SLIDE 1
“Spacetime tells matter how to move; matter tells spacetime how to curve.” — John Wheeler
3
General Relativity Spacetime tells matter how to move; matter tells - - PowerPoint PPT Presentation
General Relativity Spacetime tells matter how to move; matter tells - - PowerPoint PPT Presentation
General Relativity Spacetime tells matter how to move; matter tells spacetime how to curve. John Wheeler 3 Gravitational Waves Strain on spacetime. Generated by time-varying quadrupole moment. Propagate at speed of light. Unimpeded
SLIDE 2
SLIDE 3
4
Strain on spacetime. Generated by time-varying quadrupole moment. Propagate at speed of light. Unimpeded by matter.
Gravitational Waves
SLIDE 4
credit: wikipedia
0.000000000000000000001
SLIDE 5
Hanford, WA Livingston, LA Pisa, Italy
LIGO-Virgo Network
6
SLIDE 6
7
SLIDE 7
8
SLIDE 8
9
O1 BBH: Abbott et al. (2016) PRX 6, 041015 GW170104: Abbott et al. (2017) PRL 118, 221101 GW170608: Abbott et al. (2017) ApJL 851 L35 GW170814: Abbot et al. (2017) PRL 119, 141101
SLIDE 9
11
Isolated (“Field”) Formation
Belczynski et al. (2016)
SLIDE 10
12
credit: Carl Rodriguez
Dynamical Formation
Rodriguez et al. (2016)
SLIDE 11
13
prior
Black Hole Spins
SLIDE 12
13
GW150914
BH spin not extremal
Abbott et al. (2016):
PRX 6, 041015
Black Hole Spins
SLIDE 13
13
LVT151012
Abbott et al. (2016):
PRX 6, 041015
Black Hole Spins
SLIDE 14
13
GW151226
At least one spinning BH
Abbott et al. (2016):
PRX 6, 041015
Black Hole Spins
SLIDE 15
13
GW151226
At least one spinning BH
Abbott et al. (2016):
PRX 6, 041015
Black Hole Spins
χeff = m1a1 cos θ1 + m2a2 cos θ2 m1 + m2
<latexit sha1_base64="EHdcnmso4rxYQenBhRrmLNfThYw=">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</latexit><latexit sha1_base64="EHdcnmso4rxYQenBhRrmLNfThYw=">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</latexit><latexit sha1_base64="EHdcnmso4rxYQenBhRrmLNfThYw=">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</latexit><latexit sha1_base64="EHdcnmso4rxYQenBhRrmLNfThYw=">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</latexit> SLIDE 16
O1 + (some of) O2
15
Farr et al (2017): arXiv:1709.07896
SLIDE 17
16
Simple Population Model
SLIDE 18
Current Results
17
0.0 0.2 0.4 0.6 0.8 1.0 0.00 0.25 0.50 0.75 1.00 1.25 1.50 1.75
fraction of informative events w/ χeff > 0 (ρ) fraction of informative events (α)
marginal posterior density
SLIDE 19
Current Results
17
0.0 0.2 0.4 0.6 0.8 1.0 0.00 0.25 0.50 0.75 1.00 1.25 1.50 1.75
fraction of informative events w/ χeff > 0 (ρ) fraction of informative events (α)
marginal posterior density
Dynamical
SLIDE 20
Current Results
17
0.0 0.2 0.4 0.6 0.8 1.0 0.00 0.25 0.50 0.75 1.00 1.25 1.50 1.75
fraction of informative events w/ χeff > 0 (ρ) fraction of informative events (α)
marginal posterior density
Dynamical Field
SLIDE 21
Spin Magnitudes
18
0.0 0.2 0.4 0.6 0.8 1.0
a
0.0 0.5 1.0 1.5 2.0 2.5 3.0
p(a)
0.0 0.2 0.4 0.6 0.8 1.0
a
0.0 0.5 1.0 1.5 2.0 2.5
p(a)
0.0 0.2 0.4 0.6 0.8 1.0
a
0.0 0.5 1.0 1.5 2.0 2.5 3.0
p(a)
Aligned Isotropic
SLIDE 22
19 19
SLIDE 23
GW170817
20
SLIDE 24
21
Abbott et al. (2017) arXiv:1710.05833
SLIDE 25
21
Abbott et al. (2017) arXiv:1710.05833
