| unchecked | We find that $γ= 0.519^{+0.061}_{-0.099}$ ($0.500^{+0.054}_{-0.098}$) [$0.525^{+0.074}_{-0.073}$], which are consistent with the predictions of General Relativity.arXiv 2604.06361 · conceptual · ext:96b9fa8d0e2715bf | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | We verify that systems disrupted in this way are frequently unstable to close encounters within $\sim 100$Myr of the final flyby.arXiv 2510.18955 · ext:4cb2d4e19ff7943a | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | We find a planetesimal reservoir of total mass $\gtrsim 0.04 M_{\oplus}$ is required to disrupt MMR chains, depending on the mass distribution and the typical number of flybys executed by each planetesimal.arXiv 2510.18955 · ext:6705ab147d83502e | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | An atmospheric entry probe targeting the 10-bar level, about 5 scale heights beneath the tropopause, would yield insight into two broad themes: i) the formation history of the ice giants and, in a broader extent, that of the Solar System,…arXiv 1708.00235 · conceptual · ext:eaccd3c18643ab48 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | If we factor in the probability that the outer planetary orbits are well-replicated, we find a probability of 1% or less that the orbital architectures of the inner and outer planets are simultaneously reproduced in the same system.arXiv 1510.08448 · ext:c3d133935f35bc75 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | There is less than a ~5% chance that the terrestrial planet orbits will have a level of excitation comparable to the observed orbits.arXiv 1510.08448 · ext:5f97b056f1527840 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | The constraints on $w_E$ are consistent with dark energy, while particle creation of pressureless matter is disfavoured.arXiv 2601.14222 · ext:a2e2008231b7bdb8 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | The probability of implanting Athor analogs when the instability occurs at $\lesssim15$~Myr is at most a factor of $\sim$2 lower than that of an instability occurring at $\sim100$~Myr after the solar system formation.arXiv 2404.10828 · ext:538bdcbbe017015f | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | Under the proposed scenario, the current period ratio of 3.05 between Mars and Venus -- devoid of any special significance in traditional late formation models -- naturally arises as a relic of the former resonance chain.arXiv 2506.04164 · ext:26f31e4aa4ac2cc5 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 10 Oct 2026 |
| unchecked | The experiments, performed on the CIFAR-10 and ImageNet datasets, clearly demonstrate the efficiency of RSDTR in comparison to other state-of-the-art CNNs compression approaches.arXiv 2405.10802 · ext:4b6396f54a0b957c | 0.55 | 0.00 | 0 | 0 | Computer Science | 10 Oct 2026 |
| supported | Using this GPU-accelerated search procedure on our simplified flip graph, we find a way to multiply $7\times 7$ matrices over $\mathbb{F}_2$ using 245 multiplications, a three-multiplication improvement over the previous record.arXiv 2609.17533 · ext:230f9d0715ec7ae6 | 0.71 | 0.00 | 1 | 0 | Computer Science | 10 Oct 2026 |
| unchecked | As a consequence, in the observationally viable thawing regime the axion does not track the background fluid and spatial curvature becomes dynamically subdominant, leading to an effectively single-field evolution.arXiv 2603.18341 · ext:1c42633dd56c30c5 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | However, we show that these mechanisms arise in distinct invariant manifolds and cannot be simultaneously realized in the presence of a background fluid: no non-geodesic scaling fixed point exists within an open region of parameter space.arXiv 2603.18341 · conceptual · ext:ed6f4bcc3d66f7e4 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | While our dynamical simulations indicate that Vesta likely underwent a significant number of collisions with large comets, we find no xenon cometary signature in HED meteorites.arXiv 2507.00753 · ext:cdfef597ba12ca6c | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Our calculations show that, even under the most conservative scenario, the minimal mass of the primordial martian atmospheres would yield a surface pressure of no less than 2.9 bar.arXiv 2509.10060 · ext:1eed156a01347ca2 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Therefore, if a cometary xenon signature is ever detected in an asteroid belt object, it must have been acquired during formation, within the same source region as comet 67P/Churyumov-Gerasimenko, and have been implanted later into the ast…arXiv 2507.00753 · ext:4772da0fe1f6d9a4 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | This apparent contradiction arises due to the fact that cometary impacts were at high speeds and Vesta's weak gravitational attraction made it incapable of retaining cometary material.arXiv 2507.00753 · ext:4c9823190d587468 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Furthermore, we establish that the overlap between two independently drawn solutions concentrates precisely at two values.arXiv 2011.14270 · ext:f02ae1c772dd7d1b | 0.55 | 0.