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
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/76778
Acceder
id CONICETDig_999e6ac7a46b55a90ca5db4da5e9341f
oai_identifier_str oai:ri.conicet.gov.ar:11336/76778
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling 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 Técnicas2025-10-22T12:11:54Zoai: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:34982025-10-22 12:11:54.976CONICET 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
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
collection CONICET Digital (CONICET)
instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
_version_ 1846782513190535168
score 12.982451

Publicaciones similares