Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant
- Autores
- Eriksen, Kristoffer A.; Hughes, John P.; Badenes, Carles; Fesen, Robert; Ghavamian, Parviz; Moffett, David; Plucinksy, Paul P.; Rakowski, Cara E.; Reynoso, Estela Marta; Slane, Patrick
- Año de publicación
- 2011
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock acceleration (DSA). Since CR nuclei do not radiate efficiently, their presence must be inferred indirectly. Previous theoretical calculations and X-ray observations show that CR acceleration significantly modifies the structure of the SNR and greatly amplifies the interstellar magnetic field. We present new, deep X-ray observations of the remnant of Tycho's supernova (SN 1572, henceforth Tycho), which reveal a previously unknown, strikingly ordered pattern of non-thermal high-emissivity stripes in the projected interior of the remnant, with spacing that corresponds to the gyroradii of 1014-1015 eV protons. Spectroscopy of the stripes shows the plasma to be highly turbulent on the (smaller) scale of the Larmor radii of TeV energy electrons. Models of the shock amplification of magnetic fields produce structure on the scale of the gyroradius of the highest energy CRs present, but they do not predict the highly ordered pattern we observe. We interpret the stripes as evidence for acceleration of particles to near the knee of the CR spectrum in regions of enhanced magnetic turbulence, while the observed highly ordered pattern of these features provides a new challenge to models of DSA. © 2011. The American Astronomical Society.
Fil: Eriksen, Kristoffer A.. Rutgers, The State University Of New Jersey; Estados Unidos
Fil: Hughes, John P.. Rutgers, The State University Of New Jersey; Estados Unidos
Fil: Badenes, Carles. Weizmann Institute Of Science Israel; Israel. Tel Aviv University; Israel
Fil: Fesen, Robert. Dartmouth College; Estados Unidos
Fil: Ghavamian, Parviz. Space Telescope Science Institute; Estados Unidos
Fil: Moffett, David. Furman University; Estados Unidos
Fil: Plucinksy, Paul P.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos
Fil: Rakowski, Cara E.. Spece Sciences División. Naval Research Laboratory; Estados Unidos
Fil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Slane, Patrick. Harvard-Smithsonian Center for Astrophysics; Estados Unidos - Materia
-
ACCELERATION OF PARTICLES
COSMIC RAYS
ISM: INDIVIDUAL OBJECTS (SN 1572, TYCHO)
ISM: SUPERNOVA REMNANTS - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
- Repositorio
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/76778
Ver los metadatos del registro completo
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Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnantEriksen, Kristoffer A.Hughes, John P.Badenes, CarlesFesen, RobertGhavamian, ParvizMoffett, DavidPlucinksy, Paul P.Rakowski, Cara E.Reynoso, Estela MartaSlane, PatrickACCELERATION OF PARTICLESCOSMIC RAYSISM: INDIVIDUAL OBJECTS (SN 1572, TYCHO)ISM: SUPERNOVA REMNANTSSupernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock acceleration (DSA). Since CR nuclei do not radiate efficiently, their presence must be inferred indirectly. Previous theoretical calculations and X-ray observations show that CR acceleration significantly modifies the structure of the SNR and greatly amplifies the interstellar magnetic field. We present new, deep X-ray observations of the remnant of Tycho's supernova (SN 1572, henceforth Tycho), which reveal a previously unknown, strikingly ordered pattern of non-thermal high-emissivity stripes in the projected interior of the remnant, with spacing that corresponds to the gyroradii of 1014-1015 eV protons. Spectroscopy of the stripes shows the plasma to be highly turbulent on the (smaller) scale of the Larmor radii of TeV energy electrons. Models of the shock amplification of magnetic fields produce structure on the scale of the gyroradius of the highest energy CRs present, but they do not predict the highly ordered pattern we observe. We interpret the stripes as evidence for acceleration of particles to near the knee of the CR spectrum in regions of enhanced magnetic turbulence, while the observed highly ordered pattern of these features provides a new challenge to models of DSA. © 2011. The American Astronomical Society.Fil: Eriksen, Kristoffer