| general relativity | GR | 736 | 57 | 2.002238 | 1606.03952,1606.05590,etc |
| cosmic microwave background | CMB | 349 | 29 | 1.001968 | 1606.04906,1606.08449,etc |
| gravitational wave | GW | 948 | 28 | 2.005479 | 1606.03952,1606.04226,etc |
| black hole | BH | 1416 | 28 | 2.008872 | 1606.00147,1606.04246,etc |
| equation of state | EOS | 252 | 23 | 2.003005 | 1606.05965,1606.02523,etc |
| anti de sitter | AdS | 545 | 18 | 1.005125 | 1606.01250,1606.00100,etc |
| post newtonian | PN | 233 | 16 | 2.005171 | 1606.03117,1606.04226,etc |
| signal to noise ratio | SNR | 184 | 14 | 1.001441 | 1606.03952,1606.01011,etc |
| loop quantum gravity | LQG | 60 | 13 | 1.000742 | 1606.01250,1606.03271,etc |
| quantum field theory | QFT | 77 | 13 | 2.000538 | 1606.03481,1606.02268,etc |
| friedmann robertson walker | FRW | 60 | 13 | 1.001207 | 1606.00711,1606.09565,etc |
| cold dark matter | CDM | 96 | 11 | 2.001475 | 1606.05151,1606.05590,etc |
| dark energy | DE | 104 | 9 | 2.003976 | 1606.00147,1606.05965,etc |
| de sitter | dS | 560 | 9 | 2.005445 | 1606.01250,1606.02268,etc |
| laser interferometer gravitational wave observatory | LIGO | 53 | 8 | 1.001698 | 1606.07644,1606.00703,etc |
| dark matter | DM | 248 | 8 | 2.005775 | 1606.00147,1606.01248,etc |
| supermassive black hole | SMBH | 137 | 8 | 2.001874 | 1606.01248,1606.08879,etc |
| loop quantum cosmology | LQC | 178 | 8 | 1.003046 | 1606.03271,1606.03689,etc |
| arnowitt deser misner | ADM | 42 | 8 | 1.00068 | 1606.01801,1606.01215,etc |
| gamma ray burst | GRB | 172 | 7 | 2.004632 | 1606.08449,1606.02523,etc |
| null energy condition | NEC | 45 | 7 | 1.002629 | 1606.07733,1606.04879,etc |
| general theory of relativity | GR | 141 | 7 | 2.001953 | 1606.00618,1606.08879,etc |
| innermost stable circular orbit | ISCO | 35 | 7 | 1.000778 | 1606.08569,1606.08879,etc |
| effective one body | EOB | 80 | 6 | 2.003963 | 1606.03117,1606.01210,etc |
| bose einstein condensate | BEC | 68 | 6 | 2.0014 | 1606.09505,1606.05151,etc |
| infrared | IR | 72 | 6 | 1.001864 | 1606.01250,1606.03481,etc |
| neutron star | NS | 114 | 6 | 2.005355 | 1606.00458,1606.09090,etc |
| binary black hole | BBH | 113 | 6 | 2.007347 | 1606.00362,1606.01262,etc |
| quasi normal mode | QNM | 122 | 5 | 2.001803 | 1606.03952,1606.01132,etc |
| gravitational waves | GW | 212 | 5 | 2.012123 | 1606.07644,1606.00459,etc |
| ultraviolet | UV | 49 | 5 | 2.001718 | 1606.08449,1606.01250,etc |
| large scale structure | LSS | 15 | 5 | 1.000551 | 1606.01538,1606.00450,etc |
| power spectral density | PSD | 147 | 5 | 1.005992 | 1606.01011,1606.04226,etc |
| effective field theory | EFT | 77 | 5 | 1.001756 | 1606.02268,1606.06150,etc |
| conformal field theory | CFT | 47 | 5 | 1.0006 | 1606.07866,1606.02999,etc |
| cosmic microwave background radiation | CMB | 47 | 5 | 1.000724 | 1606.07665,1606.07333,etc |
| weak energy condition | WEC | 29 | 5 | 1.001094 | 1606.04358,1606.05295,etc |