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | Namely, we prove that with probability bounded away from zero, most of the solutions lie inside a bounded number of solution clusters whose sizes are comparable to the scale of the free energy.arXiv 2011.14270 · ext:08ce6e4ca6dd475d | 0.55 | 0.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | This results in prediction that is up to 60x faster than state-of-the-art while maintaining resolution and accuracy.DOI 10.1101/2022.07.20.500902 · ext:e416da575785724b | 0.55 | 0.00 | 0 | 0 | — | 9 Oct 2026 |
| unchecked | The ACE2 model exhibits skilful predictions of the North Atlantic Oscillation (NAO) with a correlation score of 0.47 (p=0.02), as well as a realistic global distribution of skill and ensemble spread.arXiv 2503.23953 · ext:bc8a3c5d58567c8d | 0.55 | 0.00 | 0 | 0 | Earth and Planetary Sciences | 9 Oct 2026 |
| unchecked | We find that certain data combinations, such as SPT+WMAP+BAO and PL18+BAO, can reduce the significance of the $H_0$ tension below $1σ$, but with considerably large uncertainties.arXiv 2504.17859 · ext:4b5352a7c0544bfe | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Our results generically exhibit multiple phantom divide line crossings in a single expansion history; if confirmed, this points beyond the simplest minimally coupled canonical single-field quintessence/phantom descriptions and motivates mo…arXiv 2504.17859 · ext:547a7a5b8778eabb | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | However, the inclusion of PP data restores the tension in $H_0$.arXiv 2504.17859 · ext:9bcd84fe0e65f1ee | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | In step ``0", the TianQin laser ranging station has been constructed and it has successfully ranged to all the five retro-reflectors on the Moon.arXiv 2502.11328 · ext:70266036dcfa86c5 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | For example, under 300M FLOPs constraint, our pruned MobileNetV2 achieves 75.2% Top-1 accuracy on ImageNet dataset, exceeding the original MobileNetV2 by 2.6 units while only cost 30%/16% times than BCNet/AutoAlim.arXiv 2408.16233 · ext:65b31a756be5db21 | 0.55 | 0.00 | 0 | 0 | Computer Science | 9 Oct 2026 |
| unchecked | We provide a very simple proof of this fundamental result; in fact, we prove that in the supercritical regime p=(1+ε)/n, the random graph G(n,p) contains typically a path of linear length.arXiv 1201.6529 · ext:9d958c1c65e94f35 | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | The same approach can be also used to show that pseudo-random graphs have strong induced Ramsey properties.arXiv 0706.4112 · conceptual · ext:673efa87be17cdc1 | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | The proofs are based on a simple lemma (generalizing one by Graham, Rodl, and Rucinski) that can be used as a replacement for Szemeredi's regularity lemma, thereby giving much better bounds.arXiv 0706.4112 · conceptual · ext:f58fcc67777290d6 | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | Second, disproving a folklore conjecture in the area, we show that there exists a linear hypergraph $H$ for which $r(H, K_n^{(3)})$ is superpolynomial in $n$.arXiv 2404.02021 · ext:6206ca3370c27c2d | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | First, we show that for a broad class of $H$, including links of odd cycles and tight cycles of length not divisible by three, $r(H, K_n^{(3)}) \ge 2^{Ω_H(n \log n)}$.arXiv 2404.02021 · conceptual · ext:aa3ab41ca0abab31 | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | We also present a construction showing that this bound is tight for $q \ge 4$.arXiv 2308.10833 · conceptual · ext:63df62650795a311 | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | For fixed $k \ge 3$ and $q \ge 2$ we prove that the largest possible $q$-color Ramsey number of a $k$-uniform hypergraph with $m$ edges is at most $\mathrm{tw}_k(O(\sqrt{m})),$ where $\mathrm{tw}$ denotes the tower function.arXiv 2308.10833 · conceptual · ext:939d2ced99248bfb | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | On the other hand, we prove that long loose paths are always at least asymptotically $H$-good for every $H$ and derive lower and upper bounds that are best possible in a certain sense.arXiv 2312.04955 · conceptual · ext:22c8204c38a59efc | 0.55 | 0.00 | 0 | 0 | Mathematics | 9 Oct 2026 |
