|  Gravitational-Radiation Analysis | 
In General > s.a. gravitational-wave sources;
  interferometers and space-based detectors.
  @ General references: Finn gq/97-proc [statistical inference];
    10th Workshop CQG(06)#19;
    Robinson et al PRD(08)-a0804 [network data and coincidences];
    Littenberg & Cornish PRD(09)-a0902,
    PRD(10)-a1008 [Bayesian approach];
    Jaranowski & Królak 09;
    Yunes & Pretorius PRD(09)-a0909 [theoretical bias and post-Einsteinian framework];
    GWDAW13 CQG(09)#20;
    Fairhurst CQG(11)-a1010 [source localization];
    Röver et al a1103-proc,
    Gholami a1109 [Bayesian versus frequentist upper limits];
    Jaranowski & Królak LRR(12);
    Cornish & Romano PRD(13) [unified description of template-based and cross-correlation analysis];
    Burko TPT(17)-a1602 [in the introductory physics lab];
    > s.a. interferometers.
  @ Search for continuous waves: Prix & Shaltev PRD(12)-a1201;
    Astone et al PRD(14)-a1403 [narrow-band searches];
    Zhu et al PRD(16)-a1608,
    Ming et al PRD(19)-a1903 [Einstein@home];
    Riles MPLA(17)-a1712.
  @ Search for bursts: Lynch et al PRD(17)-a1511 [information-theoretic approach].
  @ Search for unmodeled sources: 
    Searle et al CQG(09);
    Bacon et al a1805;
    Antelis & Moreno a1807 [template-free independent search].
  @ Waveforms and templates: Lindblom et al PRD(10)-a1008 [accuracy standards for waveforms];
    CQG(11)-a1102 [post-newtonian/numerical waveforms and parameter estimation];
    Sampson et al PRD(14)-a1311 [the trouble with templates];
    Field et al PRX(14) [method to quickly and accurately predict waveforms];
    Moore & Gair PRL(14)-a1412 [uncertainties in parameter estimates];
    Ashtekar et al a1906 [constraints on waveforms].
  @ With scalar waves: Maggiore & Nicolis PRD(00)gq/99;
    Fucito gq/00-ln;
    Bellucci et al PLA(01)ht;
    Babusci et al PRD(01)gq [stochastic background];
    Capozziello & Corda IJMPD(06) [scalar-tensor waves, production and detection];
    Corda gq/06-wd [interferometer response].
And Other Types of Astronomy > s.a. astronomy
  [multimessenger astronomy]; gravitational-wave propagation.
  @ And the cmb: Seljak & Zaldarriaga PRL(97)ap/96 [polarization];
    Durrer & Kahniashvili HPA(98)ap/97;
    > s.a. gravitational-wave background.
  @ Other electromagnetic waves / photons:
    Bramson PRS(06);
    Bloom et al a0902-rp [Astro2010];
    Owen CQG(09)-a0904-proc.
  @ Other types: Braginsky et al PLA(06) [cosmic-ray noise];
    Van Elewyck et al IJMPD(09)-a0906-proc [joint search with neutrino telescopes];
    Chia a2012-PhD [particle physics].
Gravitational-Wave Background > s.a. background;
  gravitational-wave detection [including astrometric effects].
  * Approach: For many
    sources, where the signal cannot be modeled like for single ones, the
    approach to the search of gravitational-wave signals is based on looking
    for cross-correlations between different detectors; Eventually one would
    like to produce a map similar to the cmb anisotropy maps.
  @ General references:
    Allen gq/96-proc [general],
    & Romano PRD(99)gq/97,
    Christensen PRD(97) [strategies];
    Vitale et al PRD(97) [bar detector];
    Lesgourgues et al A&A(00)gq/99;
    Zibin et al ap/99-GRF [and cmb];
    Amelino-Camelia gq/00 [from quantum spacetime];
    Cornish CQG(01)ap [deconvolution];
    Finn & Lazzarini PRD(01)gq [noise];
    Lazzarini et al PRD(04);
    Malaspinas & Sturani CQG(06) [correlating n detectors];
    Chiba et al PRD(07)-a0705 [search templates];
    Cella et al CQG(07)-a0704 [prospects, Virgo and LSC];
    Reynaud et al PRD(08) [using ultrastable-clock comparisons];
    Izzo et al a0902-proc [with FastICA];
    Finn et al PRD(09);
    news space(09)aug [none seen so far].
  @ Observation, pulsar timing:
    Jenet et al ApJL(05)ap;
    van Haasteren et al MNRAS(09)-a0809;
    Anholm et al PRD(09) [strategies];
    van Haasteren et al MNRAS(11)-a1103;
    Powell & Tasinato a1910 [probing a stationary non-Gaussian background];
    > s.a. pulsars.
  @ Observational bounds: LIGO PRL(05)ap [69–156 Hz];
    Abbott et LIGO PRD(07)ap;
    Abbott et LIGO+ALLEGRO PRD(07)gq [cross-correlation];
    Akutsu et al PRL(08) [100 MHz];
    Zhao & Grishchuk PRD(10)-a1009,
    Zhao et al PRD(10) [relic gravitational waves and cmb data];
    Abadie et LIGO+Virgo PRD(11)-a1112 [600–1000 Hz].
  @ From inflation:
    Turner PRD(97);
    Smith et al PRD(06);
    Cooray MPLA(05);
    Chongchitnan & Efstathiou PRD(06);
    Ni IJMPD(09);
    Jinno et al JCAP(14)-a1406 [with future space-based detectors].
  @ Polarization: Seto PRL(06)ap [circular polarization, prospects];
    Seto & Taruya PRL(07)-a0707 [Stokes parameters from laser interferometers].
