| unchecked | Instead, by plugging in purposeful "tweaks" of the sparse subnetwork architecture or its training recipe, its retraining can be significantly improved than the default, especially at high sparsity levels.arXiv 2101.03255 · ext:ffac493eeccc52fc | 0.55 | 1.00 | 0 | 0 | Computer Science | 7 Oct 2026 |
| unchecked | Yet, at one-week lead times, its skill is only about one day behind both SOTA ML forecast models and the SOTA numerical weather prediction model from the European Centre for Medium-Range Weather Forecasts.arXiv 2311.06253 · ext:05b1dcf44cd5d678 | 0.55 | 1.00 | 0 | 0 | Earth and Planetary Sciences | 7 Oct 2026 |
| unchecked | Based on an in-depth analysis, we additionally find that sparsity is crucial to prevent both 1) interference between the fine-tunings to be composed and 2) overfitting.arXiv 2110.07560 · ext:23034202fae19cc9 | 0.55 | 1.00 | 0 | 0 | Computer Science | 6 Oct 2026 |
| unchecked | Most importantly, it outperforms adapters in zero-shot cross-lingual transfer by a large margin in a series of multilingual benchmarks, including Universal Dependencies, MasakhaNER, and AmericasNLI.arXiv 2110.07560 · ext:61eee0f1fdf51273 | 0.55 | 1.00 | 0 | 0 | Computer Science | 6 Oct 2026 |
| unchecked | Our experiments on the GLUE benchmark show that the super tickets improve single task fine-tuning by $0.9$ points on BERT-base and $1.0$ points on BERT-large, in terms of task-average score.arXiv 2105.12002 · ext:bd927c9ba66c02f0 | 0.55 | 1.00 | 0 | 0 | Computer Science | 6 Oct 2026 |
| unchecked | In particular, we observe a phase transition phenomenon: As the compression ratio increases, generalization performance of the winning tickets first improves then deteriorates after a certain threshold.arXiv 2105.12002 · ext:419b5f42829a19e6 | 0.55 | 1.00 | 0 | 0 | Computer Science | 6 Oct 2026 |
| supported | We propose an algorithm requiring 48 multiplications that uses only rational coefficients, thereby removing the requirement for complex-number arithmetic, and making this algorithm valid over any ring except those of characteristic 2.arXiv 2506.13242 · ext:df36d5075eea1f70 | 0.71 | 1.00 | 1 | 0 | Computer Science | 6 Oct 2026 |
| unchecked | Moreover, inside each cluster most variables are frozen, i.e., take only one value.arXiv cs/0611052 · ext:2771adb38b08b3bb | 0.55 | 1.00 | 0 | 0 | Computer Science | 6 Oct 2026 |
| unchecked | For example, we prove that if $H$ has bounded degree, then $ER(H)$ is polynomial in $|V(H)|$ if $H$ is bipartite, but exponential in general.arXiv 2410.08644 · conceptual · ext:ff4bc702bde9cacc | 0.55 | 0.00 | 0 | 0 | Mathematics | 11 Oct 2026 |
| unchecked | We also obtain a polynomial regularity lemma for $r$-uniform algebraic hypergraphs that are defined by a single polynomial, that might be of independent interest.arXiv 2103.05618 · conceptual · ext:b82fb04d0b565112 | 0.55 | 0.00 | 0 | 0 | Mathematics | 11 Oct 2026 |
| unchecked | We extend this result by showing that such $G$ contains either a clique or an independent set of size $N^{Ω(1/ndm)}$ and prove similar results for algebraic hypergraphs of constant complexity.arXiv 2103.05618 · ext:3af7f54b39d99f6e | 0.55 | 0.00 | 0 | 0 | Mathematics | 11 Oct 2026 |
| unchecked | We prove that there exists $ε>0$ such that for every graph $G$ with $|V(G)|\ge 2$ not containing $T$ as an induced subgraph, either some vertex has at least $ε|V(G)|$ neighbours, or there are two disjoint sets of vertices $A,B$, both of ca…arXiv 1810.00811 · ext:887a7f6a88f3272e | 0.55 | 0.00 | 0 | 0 | Mathematics | 11 Oct 2026 |
| unchecked | We show analytically that grid-based planning permits shortcuts through unvisited locations and generalizes local transitions to long-range paths.arXiv 2507.02064 · conceptual · ext:72da2d741e6a7a56 | 0.55 | 0.00 | 0 | 0 | Neuroscience | 11 Oct 2026 |
| unchecked | Finally, these datasets provide a structural context for interpreting disease mutations and reveal coiled-coil regions as major enablers of quaternary structure evolution in human.DOI 10.1016/j.cell.2024.01.022 · conceptual · ext:e0a7e913d31c0ccf | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Our results suggest that approximately 45% of an archaeal proteome and a bacterial proteome and 20% of two eukaryotic proteomes form homomers.DOI 10.1016/j.cell.2024.01.022 · ext:4e9e8664c398d41d | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We find that complexes containing symmetry are accurately assembled, while asymmetrical complexes remain challenging.DOI 10.1038/s41467-022-33729-4 · ext:57a058d62519c34c | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We create a scoring function, mpDockQ, that can distinguish if assemblies are complete and predict their accuracy.DOI 10.1038/s41467-022-33729-4 · ext:35e94954b61f2c62 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We assemble 91 out of 175 complexes with 10–30 chains from predicted subcomponents using Monte Carlo tree search, with a median TM-score of 0.51.DOI 10.1038/s41467-022-33729-4 · ext:eb56711c48e746b3 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | These firing fields possessed spatial periodicity similar to a triangular tiling with a corresponding well-defined hexagonal structure in the spatial autocorrelation.DOI 10.1038/nature11587 · ext:e0b64bfaf86113c8 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We found that a simple neural network can effectively correct the grid code.DOI 10.1038/nn.2901 · ext:5b788fa626722a32 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | In particular, the representational accuracy attained by grid cells over the coding range was in a qualitatively different class from what is possible with observed sensory and motor population codes.DOI 10.1038/nn.2901 · ext:87ffb26ebb462f56 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We find Automatminer achieves the best performance on 8 of 13 tasks in the benchmark.OpenAlex W3100220443 · ext:67843e03d33c028c | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | When the Kohn-Sham band-gap by GGA (PBE) or modified Becke-Johnson (mBJ) is used as a single predictor, OLSR model predicts the G0W0 band-gap of a randomly selected test data with the root mean square error (RMSE) of 0.54 eV.arXiv 1509.00973 · ext:14f375cf7b5cc935 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We performed such a large-scale search for new ternary oxides, discovering 209 new compounds with a limited computational budget.DOI 10.1021/cm100795d · ext:3438e3050cae8b00 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | However, the addition of analogs to Uranus and Neptune can have a minor negative effect on scattering efficiency through the transfer of angular momentum from the inner giant planets.arXiv 2506.08088 · ext:e14c17cb5d016543 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | The inclusion of a Saturn analog to the dynamical model produces a similar increase, highlighting the importance of multiple giant planets beyond the snow line.arXiv 2506.08088 · ext:c88ffa1a8c012b37 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | We show that increasing the eccentricity of a Jupiter analog from its present, near-circular, value to a moderate range (0.2-0.3) results in an order of magnitude increase in scattered material to the inner part of the system.arXiv 2506.08088 · ext:1bfff63da458bcbe | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | Here, we investigate the orbital distribution of the two color classes identified by Fraser et al. and find that the orbital inclinations of the brightIR class objects are correlated with their optical colors.arXiv 2206.04096 · ext:a26a060f04ba9c5c | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | We conclude that the observed large inclination dispersion of Kuiper belt objects does not require Neptune's migration to be slow; planetary migration with e-folding timescales of 5, 10, 30, and 50 Myr can all yield inclination dispersions…arXiv 1906.00023 · ext:ec0435855a302907 | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | We do not find a consistent relationship between the degree of test particle inclination excitation and e-folding planet migration timescales in the range 5-50 Myr.arXiv 1906.00023 · ext:61e7844fbbe2e570 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | The findings reveal that after assimilating water vapor channels from the Advanced Geostationary Radiation Imager onboard Fengyun-4B, the errors in typhoon intensity forecasts are reduced.arXiv 2408.12630 · ext:e587e60b32be773a | 0.55 | 0.00 | 0 | 0 | Earth and Planetary Sciences | 11 Oct 2026 |
| unchecked | The results show that forecasts from the Pangu_SP experiment obviously outperform those by using the Global Forecast System as the initial field (GFS_INIT) and from the Integrated Forecasting System of the European Centre for Medium-Range…arXiv 2408.12630 · ext:be94aa3af7dc88b5 | 0.55 | 0.00 | 0 | 0 | Earth and Planetary Sciences | 11 Oct 2026 |
