511 keV line constraints on feebly interacting particles from supernovae
Feebly interacting particles with masses with O(10-100) MeV can be copiously produced by core-collapse supernovae (SNe). In this paper we consider the case of MeV-ish sterile neutrinos and dark photons mixed with ordinary neutrinos and photons, respectively. Furthermore, both sterile neutrinos and d...
Gespeichert in:
| Hauptverfasser: | , , , , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
29 March 2022
|
| In: |
Physical review
Year: 2022, Jahrgang: 105, Heft: 6, Pages: 1-16 |
| ISSN: | 2470-0029 |
| DOI: | 10.1103/PhysRevD.105.063026 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1103/PhysRevD.105.063026 Verlag, lizenzpflichtig, Volltext: https://link.aps.org/doi/10.1103/PhysRevD.105.063026 
|
| Verfasserangaben: | Francesca Calore, Pierluca Carenza, Maurizio Giannotti, Joerg Jaeckel, Giuseppe Lucente, Leonardo Mastrototaro, and Alessandro Mirizzi |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 1816501786 | ||
| 003 | DE-627 | ||
| 005 | 20230118145623.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 220913s2022 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1103/PhysRevD.105.063026 |2 doi | |
| 035 | |a (DE-627)1816501786 | ||
| 035 | |a (DE-599)KXP1816501786 | ||
| 035 | |a (OCoLC)1361696550 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Calore, Francesca |e VerfasserIn |0 (DE-588)1139137794 |0 (DE-627)896830950 |0 (DE-576)492945284 |4 aut | |
| 245 | 1 | 0 | |a 511 keV line constraints on feebly interacting particles from supernovae |c Francesca Calore, Pierluca Carenza, Maurizio Giannotti, Joerg Jaeckel, Giuseppe Lucente, Leonardo Mastrototaro, and Alessandro Mirizzi |
| 246 | 3 | 3 | |a Five hundred and eleven keV line constraints on feebly interacting particles from supernovae |
| 264 | 1 | |c 29 March 2022 | |
| 300 | |a 16 | ||
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 13.09.2022 | ||
| 520 | |a Feebly interacting particles with masses with O(10-100) MeV can be copiously produced by core-collapse supernovae (SNe). In this paper we consider the case of MeV-ish sterile neutrinos and dark photons mixed with ordinary neutrinos and photons, respectively. Furthermore, both sterile neutrinos and dark photons may decay into positrons on their route to Earth. Such positrons would annihilate with electrons in the Galactic medium and contribute to the photon flux in the 511 keV line. Using the spectrometer on INTEGRAL observation of this line improves the bounds on the mixing parameters for these particles by several orders of magnitude below what is already excluded by the SN 1987A energy-loss argument. | ||
| 700 | 1 | |a Carenza, Pierluca |e VerfasserIn |4 aut | |
| 700 | 1 | |a Giannotti, Maurizio |e VerfasserIn |0 (DE-588)110073452X |0 (DE-627)859531392 |0 (DE-576)469797746 |4 aut | |
| 700 | 1 | |a Jaeckel, Joerg |e VerfasserIn |0 (DE-588)124999050 |0 (DE-627)516179233 |0 (DE-576)294611916 |4 aut | |
| 700 | 1 | |a Lucente, Giuseppe |e VerfasserIn |4 aut | |
| 700 | 1 | |a Mastrototaro, Leonardo |e VerfasserIn |4 aut | |
| 700 | 1 | |a Mirizzi, Alessandro |e VerfasserIn |0 (DE-588)1062750071 |0 (DE-627)806843357 |0 (DE-576)420152636 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Physical review |d Ridge, NY : American Physical Society, 2016 |g 105(2022), 6 vom: März, Artikel-ID 063026, Seite 1-16 |h Online-Ressource |w (DE-627)846313510 |w (DE-600)2844732-3 |w (DE-576)454495811 |x 2470-0029 |7 nnas |a 511 keV line constraints on feebly interacting particles from supernovae |