  @ Non-Gaussian background: Allen et al PRD(02)gq/01;
    Martellini & Regimbau PRD(14).
  @ Analysis techniques: Whelan et al CQG(05)gq-proc [LIGO-ALLEGRO cross-correlations];
    Seto PRD(06) [correlation analysis];
    Himemoto et al PRD(07) [with non-Gaussian noise];
    Adams & Cornish PRD(10)-a1002 [distinguishing from instrument noise];
    Seto & Kyutoku PRD(12)-a1206 [parameter estimation, geometric approach];
    Adams & Cornish PRD(14)-a1307 [galactic foreground and instrument noise];
    Cornish & Romano PRD(15)-a1505 [definition of stochastic signal];
    Davies et al CQG(16)-a1603 [targeted spectral interpolation algorithm].
  @ Codes, templates: Whelan et al CQG(02)gq/01-proc;
    Bose PRD(05).
 
  @ With interferometers:
    Christensen PRD(92);
    Flanagan PRD(93)ap [LIGO sensitivity];
    Melissinos & Butler gq/05 [single detector];
    Kudoh et al PRD(06)gq/05;
    Corbin & Cornish CQG(06)gq/05 [with BBO];
    Corda APP(07)-a0806 [and linearized solutions];
    Thrane et al PRD(09)-a0910 [probing the anisotropies];
    Thrane & Romano PRD(13) [sensitivity curves];
    Romano et al a1505 [phase-coherent mapping];
    Smith & Thrane PRX(18) [optimal search].
  @ With LISA:
    Tinto et al PRD(01) [vs noise];
    Cornish PRD(02)gq/01;
    Ignatiev et al MNRAS(01)ap [from binaries];
    Timpano et al PRD(06);
    Flauger et al a2009.
  @ Other wave background: Gasperini & Ungarelli PRD(01)gq [scalar].
Specific Types of Sources and Related Effects > s.a. gravitational-wave
  sources and propagation; wave phenomena.
  * Compact binaries: For
    low masses, the best chances are by searching for the inspiral signal;
    For masses above 100 MSun,
    looking for the ringdown signal is more effective; For single binary
    sources, the approach to the search of gravitational-wave signals is
    based on matched filtering, in which segments of data are correlated with
    templates corresponding to different sets of binary system parameters.
  @ Compact binaries: Ghosh et al PRD(16)-a1505 [parameter estimation];
    Testa & Pani a1806 [post-merger gravitational-wave echoes].
  @ Compact binaries, templates: Ajith et al PRD(05) [PN test mass in Schwarzschild spacetime];
    Babak et al CQG(06);
    Porter PRD(07)-a0706 [comparable-mass black hole + black hole];
    Buonanno et al PRD(07)-a0706 [non-spinning binary black holes].
  @ Compact binaries, search: Dhurandhar & Vecchio gq/99-proc [computational cost];
    Meliani et al A&A-ap/00,
    Finn & Thorne PRD(00)gq [LISA];
    Hughes PRD(02) [algorithm];
    Brown et al CQG(04)-a0705 [LIGO S1 and S2];
    Mitra et al PRD(05) [efficiency];
    Jones PhD(08)-a1002;
    Mandel et al MNRAS(15)-a1503 [distinguishing types of compact binaries];
    Capano et al PRD(16)-a1602 [non-precessing, spinning binaries].
  @ Single compact objects: Faber et al PRL(02)ap [neutron stars, equation of state and size];
    Hughes a1002-proc [black holes].
  @ Cosmology: Schutz ESO(02)gq/01;
    Taylor et al PRD(12)-a1108 [with advanced detectors];
    > s.a. cosmological acceleration;
      observational cosmology.
  @ Early-universe cosmology:
    Maggiore PRP(00);
    Alizadeh & Hirata PRD(12)-a1201 [cross-correlation of the galaxy distribution with the CMB polarization].
  @ GRBs: Finn et al PRD(99)gq [GRBs];
    news pw(08)jan [no detection by LIGO].
And Other Theories of Gravity > s.a. astrophysical tests;
  gravitational radiation [theory]; gravitational-wave;
  space-based detectors [tests].
  * Idea: Some
    predict 3 transversal modes, and 3 longitudinal ones.
  @ General references: Yunes et al PRD(16)-a1603 [GW150914 and theoretical physics];
    Arzano & Calcagni PRD(16)-a1604 [quantum spacetime];
    Chamberlain & Yunes PRD(17)-a1704 [with future detectors];
    Pang et al a2003 [searches for alternative polarizations].
  @ Massive graviton: Loskutov TMP(96);
    Will & Yunes CQG(04)gq [and LISA];
    Corda APP(07)-a0811 [from bimetric theory].
  @ Chern-Simons-modified gravity: Sopuerta & Yunes proc(11)-a1010;
    Cañizares et al PRD(12)-a1205 [extreme-mass-ratio binaries];
    > s.a. chern-simons theory.
  @ Other higher-order gravity: Ananda et al PRD(08)-a0708 [cosmological];
    Desai et al PRD(08)-a0805;
    Capozziello et al PLB(08) [massive, and detection with LISA];
    De Laurentis & Capozziello APP(11)-a1104 [quadrupolar radiation];
    Yang et al JCAP(11)-a1106 [with non-zero background curvature];
    > s.a. phenomenology.
  @ Other types of theories:
    Canfora et al IJGMP(06) [spin-1];
    Nelson et al PRD(10)-a1005 [spectral-triple approach to non-commutative geometry];
    Blas & Sanctuary PRD(11)-a1105 [Hořava gravity];
    Chicone & Mashhoon PRD(13)-a1211 [non-local];
    > s.a. bimetric gravity; brans-dicke
      theory; hořava gravity; Relativistic Theory of
      Gravity; scalar-tensor theory; TeVeS.
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