| unchecked | The generalized second law is satisfied for all models over $0 \le z \le 1$, while the Hessian analysis reveals a transient instability at the phase transition; however, the late time thermodynamic stability is model dependent, with CPL an…arXiv 2608.30500 · ext:477ee04fa53fc76c | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | The required characteristics are identified as phantom dark energy at high redshift, crossing $w=-1$ at lower redshift.arXiv 2603.15422 · ext:a1c909fd195ec685 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | In coplanar encounters, the disk remains largely flattened, whereas polar flybys redistribute angular momentum vertically, producing nearly isotropic outer populations that resemble an emerging Oort cloud.arXiv 2510.23653 · ext:f6b6cd1223e90400 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | We find that compact disks primarily form Kuiper belt and scattered disk-like populations through planet-disk interactions, while extended disks are more strongly shaped by stellar encounters, producing Oort cloud-like structures and inter…arXiv 2510.23653 · ext:ee75ccbc909fc5fd | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | The disk mass inferred from this work, M_disk=14-28 M_Earth, is consistent with the mass deduced from recent dynamical simulations of the planetary instability.arXiv 1303.2900 · ext:d5251ae107d4d55d | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | We further note that our EFTBOSS analysis indicates a slight deviation of the BAO scale parameter (at $1.8 σ$) from its $Λ$CDM value, caused by the small scales of the bispectrum.arXiv 2602.21733 · ext:7027a07852342224 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | The corresponding EFT uncertainties are about a factor of $\sim2$ smaller than those reported in \citep{2025JCAP...09..053I}, which combined DESI full-shape and BAO measurements with DES-SN5YR and CMB data.arXiv 2606.10597 · ext:fd69561b8db27720 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | For the $(μ_0,η_0)$ case we find $μ_0=0.06^{+0.17}_{-0.23}$ and $η_0=-0.03^{+0.36}_{-0.46}$; relative to $Σ_8+fσ_8$, adding $\mathit{DR}$ improves the constraints on both parameters by a factor of $\sim1.5$.arXiv 2606.10597 · ext:eaa3bf3add20bd4e | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 11 Oct 2026 |
| unchecked | Results show that combining the best answers from different MLMs yielded an overall correct answer rate of 82.7% which is better than the 60.9% of ChatGPT.arXiv 2305.11991 · ext:836aed43b795e217 | 0.55 | 0.00 | 0 | 0 | Computer Science | 11 Oct 2026 |
| unchecked | The answer is that current technologies have NOT achieved universal intelligence and there remains a significant journey to undertake.arXiv 2408.12880 · conceptual · ext:3fdf686d68d0f37c | 0.55 | 0.00 | 0 | 0 | Computer Science | 10 Oct 2026 |
| unchecked | As a corollary, we obtain the corresponding bound for the oriented Ramsey number of a directed graph with $m$ edges.arXiv 2412.17599 · ext:ca47bff68d36bb0c | 0.55 | 0.00 | 0 | 0 | Mathematics | 10 Oct 2026 |
| unchecked | We prove that $r_<(G) \leq e^{10^9 \sqrt{m} (\log \log m)^{3/2}}$ for any such $G$, which is tight up to the $(\log \log m)^{3/2}$ factor in the exponent.arXiv 2412.17599 · ext:c0eec3963e328add | 0.55 | 0.00 | 0 | 0 | Mathematics | 10 Oct 2026 |
| unchecked | This model explains the oxidation and isotopic gradients within the inner Solar System within the context of a low-viscosity, magnetic wind-driven disk.arXiv 2601.04032 · ext:90f80c27659c3a27 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | Remaining unaccreted planetesimals can be implanted into the asteroid belt as the parent bodies of aubrites and non-carbonaceous iron meteorites, while the most reduced material is not implanted and thus unsampled in the meteorite collecti…arXiv 2601.04032 · ext:9bdac5ea501d5156 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | We show through a suite of N-body simulations that an inwardly sweeping secular resonance, caused by aerodynamic drag and perturbations from a mean-motion resonant Jupiter and Saturn, gathers the outer planetesimal disk into a narrow ring…arXiv 2601.04032 · ext:4b05000229f4ae80 | 0.55 | 0.00 | 2 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | We show that, at the very least, encounters between Saturn and one of the ice giants (Uranus or Neptune) need to have occurred, in order to reproduce the current secular properties of the giant planets, in particular the amplitude of the t…arXiv 0909.1886 · ext:0d23244d7dce1a35 | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | Using numerical simulations, we show that smooth migration of the giant planets through a planetesimal disk leads to an orbital architecture that is inconsistent with the current one: the resulting eccentricities and inclinations of their…arXiv 0909.1886 · ext:ced7c1da5712172d | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | However, if we include SH0ES $H_0$ data, which is in known strong tension with the CMB in flat $Λ$CDM, we find that the $H_0$ tension is recast in terms of a significantly negative curvature and suppressed growth of structures.arXiv 2604.06361 · ext:031841b1ca1e4826 | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 10 Oct 2026 |