SLIDE 26
22
- 100 -50
50
GW γ-ray X-ray UV Optical IR Radio
10-2 t-tc (s) t-tc (days) 10-1 100 101
LIGO, Virgo Fermi, INTEGRAL, Astrosat, IPN, Insight-HXMT, Swift, AGILE, CALET, H.E.S.S., HAWC, Konus-Wind Swift, MAXI/GSC, NuSTAR, Chandra, INTEGRAL Swift, HST Swope, DECam, DLT40, REM-ROS2, HST, Las Cumbres, SkyMapper, VISTA, MASTER, Magellan, Subaru, Pan-STARRS1, HCT, TZAC, LSGT, T17, Gemini-South, NTT, GROND, SOAR, ESO-VLT, KMTNet, ESO-VST, VIRT, SALT, CHILESCOPE, TOROS, BOOTES-5, Zadko, iTelescope.Net, AAT, Pi of the Sky, AST3-2, ATLAS, Danish Tel, DFN, T80S, EABA REM-ROS2, VISTA, Gemini-South, 2MASS,Spitzer, NTT, GROND, SOAR, NOT, ESO-VLT, Kanata Telescope, HST ATCA, VLA, ASKAP, VLBA, GMRT, MWA, LOFAR, LWA, ALMA, OVRO, EVN, e-MERLIN, MeerKAT, Parkes, SRT, Effelsberg SALT ESO-NTT SOAR ESO-VLT 7000o 4000o t-tc (days) 1.2 1.4 2.4wavelength (nm) normalized Fλ 400 600 1000 2000
INTEGRAL/SPI-ACS Fermi/GBMt-tc (s)
- 12 -10 -8 -6 -4 -2 0 2 4 6
counts/s (arb. scale) frequency (Hz) 500 400 300 200 100 50
LIGO - Virgo Chandra 9d J VLA 16.4d Radio Las Cumbres 11.57h w DECam 11.40h iz MASTER 11.31h W VISTA 11.24h YJKs X-ray DLT40 11.08h h 1M2H Swope 10.86h i
Talking Picture
Abbott et al. (2017) arXiv:1710.05833
SLIDE 27
Masses
23
Abbott et al. (2018) arXiv:1805.11579
SLIDE 28
Known NSs
24
Opel and Freire (2016)
SLIDE 29
25
- 100 -50
50
GW γ-ray X-ray UV Optical IR Radio
10-2 t-tc (s) t-tc (days) 10-1 100 101
LIGO, Virgo Fermi, INTEGRAL, Astrosat, IPN, Insight-HXMT, Swift, AGILE, CALET, H.E.S.S., HAWC, Konus-Wind Swift, MAXI/GSC, NuSTAR, Chandra, INTEGRAL Swift, HST Swope, DECam, DLT40, REM-ROS2, HST, Las Cumbres, SkyMapper, VISTA, MASTER, Magellan, Subaru, Pan-STARRS1, HCT, TZAC, LSGT, T17, Gemini-South, NTT, GROND, SOAR, ESO-VLT, KMTNet, ESO-VST, VIRT, SALT, CHILESCOPE, TOROS, BOOTES-5, Zadko, iTelescope.Net, AAT, Pi of the Sky, AST3-2, ATLAS, Danish Tel, DFN, T80S, EABA REM-ROS2, VISTA, Gemini-South, 2MASS,Spitzer, NTT, GROND, SOAR, NOT, ESO-VLT, Kanata Telescope, HST ATCA, VLA, ASKAP, VLBA, GMRT, MWA, LOFAR, LWA, ALMA, OVRO, EVN, e-MERLIN, MeerKAT, Parkes, SRT, Effelsberg SALT ESO-NTT SOAR ESO-VLT 7000o 4000o t-tc (days) 1.2 1.4 2.4wavelength (nm) normalized Fλ 400 600 1000 2000
INTEGRAL/SPI-ACS Fermi/GBMt-tc (s)
- 12 -10 -8 -6 -4 -2 0 2 4 6
counts/s (arb. scale) frequency (Hz) 500 400 300 200 100 50
LIGO - Virgo Chandra 9d J VLA 16.4d Radio Las Cumbres 11.57h w DECam 11.40h iz MASTER 11.31h W VISTA 11.24h YJKs X-ray DLT40 11.08h h 1M2H Swope 10.86h i
Talking Picture
Abbott et al. (2017) arXiv:1710.05833
SLIDE 30
EM Counterparts to BNS
26
credit: Berger (2014)
SLIDE 31
GRB and afterglow
27
credit: NASA's Goddard Space Flight Center
SLIDE 32
GRB and afterglow
27
credit: NASA's Goddard Space Flight Center
credit: Lijnis Nelemans
SLIDE 33
Kilonova
28
SLIDE 34
29
SLIDE 35
30
credit:Open Kilonova Catalog Cowperthwaite et al. (2017)
SLIDE 36
31
SLIDE 37
32
SLIDE 38
Standard Siren
33
Abbott et al. (2017) arXiv:1710.05835
SLIDE 39
Speed of Gravity
34
temporal offset: 1.74 ± 0.05 s
−3 × 10−15 ≤ ∆v νEM ≥ +7 × 10−16
Abbott et al. (2017) arXiv:1710.05834
SLIDE 40
Conclusions
35