Advanced search

Browse by subject

Browse by provider

Browse by language

Content Details
Normal View
CIP View

Multi-messenger signals of long-term cor...

Nakamura, Ko...

Free

Share this content

Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies by Nakamura, Ko ( Author )

Content Provider	Lemonjar Open Access
Publisher	N.A
Publication Date	09-02-2016
Summary	The next Galactic supernova is expected to bring great opportunities for the direct detection of gravitational waves (GW), full flavor neutrinos, and multi-wavelength photons. To maximize the science return from such a rare event, it is essential to have established classes of possible situations and preparations for appropriate observations. To this end, we use a long-term numerical simulation of the core-collapse supernova (CCSN) of a 17 solar-mass red supergiant progenitor to self-consistently model the multi-messenger signals expected in GW, neutrino, and electromagnetic messengers. This supernova model takes into account the formation and evolution of a protoneutron star, neutrino-matter interaction, and neutrino transport, all within a two-dimensional shock hydrodynamics simulation. With this, we separately discuss three situations: (i) a CCSN at the Galactic Center, (ii) an extremely nearby CCSN within hundreds of parsecs, and (iii) a CCSN in nearby galaxies within several Mpc. These distance regimes necessitate different strategies for synergistic observations. In a Galactic CCSN, neutrinos provide strategic timing and pointing information. We explore how these in turn deliver an improvement in the sensitivity of GW analyses and help to guarantee observations of early electromagnetic signals. To facilitate the detection of multi-messenger signals of CCSNe in extremely nearby and extragalactic distances, we compile a list of nearby red supergiant candidates and a list of nearby galaxies with their expected CCSN rates. By exploring the sequential multi-messenger signals of a nearby CCSN, we discuss preparations for maximizing successful studies of such an unprecedented stirring event.
ISBN	-
Item Type	Article
File Type	pdf
File Size	36.88 KB
Language	English
Subjects	-
Unlimited	MYR 0.01
Total read	-
URL	https://arxiv.org/abs/1602.03028

Citation

Review the full bibliography data and make any necessary corrections before using. Always consult your library resources for the exact formatting and punctuation guidelines.

AMA 11th EditionReferences

Nakamura, Ko. Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies. N.A. February 09, 2016. Accessed November 10, 2024. https://online.provdatabase.com/cite/22755

APA 7th EditionReferences

Nakamura, Ko. (2016). Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies. N.A. https://online.provdatabase.com/cite/22755

Chicago 17th EditionReferences

Nakamura, Ko. Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies. N.A. 2016. https://online.provdatabase.com/cite/22755

HarvardReferences

Nakamura, Ko. (2016). Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies. [Online]. N.A. Available from: https://online.provdatabase.com/cite/22755. (Accessed 10 November 2024).

Harvard AustraliaReferences

Nakamura, Ko, 2016, Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies, N.A, viewed 10 November 2024, <https://online.provdatabase.com/cite/22755>

MLA 9th EditionWorks Cited

Nakamura, Ko. Multi-messenger signals of long-term core-collapse supernova simulations : synergetic observation strategies. N.A, 2016. PROV Database, https://online.provdatabase.com/cite/22755.

Share this eBook