This content will become publicly available on December 29, 2026

Title: Sequence modeling of higher-order wave modes of quasi-circular, spinning, non-precessing binary black hole mergers
Abstract Higher-order gravitational wave modes from quasi-circular, spinning, non-precessing binary-black-hole (BBH) mergers encode rich information about the nonlinear dynamics of strong-field gravity. We present a transformer-based sequence-completion surrogate that, given an early-inspiral segment, forecasts the subsequent late inspiral, merger, and ringdown. The intended applications are (i) patching or completing expensive or interrupted numerical-relativity (NR) simulations and (ii) providing late-time cross-checks and rapid hybridization studies. The training set is built from theNRHybSur3dq8surrogate, which provides spherical-harmonic modes up to 4 (excluding (4, 0) and ( 4 , ± 1 ) , and including (5, 5)) for mass ratios q 8 , dimensionless spin components s 1 , 2 z [ 0.8 , 0.8 ] , and inclination angles θ [ 0 , π ] . Waveforms are supplied on the interval t [ 5000 M , 100 M ) and the model autoregressively generates the plus and cross polarizations ( h + , h × ) on t [ 100 M , 130 M ] . Training on the Delta supercomputer with 16 NVIDIA A100 GPUs required 15  h on more than 14 million hybrid waveforms. Evaluation on a held-out test set of 840,000 samples yields mean and median overlaps of 0.996 and 0.997, respectively, with respect to the surrogate ground truth. The model generalises reasonably well to out-of-distribution NR simulations from the SXS catalogue: across 521 NR waveforms with mass ratios up toq = 15 and spin magnitudes | s | 0.998 , we obtain a median overlap of 0.969, rising to 0.998 for face-on/off orientations. Within the surrogate’s training domain, the transformer provides accurate, millisecond-scale sequence completion of BBH waveforms, including higher-order modes, from early inspiral to ringdown. The NR tests indicate promising performance on higher-fidelity, out-of-distribution data, particularly for detector-favourable orientations.  more » « less
Award ID(s):
2209892
PAR ID:
10695530
Author(s) / Creator(s):
; ;
Publisher / Repository:
Classical and Quantum Gravity
Date Published:
Journal Name:
Classical and Quantum Gravity
Volume:
43
Issue:
1
ISSN:
0264-9381
Page Range / eLocation ID:
015009
Format(s):
Medium: X
Sponsoring Org:
National Science Foundation
More Like this
  1. Abstract A search for resonances in top quark pair ( t t ) production in final states with two charged leptons and multiple jets is presented, based on proton–proton collision data collected by the CMS experiment at the CERN LHC at s = 13 TeV , corresponding to 138 fb−1. The analysis explores the invariant mass of the t t system and two angular observables that provide direct access to the correlation of top quark and antiquark spins. A significant excess of events is observed near the kinematic t t threshold compared to the non-resonant production predicted by fixed-order perturbative quantum chromodynamics (pQCD). The observed enhancement is consistent with the production of a color-singlet pseudoscalar ( 1 S 0 [ 1 ] ) quasi-bound toponium state, as predicted by non-relativistic quantum chromodynamics. Using a simplified model for 1 S 0 [ 1 ] toponium, the cross section of the excess above the pQCD prediction is measured to be 8.8 1.4 + 1.2 pb
    more » « less
  2. Abstract The production of a pair of τ leptons via photon–photon fusion, γ γ τ τ , is observed for the first time in proton–proton collisions, with a significance of 5.3 standard deviations. This observation is based on a data set recorded with the CMS detector at the LHC at a center-of-mass energy of 13 TeV and corresponding to an integrated luminosity of 138 fb−1. Events with a pair of τ leptons produced via photon–photon fusion are selected by requiring them to be back-to-back in the azimuthal direction and to have a minimum number of charged hadrons associated with their production vertex. The τ leptons are reconstructed in their leptonic and hadronic decay modes. The measured fiducial cross section of γ γ τ τ is σ obs fid = 12.4 3.1 + 3.8 fb . Constraints are set on the contributions to the anomalous magnetic moment ( a τ ) and electric dipole moments ( d τ ) of the τ lepton originating from potential effects of new physics on the γ τ τ vertex: a τ = 0.0009 0.0031 + 0.0032 and | d τ | < 2.9 × 10 17 e cm (95% confidence level), consistent with the standard model. 