A.. Rutgers, The State University Of New Jersey; Estados UnidosFil: Hughes, John P.. Rutgers, The State University Of New Jersey; Estados UnidosFil: Badenes, Carles. Weizmann Institute Of Science Israel; Israel. Tel Aviv University; IsraelFil: Fesen, Robert. Dartmouth College; Estados UnidosFil: Ghavamian, Parviz. Space Telescope Science Institute; Estados UnidosFil: Moffett, David. Furman University; Estados UnidosFil: Plucinksy, Paul P.. Harvard-Smithsonian Center for Astrophysics; Estados UnidosFil: Rakowski, Cara E.. Spece Sciences División. Naval Research Laboratory; Estados UnidosFil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Slane, Patrick. Harvard-Smithsonian Center for Astrophysics; Estados UnidosInstitute of Physics Publishing2011-02info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/76778Eriksen, Kristoffer A.; Hughes, John P.; Badenes, Carles; Fesen, Robert; Ghavamian, Parviz; et al.; Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant; Institute of Physics Publishing; Astrophysical Journal Letters; 728; 2 Part II; 2-2011; 28-322041-8213CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/728/2/L28info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T10:39:37Zoai:ri.conicet.gov.ar:11336/76778instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 10:39:37.966CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
dc.title.none.fl_str_mv |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
title |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
spellingShingle |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant Eriksen, Kristoffer A. ACCELERATION OF PARTICLES COSMIC RAYS ISM: INDIVIDUAL OBJECTS (SN 1572, TYCHO) ISM: SUPERNOVA REMNANTS |
title_short |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
title_full |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
title_fullStr |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
title_full_unstemmed |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
title_sort |
Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant |
dc.creator.none.fl_str_mv |
Eriksen, Kristoffer A. Hughes, John P. Badenes, Carles Fesen, Robert Ghavamian, Parviz Moffett, David Plucinksy, Paul P. Rakowski, Cara E. Reynoso, Estela Marta Slane, Patrick |
author |
Eriksen, Kristoffer A. |
author_facet |
Eriksen, Kristoffer A. Hughes, John P. Badenes, Carles Fesen, Robert Ghavamian, Parviz Moffett, David Plucinksy, Paul P. Rakowski, Cara E. Reynoso, Estela Marta Slane, Patrick |
author_role |
author |
author2 |
Hughes, John P. Badenes, Carles Fesen, Robert Ghavamian, Parviz Moffett, David Plucinksy, Paul P. Rakowski, Cara E. Reynoso, Estela Marta Slane, Patrick |
author2_role |
author author author author author author author author author |
dc.subject.none.fl_str_mv |
ACCELERATION OF PARTICLES COSMIC RAYS ISM: INDIVIDUAL OBJECTS (SN 1572, TYCHO) ISM: SUPERNOVA REMNANTS |
topic |
ACCELERATION OF PARTICLES COSMIC RAYS ISM: INDIVIDUAL OBJECTS (SN 1572, TYCHO) ISM: SUPERNOVA REMNANTS |
dc.description.none.fl_txt_mv |
Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock acceleration (DSA). Since CR nuclei do not radiate efficiently, their presence must be inferred indirectly. Previous theoretical calculations and X-ray observations show that CR acceleration significantly modifies the structure of the SNR and greatly amplifies the interstellar magnetic field. We present new, deep X-ray observations of the remnant of Tycho's supernova (SN 1572, henceforth Tycho), which reveal a previously unknown, strikingly ordered pattern of non-thermal high-emissivity stripes in the projected interior of the remnant, with spacing that corresponds to the gyroradii of 1014-1015 eV protons. Spectroscopy of the stripes shows the plasma to be highly turbulent on the (smaller) scale of the Larmor radii of TeV energy electrons. Models of the shock amplification of magnetic fields produce structure on the scale of the gyroradius of the highest energy CRs present, but they do not predict the highly ordered pattern we observe. We interpret the stripes as evidence for acceleration of particles to near the knee of the CR spectrum in regions of enhanced magnetic turbulence, while the observed highly ordered pattern of these features provides a new challenge to models of DSA. © 2011. The American Astronomical