POEMMA's target-of-opportunity sensitivity to cosmic neutrino transient sources

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A_____%2F20%3A00546317" target="_blank" >RIV/68378271:_____/20:00546317 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1103/PhysRevD.102.123013" target="_blank" >https://doi.org/10.1103/PhysRevD.102.123013</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1103/PhysRevD.102.123013" target="_blank" >10.1103/PhysRevD.102.123013</a>

Jazyk výsledku

angličtina

Název v původním jazyce

POEMMA's target-of-opportunity sensitivity to cosmic neutrino transient sources

Popis výsledku v původním jazyce

We investigate the capability of the Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) in performing target-of-opportunity (ToO) neutrino observations. POEMMA is a proposed space-based probe-class mission for ultrahigh-energy cosmic ray and very-high-energy neutrino detection using two spacecraft, each equipped with a large Schmidt telescope to detect optical and near-ultraviolet signals generated by extensive air showers (EASs). POEMMA will be sensitive to Cherenkov radiation from upward-moving EASs initiated by tau neutrinos interacting in the Earth. POEMMA will be able to quickly repoint (90 degrees in 500 s) each of the two spacecrafts to the direction of an astrophysical source, which in combination with its orbital speed will provide it with unparalleled capability to follow-up transient alerts.

Název v anglickém jazyce

POEMMA's target-of-opportunity sensitivity to cosmic neutrino transient sources

Popis výsledku anglicky

We investigate the capability of the Probe Of Extreme Multi-Messenger Astrophysics (POEMMA) in performing target-of-opportunity (ToO) neutrino observations. POEMMA is a proposed space-based probe-class mission for ultrahigh-energy cosmic ray and very-high-energy neutrino detection using two spacecraft, each equipped with a large Schmidt telescope to detect optical and near-ultraviolet signals generated by extensive air showers (EASs). POEMMA will be sensitive to Cherenkov radiation from upward-moving EASs initiated by tau neutrinos interacting in the Earth. POEMMA will be able to quickly repoint (90 degrees in 500 s) each of the two spacecrafts to the direction of an astrophysical source, which in combination with its orbital speed will provide it with unparalleled capability to follow-up transient alerts.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10303 - Particles and field physics

Projekt

—

Návaznosti

—

Rok uplatnění

2020

Kód důvěrnosti údajů

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Název periodika

Physical Review D

ISSN

2470-0010

e-ISSN

2470-0029

Svazek periodika

102

Číslo periodika v rámci svazku

12

Stát vydavatele periodika

US - Spojené státy americké

Počet stran výsledku

34

Strana od-do

123013

Kód UT WoS článku

000596370800005

EID výsledku v databázi Scopus

2-s2.0-85102075278