrons. Finally, we find that the conditions required to account for the observed teraelectronvolt component are typical for GRBs, supporting the possibility that inverse Compton emission is commonly produced in GRBs.},
doi = {10.1038/s41586-019-1754-6},
journal = {Nature (London)},
number = 7783,
volume = 575,
place = {United States},
year = {Wed Nov 20 00:00:00 EST 2019},
month = {Wed Nov 20 00:00:00 EST 2019}
}
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Works referencing / citing this record:
GRB 190114C in the nuclear region of an interacting galaxy: A detailed host analysis using ALMA, the HST, and the VLT
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GRB 190114C in the nuclear region of an interacting galaxy -- A detailed host analysis using ALMA, HST and VLT
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