| unchecked | For such an encounter to happen with a reasonably high probability the Sun must have formed in a stellar cluster with $ηT \gtrsim 10^4$ Myr pc$^{-3}$, where $η$ is the stellar number density and $T$ is the Sun's residence time in the clust…arXiv 2308.11059 · conceptual · ext:dadb81e558708017 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | In these simulations, accretion has begun in the Mars region before the instability, but the dynamical perturbation induced by the giant planets' scattering removes large embryos from Mars' vicinity.arXiv 1804.04233 · ext:8423f6a6144a2f58 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | Here we use 800 dynamical simulations to show that an early instability in the outer solar system strongly influences terrestrial planet formation and regularly yields properly sized Mars analogs.arXiv 1804.04233 · ext:38e0d88190585ab0 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | The jump capture is potentially capable of explaining the observed asymmetry in the number of leading and trailing Trojans.arXiv 1303.2900 · ext:7cdf6fc515983ba1 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | We find that the capture probability is (6-8)x10^-7 for each particle in the original transplanetary disk, implying that the disk contained (3-4)x10^7 planetesimals with absolute magnitude H<9 (corresponding to diameter D=80 km for a 7% al…arXiv 1303.2900 · ext:dab4b3b600d4612f | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | After the disappearance of the gas, and in absence of planetesimals, only two of these six configurations (the least compact ones) are stable for a time of hundreds of millions of years or more.arXiv 0706.1713 · ext:b9ccb0c87eab231e | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 9 Oct 2026 |
| unchecked | As the language models are scaled they learn information that enables prediction of the three-dimensional structure of a protein at the resolution of individual atoms.DOI 10.1101/2022.07.20.500902 · ext:9d738b79626dfaf7 | 0.55 | 0.00 | 0 | 0 | — | 8 Oct 2026 |
| unchecked | The atlas reveals more than 225 million high confidence predictions, including millions whose structures are novel in comparison with experimentally determined structures, giving an unprecedented view into the vast breadth and diversity of…DOI 10.1101/2022.07.20.500902 · ext:040affaa7676fb61 | 0.55 | 0.00 | 0 | 0 | — | 8 Oct 2026 |
| unchecked | Preferential desorption of CO and CO$_2$ relative to H$_2$O in the interstellar medium implies that measured C/O ratios represent lower limits on the primordial ratios.arXiv 2204.13211 · conceptual · ext:afbc91c37cd29fb9 | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 8 Oct 2026 |
| unchecked | This limit exhibits a complicated non-Markovian structure arising from the space of solutions being dominated by a small number of large clusters.arXiv 2305.17334 · ext:aab80141c0eb3845 | 0.55 | 0.00 | 0 | 0 | Computer Science | 8 Oct 2026 |
| supported | Notably, a new $4 \times 4 \times 10$ scheme requiring only 115 multiplications is discovered, achieving $ω\approx 2.80478$ and beating Strassen's exponent for this specific size.arXiv 2603.02398 · ext:1a12e2474ed439c5 | 0.71 | 0.00 | 1 | 0 | Computer Science | 8 Oct 2026 |
| unchecked | The combined effects of modified late-time expansion and additional relativistic degrees of freedom systematically raise the inferred Hubble constant, substantially alleviating the \(H_0\) tension without invoking early dark energy or intr…arXiv 2601.02077 · ext:81cdc3a72135bf85 | 0.55 | 0.00 | 1 | 0 | Physics and Astronomy | 8 Oct 2026 |
| unchecked | Crucially, the data exhibit a statistically significant preference for a late-time dark-energy transition, characterized by a robust quintessence--phantom crossing that remains stable across all dataset combinations and neutrino-sector ext…arXiv 2601.02077 · ext:9d5fbaac7f36e38e | 0.55 | 0.00 | 0 | 0 | Physics and Astronomy | 8 Oct 2026 |
| supported | Our results are new schemes for multiplying $5\times 5$ matrices using $93$ multiplications and $6\times 6$ matrices using $153$ multiplications over arbitrary ground fields.arXiv 2502.04514 · ext:e7af2cfc4f8205e6 | 0.71 | 0.00 | 1 | 0 | Computer Science | 8 Oct 2026 |
| unchecked | Our combined approach yields an upper bound of $ω$ < 2.371177, improving the previous best bound of 2.371339.arXiv 2608.16884 · ext:220d68fc2177402b | 0.55 | 0.00 | 0 | 0 | Computer Science | 7 Oct 2026 |
| supported | We compute digits of $ζ(3)$ and $ζ(5)$, starting at the ten millionth hexadecimal place.arXiv math/9803067 · ext:b5a5d5e466728267 | 0.71 | 0.00 | 1 | 0 | Mathematics | 7 Oct 2026 |