| 773 | 1 | 8 | |g volume:105 |g year:2022 |g number:6 |g month:03 |g elocationid:063026 |g pages:1-16 |g extent:16 |a 511 keV line constraints on feebly interacting particles from supernovae |
| 856 | 4 | 0 | |u https://doi.org/10.1103/PhysRevD.105.063026 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 856 | 4 | 0 | |u https://link.aps.org/doi/10.1103/PhysRevD.105.063026 |x Verlag |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20220913 | ||
| 993 | |a Article | ||
| 994 | |a 2022 | ||
| 998 | |g 124999050 |a Jaeckel, Joerg |m 124999050:Jaeckel, Joerg |d 130000 |d 130300 |e 130000PJ124999050 |e 130300PJ124999050 |k 0/130000/ |k 1/130000/130300/ |p 4 | ||
| 999 | |a KXP-PPN1816501786 |e 418731279X | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"title":[{"title_sort":"511 keV line constraints on feebly interacting particles from supernovae","title":"511 keV line constraints on feebly interacting particles from supernovae"}],"person":[{"family":"Calore","given":"Francesca","display":"Calore, Francesca","roleDisplay":"VerfasserIn","role":"aut"},{"display":"Carenza, Pierluca","roleDisplay":"VerfasserIn","role":"aut","family":"Carenza","given":"Pierluca"},{"role":"aut","display":"Giannotti, Maurizio","roleDisplay":"VerfasserIn","given":"Maurizio","family":"Giannotti"},{"role":"aut","roleDisplay":"VerfasserIn","display":"Jaeckel, Joerg","given":"Joerg","family":"Jaeckel"},{"given":"Giuseppe","family":"Lucente","role":"aut","roleDisplay":"VerfasserIn","display":"Lucente, Giuseppe"},{"role":"aut","display":"Mastrototaro, Leonardo","roleDisplay":"VerfasserIn","given":"Leonardo","family":"Mastrototaro"},{"given":"Alessandro","family":"Mirizzi","role":"aut","roleDisplay":"VerfasserIn","display":"Mirizzi, Alessandro"}],"titleAlt":[{"title":"Five hundred and eleven keV line constraints on feebly interacting particles from supernovae"}],"recId":"1816501786","language":["eng"],"type":{"bibl":"article-journal","media":"Online-Ressource"},"note":["Gesehen am 13.09.2022"],"id":{"eki":["1816501786"],"doi":["10.1103/PhysRevD.105.063026"]},"origin":[{"dateIssuedKey":"2022","dateIssuedDisp":"29 March 2022"}],"name":{"displayForm":["Francesca Calore, Pierluca Carenza, Maurizio Giannotti, Joerg Jaeckel, Giuseppe Lucente, Leonardo Mastrototaro, and Alessandro Mirizzi"]},"relHost":[{"title":[{"title":"Physical review","title_sort":"Physical review"}],"corporate":[{"role":"isb","roleDisplay":"Herausgebendes Organ","display":"American Physical Society"}],"language":["eng"],"recId":"846313510","disp":"511 keV line constraints on feebly interacting particles from supernovaePhysical review","type":{"bibl":"periodical","media":"Online-Ressource"},"note":["Gesehen am 14.03.2023"],"titleAlt":[{"title":"Particles, fields, gravitation, and cosmology"}],"part":{"issue":"6","pages":"1-16","year":"2022","extent":"16","volume":"105","text":"105(2022), 6 vom: März, Artikel-ID 063026, Seite 1-16"},"pubHistory":["3rd series, volume 93, number 1 (January 2016)-"],"name":{"displayForm":["published by American Physical Society"]},"id":{"issn":["2470-0029"],"eki":["846313510"],"zdb":["2844732-3"]},"origin":[{"dateIssuedDisp":"2016-","publisher":"American Physical Society","dateIssuedKey":"2016","publisherPlace":"Ridge, NY"}],"physDesc":[{"extent":"Online-Ressource"}]}],"physDesc":[{"extent":"16 S."}]} | ||
| SRT | |a CALOREFRAN511KEVLINE2920 | ||