| unchecked | Our analysis shows that Nash gravity provides a good fit to the data, yielding a slightly higher value for the Hubble constant, $H_0 = 69.32 \pm 0.72$ km/s/Mpc, compared to the $Λ$CDM model, thus offering a potential alleviation of the $H_…arXiv 2601.09429 · ext:7a00db0ef462b213 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | We find no significant hint for spatial curvature.arXiv 2405.17396 · ext:f65a20fb09d65fc0 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | Conversely, GPT-series models exhibited proficiency in lesion segmentation and anatomical localization but encountered difficulties in disease diagnosis and lesion detection.arXiv 2407.05758 · ext:5340cde13457cb84 | 0.55 | 1.00 | 0 | 0 | Computer Science | 10 Oct 2026 |
| unchecked | We train models with up to 6.7B parameters, and find differences to remain consistent at scale.arXiv 2205.11726 · ext:6621d5878346f865 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | We find that the optimal configuration is largely application-dependent (e.g., bidirectional attention is beneficial for fine-tuning and infilling, but harmful for next token prediction and zero-shot priming).arXiv 2205.11726 · ext:041967aef18bf6a8 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | For three of our resonant chains, about 1% of the final configurations pass the four criteria to fit the Solar System.arXiv 2406.20075 · ext:8ec3f522e46a3268 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | In a thin PPD, the four giant planets revert their migration and migrate outwards.arXiv 2406.20075 · ext:be1d1d21f4b5b884 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | The gaps open by giant planets are wider and deeper for lower viscosity, reducing the damping effect of the disc and thus weakening resonant chains.arXiv 2406.20075 · ext:d0e323aae86a22cd | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | About half of the simulations form a pair of Venus and Earth analogues and, independently, about 10% form a Mars analogue.arXiv 2404.17259 · ext:113f06dfd588ec12 | 0.55 | 1.00 | 0 | 1 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Six out of the eleven tasks exhibit "U-shaped scaling", where performance decreases up to a certain size, and then increases again up to the largest model evaluated (the one remaining task displays positive scaling).arXiv 2211.02011 · ext:98250e6a8fda0088 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | In addition, we find that 1-shot examples and chain-of-thought can help mitigate undesirable scaling patterns even further.arXiv 2211.02011 · ext:0c751838e7a5a515 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | With this increased range of model sizes and training compute, only four out of the eleven tasks remain inverse scaling.arXiv 2211.02011 · ext:1c69acf0c17eafd2 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | We further apply the cavity method to extract Griffiths-McCoy singularities in a diluted (classical) ferromagnet and finally observe that there are no Goldstone bosons on the Bethe lattice.OpenAlex W1555388595 · ext:ce8f7ce299133255 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | In particular, we introduce the study of random quantum satisfiability (QSAT) and identify the coarse aspects of its phase diagram, including a new form of entanglement transition.OpenAlex W1555388595 · conceptual · ext:9d390ba40d4737b0 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Based on the solution clustering (percolation-type) argument, we conjecture two possible values of the FSS exponent, which are confirmed reasonably well in numerical simulations for 2 ≤ K ≤ 3.DOI 10.1103/physreve.82.061109 · conceptual · ext:520dfc880b4bf070 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | Using the FSS theory of nonequilibrium absorbing phase transitions, we show that the density of unsatisfied clauses clearly indicates the transition from the solvable (absorbing) phase to the unsolvable (active) phase as varying the noise…DOI 10.1103/physreve.82.061109 · ext:40c43c8ba9a08553 | 0.55 | 1.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | The weakest ones, from an impact energy per mass perspective, were 20 m in diameter.arXiv 2307.07089 · ext:0422077a9bac436d | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | The only systems that we found to reach a steady state are those in which the planets are locked in a quadruple mean motion resonance (i.e. each planet is in resonance with its neighbor).arXiv 0706.1713 · ext:7bfd311d65718246 | 0.55 | 1.00 | 0 | 1 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | By extracting the mixed metallicity, ionicity, and covalency of solid-state bonding from the DFT-computed electron density, we reveal the complex interplay between chemistry, composition, and electronic structure in governing large-scale s…arXiv 1809.09202 · ext:05428164d67aff2d | 0.55 | 1.00 | 0 | 0 | Materials Science | 8 Oct 2026 |
| unchecked | Our map clusters the ternary nitrides into chemical families with distinct stability and metastability, and highlights hundreds of promising new ternary nitride spaces for experimental investigation--from which we experimentally realized 7…arXiv 1809.09202 · ext:0f36229382cb0233 | 0.55 | 1.00 | 0 | 0 | Materials Science | 8 Oct 2026 |
| unchecked | Its wide survey covers 14,500 square degrees.arXiv 2108.01201 · ext:af6971c54c8d8dcd | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 8 Oct 2026 |
