4.2 Article

Ocular biometric changes with different accommodative stimuli using swept-source optical coherence tomography

Journal

INTERNATIONAL OPHTHALMOLOGY
Volume 39, Issue 2, Pages 303-310

Publisher

SPRINGER
DOI: 10.1007/s10792-017-0813-y

Keywords

Ocular biometry; Accommodation; Cataract; Optical biometer

Categories

Funding

  1. Spanish Government Grant Explora [SAF2013-49284-EXP]
  2. Formacion de Profesorado Universitario'' Grant (Ministerio de Educacion, Cultura y Deporte) [FPU13/05332]

Ask authors/readers for more resources

PurposeTo evaluate ocular biometric changes with different accommodative stimuli using a new swept-source optical biometer.MethodsOnly the right eye was analyzed. Each subject was measured six times with the IOLMaster 700 swept-source optical biometer (Carl Zeiss Meditec, Jena, Germany) with the subject looking at the stimulus shown by the instrument and with the subject looking at a target placed outside the instrument at 0D of vergence. Axial length (AL), anterior chamber depth (ACD), central corneal thickness (CCT), lens thickness (LT), white-to-white (WTW), and keratometry readings (K1 and K2) were evaluated in both cases. To assess if the changes found may affect the intraocular (IOL) power calculation for surgical applications, we have applied some formulae, using the software provided by the optical biometer manufacturer, to the ocular parameters found in both situations for three different types of IOLs.ResultsNo statistically significant differences were found for AL, CCT, WTW, K1 and K2 between the subject looking at the stimulus of the biometer and looking at the outside target at 0D of vergence (p>0.05). However, the measurement of ACD revealed a statistically significant reduction of 20 microns (p=0.03) and, on the contrary, LT increased significantly 30 microns (p=0.02). ACD and LT changes were highly correlated (R-2=0.91). As for the IOL power calculation, in all cases, the mean change was lower than 0.25 D both for IOL power selection and residual refraction.ConclusionsAlthough ACD and LT change significantly with different accommodative stimuli measured by swept-source optical biometry, these changes are not clinically relevant.

Authors

I am an author on this paper
Click your name to claim this paper and add it to your profile.

Reviews

Primary Rating

4.2
Not enough ratings

Secondary Ratings

Novelty
-
Significance
-
Scientific rigor
-
Rate this paper

Recommended

Article Astronomy & Astrophysics

Computational general relativistic force-free electrodynamics: II. Characterization of numerical diffusivity

J. F. Mahlmann, M. A. Aloy, V Mewes, P. Cerda-Duran

Summary: Scientific codes serve as a crucial link between theory and experiment, providing insight into extreme energy flows in the universe. Understanding numerical diffusion in these codes is essential for assessing their reliability, with a minimum of eight numerical cells per characteristic size needed for consistency between numerical and physical results. High-order discretization of force-free currents can achieve nearly ideal convergence for smooth plasma wave dynamics, but modeling resistive layers requires suitable current prescriptions or sub-grid modeling for parallel current evolution.

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

Computational general relativistic force-free electrodynamics: I. Multi-coordinate implementation and testing

J. F. Mahlmann, M. A. Aloy, V Mewes, P. Cerda-Duran

Summary: This study introduces a method called general relativistic force-free electrodynamics to analyze energetic outflows dominated by strong magnetic fields, discussing its application in modeling the dynamics of magnetospheres around compact astrophysical objects like black holes and neutron stars.

ASTRONOMY & ASTROPHYSICS (2021)

Article Astronomy & Astrophysics

Nucleosynthesis in magneto-rotational supernovae

M. Reichert, M. Obergaulinger, M. Eichler, M. A. Aloy, A. Arcones

Summary: This study presents the nucleosynthesis of magneto-rotational supernovae based on 2D simulations with accurate neutrino transport for the first time. Different rotation and magnetic field models are analyzed to explore their impact on the nucleosynthesis processes. Results indicate that the strength of the magnetic field influences the production of heavy elements through the r-process, while accurate neutrino transport is crucial in analyzing the ejecta composition.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2021)

Article Ophthalmology

Evaluation of 6 biometers based on different optical technologies

Robert Montes-Mico

Summary: This study evaluated the repeatability and agreement of various biometric parameters using 6 biometers based on different optical technologies. The results showed that these biometers provided repeatable measurements for different parameters, but there were significant differences between the biometers. Therefore, the interchangeability of these devices should be carefully considered when using them.