| quasinormal mode | QNM | 93 | 4 | 2.002776 | 1606.00703,1606.01132,etc |
| advanced ligo | aLIGO | 11 | 4 | 1.000944 | 1606.01095,1606.00362,etc |
| reissner nordstr"om | RN | 76 | 4 | 2.002926 | 1606.00444,1606.07900,etc |
| wilkinson microwave anisotropy probe | WMAP | 9 | 4 | 1.000302 | 1606.06273,1606.09565,etc |
| cosmological constant | CC | 23 | 4 | 1.00114 | 1606.01887,1606.07045,etc |
| vacuum expectation value | VEV | 10 | 4 | 1.00073 | 1606.05515,1606.02826,etc |
| dirac born infeld | DBI | 27 | 4 | 2.000459 | 1606.08380,1606.02295,etc |
| friedmann lema^{i}tre robertson walker | FLRW | 11 | 4 | 1.001504 | 1606.04260,1606.06627,etc |
| globular cluster | GC | 65 | 4 | 1.005349 | 1606.01909,1606.07437,etc |
| born infeld | BI | 65 | 4 | 1.001474 | 1606.02733,1606.04364,etc |
| big bang nucleosynthesis | BBN | 19 | 3 | 1.000087 | 1606.06112,1606.05339,etc |
| friedmann lema^tre robertson walker | FLRW | 11 | 3 | 1.000613 | 1606.07733,1606.00659,etc |
| boyer lindquist | BL | 24 | 3 | 2.000296 | 1606.04246,1606.07725,etc |
| japan society for the promotion of science | JSPS | 5 | 3 | 1.000135 | 1606.00618,1606.06367,etc |
| two dimensional | 2D | 54 | 3 | 1.001791 | 1606.08192,1606.00693,etc |
| equations of motion | EOM | 14 | 3 | 2.000401 | 1606.02268,1606.02295,etc |
| numerical relativity | NR | 71 | 3 | 1.004022 | 1606.04226,1606.01210,etc |
| advanced virgo | AdV | 5 | 3 | 1.001257 | 1606.01095,1606.00362,etc |
| national research foundation | NRF | 3 | 3 | 1.00007 | 1606.09195,1606.06725,etc |
| cosmic background explorer | COBE | 5 | 3 | 1.000204 | 1606.06273,1606.09565,etc |
| fundamental research on matter | FOM | 3 | 3 | 1.000121 | 1606.06273,1606.03307,etc |
| gamma ray burst monitor | GBM | 23 | 3 | 2.001114 | 1606.00458,1606.08031,etc |
| friedmann lemaitre robertson walker | FLRW | 10 | 3 | 1.000325 | 1606.02999,1606.04846,etc |
| active galactic nucleus | AGN | 40 | 3 | 2.001715 | 1606.00844,1606.08879,etc |
| science and technology facilities council | STFC | 4 | 3 | 1.000115 | 1606.00844,1606.04856,etc |
| baryon acoustic oscillation | BAO | 29 | 3 | 2.001553 | 1606.00845,1606.07333,etc |
| tolman oppenheimer volkoff | TOV | 88 | 3 | 2.005091 | 1606.05515,1606.05106,etc |
| generalized second law | GSL | 20 | 3 | 1.000506 | 1606.04846,1606.04713,etc |
| strong energy condition | SEC | 21 | 3 | 1.002395 | 1606.02212,1606.04358,etc |
| mathisson papapetrou | MP | 37 | 3 | 2.003496 | 1606.09430,1606.00756,etc |
| parameterised post newtonian | PPN | 16 | 3 | 1.000345 | 1606.03282,1606.06627,etc |
| supernova | SN | 44 | 3 | 2.004567 | 1606.08462,1606.00454,etc |
| probability distribution function | PDF | 11 | 3 | 2.000099 | 1606.07437,1606.02530,etc |
| markov chain monte carlo | MCMC | 11 | 3 | 1.000314 | 1606.00672,1606.07725,etc |
| generalized uncertainty principle | GUP | 25 | 3 | 2.00198 | 1606.08295,1606.06635,etc |