The enhanced X-ray Timing and Polarimetry mission-eXTP

Kód výsledku v IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F19%3A00519773" target="_blank" >RIV/67985815:_____/19:00519773 - isvavai.cz</a>

Výsledek na webu

<a href="https://doi.org/10.1007/s11433-018-9309-2" target="_blank" >https://doi.org/10.1007/s11433-018-9309-2</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1007/s11433-018-9309-2" target="_blank" >10.1007/s11433-018-9309-2</a>

Jazyk výsledku

angličtina

Název v původním jazyce

The enhanced X-ray Timing and Polarimetry mission-eXTP

Popis výsledku v původním jazyce

In this paper we present the enhanced X-ray Timing and Polarimetry mission-eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload, (2) the elements and functions of the mission, from the spacecraft to the ground segment.

Název v anglickém jazyce

The enhanced X-ray Timing and Polarimetry mission-eXTP

Popis výsledku anglicky

In this paper we present the enhanced X-ray Timing and Polarimetry mission-eXTP. eXTP is a space science mission designed to study fundamental physics under extreme conditions of density, gravity and magnetism. The mission aims at determining the equation of state of matter at supra-nuclear density, measuring effects of QED, and understanding the dynamics of matter in strong-field gravity. In addition to investigating fundamental physics, eXTP will be a very powerful observatory for astrophysics that will provide observations of unprecedented quality on a variety of galactic and extragalactic objects. In particular, its wide field monitoring capabilities will be highly instrumental to detect the electro-magnetic counterparts of gravitational wave sources. The paper provides a detailed description of: (1) the technological and technical aspects, and the expected performance of the instruments of the scientific payload, (2) the elements and functions of the mission, from the spacecraft to the ground segment.

Druh

J_imp - Článek v periodiku v databázi Web of Science

CEP obor

—

OECD FORD obor

10308 - Astronomy (including astrophysics,space science)

Projekt

—

Návaznosti

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Rok uplatnění

2019

Kód důvěrnosti údajů

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

Název periodika

Science China Physics, Mechanics & Astronomy

ISSN

1674-7348

e-ISSN

—

Svazek periodika

62

Číslo periodika v rámci svazku

2

Stát vydavatele periodika

CN - Čínská lidová republika

Počet stran výsledku

25

Strana od-do

029502

Kód UT WoS článku

000459907000001

EID výsledku v databázi Scopus

2-s2.0-85058963352