    more » « less
  3. Abstract A test of lepton flavor universality in B ± K ± μ + μ and B ± K ± e + e decays, as well as a measurement of differential and integrated branching fractions of a nonresonant B ± K ± μ + μ decay are presented. The analysis is made possible by a dedicated data set of proton-proton collisions at s = 13 TeV recorded in 2018, by the CMS experiment at the LHC, using a special high-rate data stream designed for collecting about 10 billion unbiased b hadron decays. The ratio of the branching fractions B ( B ± K ± μ + μ ) to B ( B ± K ± e + e ) is determined from the measured double ratio R ( K ) of these decays to the respective branching fractions of the B ± J / ψ K ± with J / ψ μ + μ and e + e decays, which allow for significant cancellation of systematic uncertainties. The ratio R ( K ) is measured in the range 1.1 < q 2 < 6.0 GeV 2 , whereqis the invariant mass of the lepton pair, and is found to be R ( K ) = 0.78 0.23 + 0.47 , in agreement with the standard model expectation R ( K ) 1 . This measurement is limited by the statistical precision of the electron channel. The integrated branching fraction in the sameq2range, B ( B ± K ± μ + μ ) = ( 12.42 ± 0.68 ) × 10 8 , is consistent with the present world-average value and has a comparable precision. 
    more » « less
  4. Abstract Over the past decade, an abundance of information from neutron-star observations, nuclear experiments and theory has transformed our efforts to elucidate the properties of dense matter. However, at high densities relevant to the cores of neutron stars (NSs), substantial uncertainty about the dense matter equation of state (EoS) remains. In this work, we present a semiparametric EoS framework aimed at better integrating knowledge across these domains in astrophysical inference. We use a meta-model and realistic crust at low densities, and Gaussian process (GP) extensions at high densities. Comparisons between our semiparametric framework to fully nonparametric EoS representations show that imposing nuclear theoretical and experimental constraints through the meta-model up to nuclear saturation density results in constraints on the pressure up to twice nuclear saturation density. We also show that our GP trained on EoS models with nucleonic, hyperonic, and quark compositions extends the range of EoS explored at high density compared to a piecewise polytropic extension schema, under the requirements of causality of matter and of supporting the existence of heavy pulsars (PSRs). We find that maximum Tolman–Oppenheimer–Volkoff masses above 3.2 M can be supported by causal EoS compatible with nuclear constraints at low densities. We then combine information from existing observations of heavy PSR masses, gravitational waves emitted from binary NS mergers, and x-ray pulse profile modeling of millisecond PSRs within a Bayesian inference scheme using our semiparametric EoS prior. With information from all public NS Interior Composition ExploRer PSRs (including PSR J0030+0451, PSR J0740+6620, PSR J0437–4715, and PSR J0614–3329), we find an astrophysically favored pressure at two times nuclear saturation density of P ( 2 ρ nuc ) = 1.98 1.08 + 2.13 × 10 34 dyn cm−2, a radius of a 1.4 M NS value of R 1.4 = 11.4 0.60 + 0.98  km, and M max = 2.31 0.23 + 0.35 M at the 90% credible level (C.L). 
    more » « less
  5. Abstract Polyatomic molecules have been identified as sensitive probes of charge-parity violating and parity violating physics beyond the Standard Model (BSM). For example, many linear triatomic molecules are both laser-coolable and have parity doublets in the ground electronic X ˜ 2 Σ + ( 010 ) state arising from the bending vibration, both features that can greatly aid BSM searches. Understanding the X ˜ 2 Σ + ( 010 ) state is a crucial prerequisite to precision measurements with linear polyatomic molecules. Here, we characterize the fundamental bending vibration of 174 YbOH using high-resolution optical spectroscopy on the nominally forbidden X ˜ 2 Σ + ( 010 ) A ˜ 2 Π 1 / 2 ( 000 ) transition at 588 nm. We assign 39 transitions originating from the lowest rotational levels of the X ˜ 2 Σ + ( 010 ) state, and accurately model the state’s structure with an effective Hamiltonian using best-fit parameters. Additionally, we perform Stark and Zeeman spectroscopy on the X ˜ 2 Σ + ( 010 ) state and fit the molecule-frame dipole moment to D m o l = 2.16 ( 1 ) Dand the effective electrong-factor to g S = 2.07 ( 2 ) . Further, we use an empirical model to explain observed anomalous line intensities in terms of interference from spin–orbit and vibronic perturbations in the excited A ˜ 2 Π 1 / 2 ( 000 ) state. Our work is an essential step toward searches for BSM physics in YbOH and other linear polyatomic molecules. 
    more » « less