ASPHWWW.PH.NODA.TUS.AC.JP

Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus)

Tokyo University of Science, Noda Campus. Welcome to the website of Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus). We are especially interested in the supernova physics. Model Spectrum of Supernova Relic Neutrino Background. EOS for Neutron Star Matter. Study of Explosive Astrophysical Phenomena and Nucleosynthesis based on Quark Dynamics and Nuclear Structure. Department of Physics, Faculty of Science and Technology, Tokyo University of Science. Last up date, Mar 31, 2015.

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Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus) | asphwww.ph.noda.tus.ac.jp Reviews

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Tokyo University of Science, Noda Campus. Welcome to the website of Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus). We are especially interested in the supernova physics. Model Spectrum of Supernova Relic Neutrino Background. EOS for Neutron Star Matter. Study of Explosive Astrophysical Phenomena and Nucleosynthesis based on Quark Dynamics and Nuclear Structure. Department of Physics, Faculty of Science and Technology, Tokyo University of Science. Last up date, Mar 31, 2015.

<META> KEYWORDS

1 theoretical astrophysics group

2 staffs

3 hideyuki suzuki professor

4 ken'ichiro nakazato

5 assistant professor

6 supernova neutrino database

7 project

8 in japanese

9 address

10 coupons

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theoretical astrophysics group,staffs,hideyuki suzuki professor,ken'ichiro nakazato,assistant professor,supernova neutrino database,project,in japanese,address

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Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus) | asphwww.ph.noda.tus.ac.jp Reviews

https://asphwww.ph.noda.tus.ac.jp

Tokyo University of Science, Noda Campus. Welcome to the website of Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus). We are especially interested in the supernova physics. Model Spectrum of Supernova Relic Neutrino Background. EOS for Neutron Star Matter. Study of Explosive Astrophysical Phenomena and Nucleosynthesis based on Quark Dynamics and Nuclear Structure. Department of Physics, Faculty of Science and Technology, Tokyo University of Science. Last up date, Mar 31, 2015.

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asphwww.ph.noda.tus.ac.jp

1

Supernova Neutrino Database

http://asphwww.ph.noda.tus.ac.jp/snn

Web site of Supernova Neutrino Database. This web site provides a series of numerical simulations of supernova neutrino emission from core collapse to neutron star cooling ( 20 sec) for various progenitor stellar models (13-50 M. ArXiv:1210.6841 [astro-ph.HE]. This data set is open for general use in any research for astronomy, astrophysics, and physics, provided that our paper is referenced in your publication. Because the neutrino signal from BH formation considerably depends on nuclear EOS. While ...

2

Ken'ichiro Nakazato web site

http://asphwww.ph.noda.tus.ac.jp/nakazato

Ken'ichiro Nakazato web site. Japanese version is here. Institution: Department of Physics, Faculty of Science and Technology, Tokyo University of Science. Address: 2641 Yamazaki, Noda, Chiba 278-8510, Japan. Phone: 81-4-7124-1501 (ext. 3267). Research interests: Theoretical Astrophysics (High Energy Astrophysics, Neutrino Astronomy, Nuclear Astrophysics). List of Research Activity. Last up date, Oct. 13, 2013.

3

Supernova Relic Neutrino

http://asphwww.ph.noda.tus.ac.jp/srn

Web site of Supernova Relic Neutrino Background. On the basis of the metallicity evolution of galaxies - -. ArXiv:1503.01236 [astro-ph.HE]. For the neutrino spectra emitted from various progenitors, we utilize the Supernova Neutrino Database. Nakazato et al., Astrophys. J. Supp. 205 (2013) 2. ArXiv:1210.6841 [astro-ph.HE]. This data set is open for general use in any research for astronomy, astrophysics, and physics, provided that our papers are referenced in your publication. User's Guide (read me first).

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asphwww.ph.noda.tus.ac.jp

Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus)

Tokyo University of Science, Noda Campus. Welcome to the website of Theoretical Astrophysics Group, Tokyo University of Science (Noda Campus). We are especially interested in the supernova physics. Model Spectrum of Supernova Relic Neutrino Background. EOS for Neutron Star Matter. Study of Explosive Astrophysical Phenomena and Nucleosynthesis based on Quark Dynamics and Nuclear Structure. Department of Physics, Faculty of Science and Technology, Tokyo University of Science. Last up date, Mar 31, 2015.

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