| unchecked | In this paper we rigorise this picture completely for a broad class of models, encompassing the Potts antiferromagnet on the random graph, the $k$-XORSAT model and the diluted $k$-spin model for even $k$.arXiv 1704.01043 · conceptual · ext:343e5f74e797a5ab | 0.55 | 1.00 | 0 | 1 | Physics and Astronomy | 8 Oct 2026 |
| unchecked | The algorithms also show competitive performance on the 10- and 20-dimensional instances of the test functions, although they have not seen such instances during the automated generation process.arXiv 2405.20132 · ext:9a3e5660a8b1e894 | 0.55 | 1.00 | 0 | 0 | Computer Science | 7 Oct 2026 |
| unchecked | With P9, the inclination distribution of model ECs is wider than the observed one.arXiv 1706.07447 · ext:50f02de02a2a6942 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 7 Oct 2026 |
| unchecked | Np(2.5)>1000 is required to obtain a steady-state population of large active HTCs that is consistent with observations.arXiv 1706.07447 · ext:311d323c2ff22891 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 7 Oct 2026 |
| unchecked | The orbital distribution of ecliptic comets (ECs) is well reproduced in models with Np(2.5)=500 and without P9.arXiv 1706.07447 · ext:732cb1f716ca0699 | 0.55 | 1.00 | 0 | 0 | Physics and Astronomy | 7 Oct 2026 |
| unchecked | The RSD measurements indicate a growth rate that is consistent with predictions from Planck primary data and with General Relativity.arXiv 2007.08991 · ext:9b6d37046c0ec35f | 0.55 | 1.00 | 0 | 1 | Physics and Astronomy | 7 Oct 2026 |
| unchecked | Moreover, our methods are shown to generalize across datasets (CIFAR10, CIFAR100, TinyImageNet) and architectures (Vgg16, ResNet-18/ResNet-34, MobileNet).arXiv 2101.03255 · ext:874d5b29c4d22758 | 0.55 | 1.00 | 0 | 0 | Computer Science | 7 Oct 2026 |
| unchecked | Specifically, we have achieved a significant and consistent performance gain of1.05% - 4.93% for ResNet18 on CIFAR-100 over vanilla-LTH.arXiv 2101.03255 · ext:66fc4f57cf82d8bc | 0.55 | 1.00 | 0 | 0 | Computer Science | 7 Oct 2026 |
| 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 | Our findings suggest that probing the representations of current pre-trained gLMs do not offer substantial advantages over conventional machine learning approaches that use one-hot encoded sequences.DOI 10.1186/s13059-025-03674-8 · ext:8b128131f6c7db10 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Guiding Evo 2 via inference-time search enables controllable generation of epigenomic structure, for which we demonstrate the first inference-time scaling results in biology.DOI 10.1101/2025.02.18.638918 · ext:f8a1fd9109cbba2e | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Beyond its predictive capabilities, Evo 2 generates mitochondrial, prokaryotic, and eukaryotic sequences at genome scale with greater naturalness and coherence than previous methods.DOI 10.1101/2025.02.18.638918 · ext:2d48113ef09f048c | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Despite varying levels of advantage across landscapes, focused training with zero-shot predictors leveraging distinct evolutionary, structural, and stability knowledge sources consistently outperforms random sampling for both binding inter…DOI 10.1016/j.cels.2025.101387 · ext:43b0fdfaacab5c21 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | By quantifying landscape navigability with six attributes, we found that MLDE offers a greater advantage on landscapes that are more challenging for directed evolution, especially when focused training is combined with active learning.DOI 10.1016/j.cels.2025.101387 · ext:7c8caa37d11575d0 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We demonstrate the potential of co-piloted auditing, by fine-tuning GPT-4 using OpenAI's ChatGPT interface towards three different audit tasks namely financial ratio analysis, text mining, and journal entry testing.DOI 10.2139/ssrn.4444763 · ext:2b79898141869c04 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Extensive experiments on the LAMA benchmark for extracting relational knowledge from LMs demonstrate that our methods can improve accuracy from 31.1% to 39.6%, providing a tighter lower bound on what LMs know.arXiv 1911.12543 · ext:c39099d2a63df34e | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | However, human performance (86.8%) is much higher, indicating that the dataset presents a good challenge problem for future research.arXiv 1606.05250 · ext:0a03b0bc381897a8 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | We build a strong logistic regression model, which achieves an F1 score of 51.0%, a significant improvement over a simple baseline (20%).arXiv 1606.05250 · ext:aba76b3b5bedb97a | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | Furthermore, the accuracy on 358 datasets across 20 applications is reviewed and unexpected results emerge which show that LLMs are not always the most accurate or least expensive option.DOI 10.1109/access.2024.3349952 · ext:4f95f3682516df17 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | When fine-tuned on Science QA, the synergy of LLaVA and GPT-4 achieves a new state-of-the-art accuracy of 92.53%.arXiv 2304.08485 · ext:00c5deee92353a79 | 0.55 | 0.00 | 0 | 0 | — | 11 Oct 2026 |
| unchecked | SciBERT leverages unsupervised pretraining on a large multi-domain corpus of scientific publications to improve performance on downstream scientific NLP tasks.arXiv 1903.10676 · ext:764349f5d8b228b6 | 0.55 | 0.00 | 0 | 0 | — | 11 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 |