Society. Fil: Eriksen, Kristoffer A.. Rutgers, The State University Of New Jersey; Estados Unidos Fil: Hughes, John P.. Rutgers, The State University Of New Jersey; Estados Unidos Fil: Badenes, Carles. Weizmann Institute Of Science Israel; Israel. Tel Aviv University; Israel Fil: Fesen, Robert. Dartmouth College; Estados Unidos Fil: Ghavamian, Parviz. Space Telescope Science Institute; Estados Unidos Fil: Moffett, David. Furman University; Estados Unidos Fil: Plucinksy, Paul P.. Harvard-Smithsonian Center for Astrophysics; Estados Unidos Fil: Rakowski, Cara E.. Spece Sciences División. Naval Research Laboratory; Estados Unidos Fil: Reynoso, Estela Marta. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: Slane, Patrick. Harvard-Smithsonian Center for Astrophysics; Estados Unidos |
description |
Supernova remnants (SNRs) have long been assumed to be the source of cosmic rays (CRs) up to the "knee" of the CR spectrum at 1015 eV, accelerating particles to relativistic energies in their blast waves by the process of diffusive shock acceleration (DSA). Since CR nuclei do not radiate efficiently, their presence must be inferred indirectly. Previous theoretical calculations and X-ray observations show that CR acceleration significantly modifies the structure of the SNR and greatly amplifies the interstellar magnetic field. We present new, deep X-ray observations of the remnant of Tycho's supernova (SN 1572, henceforth Tycho), which reveal a previously unknown, strikingly ordered pattern of non-thermal high-emissivity stripes in the projected interior of the remnant, with spacing that corresponds to the gyroradii of 1014-1015 eV protons. Spectroscopy of the stripes shows the plasma to be highly turbulent on the (smaller) scale of the Larmor radii of TeV energy electrons. Models of the shock amplification of magnetic fields produce structure on the scale of the gyroradius of the highest energy CRs present, but they do not predict the highly ordered pattern we observe. We interpret the stripes as evidence for acceleration of particles to near the knee of the CR spectrum in regions of enhanced magnetic turbulence, while the observed highly ordered pattern of these features provides a new challenge to models of DSA. © 2011. The American Astronomical Society. |
publishDate |
2011 |
dc.date.none.fl_str_mv |
2011-02 |
dc.type.none.fl_str_mv |
info:eu-repo/semantics/article info:eu-repo/semantics/publishedVersion http://purl.org/coar/resource_type/c_6501 info:ar-repo/semantics/articulo |
format |
article |
status_str |
publishedVersion |
dc.identifier.none.fl_str_mv |
http://hdl.handle.net/11336/76778 Eriksen, Kristoffer A.; Hughes, John P.; Badenes, Carles; Fesen, Robert; Ghavamian, Parviz; et al.; Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant; Institute of Physics Publishing; Astrophysical Journal Letters; 728; 2 Part II; 2-2011; 28-32 2041-8213 CONICET Digital CONICET |
url |
http://hdl.handle.net/11336/76778 |
identifier_str_mv |
Eriksen, Kristoffer A.; Hughes, John P.; Badenes, Carles; Fesen, Robert; Ghavamian, Parviz; et al.; Evidence for particle acceleration to the knee of the cosmic ray spectrum in Tycho's supernova remnant; Institute of Physics Publishing; Astrophysical Journal Letters; 728; 2 Part II; 2-2011; 28-32 2041-8213 CONICET Digital CONICET |
dc.language.none.fl_str_mv |
eng |
language |
eng |
dc.relation.none.fl_str_mv |
info:eu-repo/semantics/altIdentifier/doi/10.1088/2041-8205/728/2/L28 |
dc.rights.none.fl_str_mv |
info:eu-repo/semantics/openAccess https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
eu_rights_str_mv |
openAccess |
rights_invalid_str_mv |
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/ |
dc.format.none.fl_str_mv |
application/pdf application/pdf |
dc.publisher.none.fl_str_mv |
Institute of Physics Publishing |
publisher.none.fl_str_mv |
Institute of Physics Publishing |
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reponame:CONICET Digital (CONICET) instname:Consejo Nacional de Investigaciones Científicas y Técnicas |
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Consejo Nacional de Investigaciones Científicas y Técnicas |
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CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas |
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