Gravitational-wave astronomy and astrophysics

Chunglee Kim; Hee Suk Cho; Gungwon Kang; Hyung Won Lee; Chang Hwan Lee; Hyun Kyu Lee

doi:10.3938/NPSM.66.293

Gravitational-wave astronomy and astrophysics

Chunglee Kim, Hee Suk Cho, Gungwon Kang, Hyung Won Lee, Chang Hwan Lee, Hyun Kyu Lee

Department of Physics

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

Abstract

On September 14, 2015, gravitational waves (GWs) were detected by the LIGO (Laser Interferometer gravitational-wave observatory) detectors in USA. The event (GW150914) is originated from a coalescence of two black holes (BHs) located at 13 billion light years away from the Earth. This is the first direct detection of GWs and the first observation of a BH-BH binary. We overview astrophysical sources that can be detected by km-scale laser interferometers on Earth, summarize astrophysical implications of GW150914, and discuss how to explore a Universe with GWs.

Original language	English
Pages (from-to)	293-303
Number of pages	11
Journal	New Physics: Sae Mulli
Volume	66
Issue number	3
DOIs	https://doi.org/10.3938/NPSM.66.293
State	Published - Mar 2016

Bibliographical note

Funding Information:
NRF-2013R1A1A206 0677, NRF-2015R1D1A1A01060210, NRF-2015R1A2A2 A01004238, (APCTP), KISTI GSDC.

Keywords

Astrophysics
Bayesian inference
Black holes
Gamma-ray bursts
Gravitational waves
Neutron stars
Statistical analysis
Supernovae

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10.3938/NPSM.66.293

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title = "Gravitational-wave astronomy and astrophysics",

abstract = "On September 14, 2015, gravitational waves (GWs) were detected by the LIGO (Laser Interferometer gravitational-wave observatory) detectors in USA. The event (GW150914) is originated from a coalescence of two black holes (BHs) located at 13 billion light years away from the Earth. This is the first direct detection of GWs and the first observation of a BH-BH binary. We overview astrophysical sources that can be detected by km-scale laser interferometers on Earth, summarize astrophysical implications of GW150914, and discuss how to explore a Universe with GWs.",

keywords = "Astrophysics, Bayesian inference, Black holes, Gamma-ray bursts, Gravitational waves, Neutron stars, Statistical analysis, Supernovae",

author = "Chunglee Kim and Cho, {Hee Suk} and Gungwon Kang and Lee, {Hyung Won} and Lee, {Chang Hwan} and Lee, {Hyun Kyu}",

note = "Funding Information: NRF-2013R1A1A206 0677, NRF-2015R1D1A1A01060210, NRF-2015R1A2A2 A01004238, (APCTP), KISTI GSDC.",

year = "2016",

month = mar,

doi = "10.3938/NPSM.66.293",

language = "English",

volume = "66",

pages = "293--303",

journal = "New Physics: Sae Mulli",

issn = "0374-4914",

publisher = "Korean Physical Society",

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T1 - Gravitational-wave astronomy and astrophysics

AU - Kim, Chunglee

AU - Cho, Hee Suk

AU - Kang, Gungwon

AU - Lee, Hyung Won

AU - Lee, Chang Hwan

AU - Lee, Hyun Kyu

N1 - Funding Information: NRF-2013R1A1A206 0677, NRF-2015R1D1A1A01060210, NRF-2015R1A2A2 A01004238, (APCTP), KISTI GSDC.

PY - 2016/3

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N2 - On September 14, 2015, gravitational waves (GWs) were detected by the LIGO (Laser Interferometer gravitational-wave observatory) detectors in USA. The event (GW150914) is originated from a coalescence of two black holes (BHs) located at 13 billion light years away from the Earth. This is the first direct detection of GWs and the first observation of a BH-BH binary. We overview astrophysical sources that can be detected by km-scale laser interferometers on Earth, summarize astrophysical implications of GW150914, and discuss how to explore a Universe with GWs.

AB - On September 14, 2015, gravitational waves (GWs) were detected by the LIGO (Laser Interferometer gravitational-wave observatory) detectors in USA. The event (GW150914) is originated from a coalescence of two black holes (BHs) located at 13 billion light years away from the Earth. This is the first direct detection of GWs and the first observation of a BH-BH binary. We overview astrophysical sources that can be detected by km-scale laser interferometers on Earth, summarize astrophysical implications of GW150914, and discuss how to explore a Universe with GWs.

KW - Astrophysics

KW - Bayesian inference

KW - Black holes

KW - Gamma-ray bursts

KW - Gravitational waves

KW - Neutron stars

KW - Statistical analysis

KW - Supernovae

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U2 - 10.3938/NPSM.66.293

DO - 10.3938/NPSM.66.293

M3 - Article

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VL - 66

SP - 293

EP - 303

JO - New Physics: Sae Mulli

JF - New Physics: Sae Mulli

IS - 3

ER -

Gravitational-wave astronomy and astrophysics

Abstract

Bibliographical note

Keywords

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