(kek, sokendai) - icrr...general relativity cosmic ray r-process elements hadron physics merger of...

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井岡 邦仁 (KEK, Sokendai) 宇宙線・宇宙物理領域、理論核物理領域合同シンポジウム 重力波源とその電磁波、ニュートリノ対応天体

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Page 1: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

井岡 邦仁 (KEK, Sokendai)

宇宙線・宇宙物理領域、理論核物理領域合同シンポジウム 重力波源とその電磁波、ニュートリノ対応天体 

Page 2: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

2nd Generation of �GW Observatories

©Ando

2014.3.28 重力波源と対応天体 by K. Ioka 2

Hanford (1or2)

Livingston

GW will be directly detected within ~5 yr

Page 3: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

3 重力波源と対応天体 by K. Ioka 2014.3.28

? ? ? Gravitational wave X-ray IR-Opt Radio

!!!

? ? Neutrino Gamma-ray Gravitational Wave Sources

Counterparts to GW

Page 4: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

2014.3.28 重力波源と対応天体 by K. Ioka 4

? ? ? Gravitational wave X-ray IR-Opt Radio

!!!

? ? Neutrino Gamma-ray Gravitational Wave Sources

Counterparts to GW

  Short GRB origin   Confident GW detection   Parameter reduction   GW Astronomy, Cosmology   General relativity   Cosmic ray   r-process elements   Hadron physics

Page 5: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

Merger of 1.3-1.4 Msun NS: EOS=APR4; stiff but relatively soft

ρ (g/cm3)

Orbital plane X-Z plane

Relatively wider view

©Shibata, Hotokezaka

2014.3.28 重力波源と対応天体 by K. Ioka 5

Page 6: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

BH-NS Merger

Only Ejecta

x-z plane, only ejecta Full GR Q=5 χ=0.75 H4 EOS

Kyutoku, KI & Shibata 13 Hotokezaka+ 13 Tanaka+ 14 Kiuchi+ 14

©Kyutoku

2014.3.28 重力波源と対応天体 by K. Ioka 6

Page 7: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

7 11/28/12  GRBと重力波 by K. Ioka 

r-Process

N=

50

Z=

N=

28

Z=

50

Sn Te

N=

82

Z=

82, N

=12

6

Th U Bi

1st p

eak

2nd

peak

3rd

peak

Neutron-rich Ejecta ⇒ n-capture>β decay

2014.3.28 重力波源と対応天体 by K. Ioka

Page 8: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

Macro/Kilo-nova Radioactivity (r-process → β-decay, fission, neutron)

f: fraction of rest mass released as heat

M=10-2M

v=c/3 optically thin

  超新星-like   Duration ∝(M/v)1/2

  T∝(f2/Mv)1/8 ~ IR-Opt

  f~3x10-6 ⇒ 暗い超新星

Li & Paczynski 98 Kulkarni 05

~Supernova (SN)

2014.3.28 重力波源と対応天体 by K. Ioka 8

Page 9: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

Discovery of Macro/Kilo-nova?

9

Tanvir+ 13 Berger+ 13 Ejecta with

~0.01-0.1M ~0.1-0.3c ~1050-1052erg Radioactivity f~εr/mc2~3e-6

HST

L~1041erg/s @z~0.356 22-23 mag if @200Mpc ~10 days

X Opt

NearIR

t-2.7

Swift

2014.3.28 重力波源と対応天体 by K. Ioka

Page 10: (KEK, Sokendai) - ICRR...General relativity Cosmic ray r-process elements Hadron physics Merger of 1.3-1.4 M sun NS: EOS=APR4; stiff but relatively soft ρ (g/cm3) Orbital plane X-Z

2014.3.28 重力波源と対応天体 by K. Ioka 10

? ? ? Gravitational wave X-ray IR-Opt Radio

!!!

? ? Neutrino Gamma-ray Gravitational Wave Sources

Counterparts to GW

  Short GRB origin   Confident GW detection   Parameter reduction   GW Astronomy, Cosmology   General relativity   Cosmic ray   r-process elements   Hadron physics