JOURNAL OF CATARACT AND REFRACTIVE SURGERY (2022)

Article Ophthalmology

Transitional conic toric intraocular lens evaluation after femtosecond laser-assisted cataract surgery using intraoperative aberrometry

Francisco Pastor-Pascual, Rafael Pastor-Pascual, Robert Montes-Mico, Ramon Ruiz-Mesa, Pedro Tana-Rivero

Summary: The study results indicate that using Precizon IOL after FLACS in patients with different degrees of astigmatism can provide good visual acuity, accurate refractive outcomes, and excellent rotational stability.

INTERNATIONAL OPHTHALMOLOGY (2022)

Article Astronomy & Astrophysics

Diffusivity in force-free simulations of global magnetospheres

J. F. Mahlmann, M. A. Aloy

Summary: This study examines the impact of numerical diffusivity on the overall dynamics of force-free aligned pulsar magnetospheres, assessing constraint violations as a diffusivity source and the effects of modifications on electric fields. By comparing different techniques to model rho, the global consequences of diffusivity are quantified. The conservative approach reduces Poynting flux dissipation in the ECS and increases pulsar luminosity by shifting the Y-point location, with luminosity changes proportional to alpha(0.11).

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Gravitational wave signature of proto-neutron star convection: I. MHD numerical simulations

Raphael Raynaud, Pablo Cerda-Duran, Jerome Guilet

Summary: Gravitational waves provide a unique window to constrain dynamics in proto-neutron stars during core collapse supernovae. Convection and magnetic fields play important roles in neutron star formation, with magnetic fields slightly affecting gravitational wave amplitude in slow rotation regimes and dramatically changing it in fast rotation scenarios. The observed excess of low-frequency gravitational waves at the transition to a strong field dynamo could be used to determine dynamo efficiency in proto-neutron stars.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Ophthalmology

Lens-vault analysis and its correlation with other biometric parameters using swept-source OCT

Pedro Tana-Rivero, Ramon Ruiz-Mesa, Salvador Aguilar-Corcoles, Cristina Tello-Elordi, Maria Ramos-Alzamora, Robert Montes-Mico

Summary: Using the same high-resolution SS-OCT device, lens vault (LV) was measured in healthy eyes, revealing correlations with anterior chamber depth, axial length, anterior chamber volume, lens thickness, and age.

JOURNAL OF OPTOMETRY (2022)

Article Astronomy & Astrophysics

Magnetorotational core collapse of possible gamma-ray burst progenitors-IV. A wider range of progenitors

M. Obergaulinger, M. A. Aloy

Summary: The collapse of massive star cores can have various outcomes regarding energy release, nucleosynthesis, and remnants. The relationship between explosion and remnant types and the properties of the progenitors is still an open question. The rotation and magnetic fields in Wolf-Rayet stars may explain extreme events like superluminous supernovae and gamma-ray bursts.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

The magneto-rotational instability in massive stars

Adam Griffiths, Patrick Eggenberger, Georges Meynet, Facundo Moyano, Miguel-A Aloy

Summary: This study explores the effects of the magneto-rotational instability (MRI) on the evolution of massive stars. The results show that the activation of MRI is highly sensitive to the treatment of meridional circulation and the existence of chemical gradients. The MRI efficiently transports matter and angular momentum, leading to noticeable differences in rotation rates and chemical structure of stars.

ASTRONOMY & ASTROPHYSICS (2022)

Article Astronomy & Astrophysics

r-process Viable Outflows are Suppressed in Global Alpha-viscosity Models of Collapsar Disks

O. Just, M. A. Aloy, M. Obergaulinger, S. Nagataki

Summary: This study presents global models of collapsars and finds that neutron-rich, neutrino-dominated accretion flows are only established for short times or relatively low viscosities, while stable NDAFs are unable to release neutron-rich ejecta. The research suggests that collapsar models based on the alpha-viscosity are inefficient r-process sites and that magnetohydrodynamic effects may be required to generate neutron-rich outflows to improve the prospects for obtaining neutron-rich ejecta.

ASTROPHYSICAL JOURNAL LETTERS (2022)

Article Astronomy & Astrophysics

Assessment of a new sub-grid model for magnetohydrodynamical turbulence. I. Magnetorotational instability

Miquel Miravet-Tenes, Pablo Cerda-Duran, Martin Obergaulinger, Jose A. Font

Summary: In this study, a new sub-grid model called MInIT mean-field model is proposed to capture the effects of turbulence at small scales. Through linking the turbulent stress tensors with the energy densities, the model successfully simulates the DNS data of MRI in-box and compares it with the filtered data.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2022)

Article Astronomy & Astrophysics

Magnetorotational supernovae: a nucleosynthetic analysis of sophisticated 3D models

M. Reichert, M. Obergaulinger, M. A. Aloy, M. Gabler, A. Arcones, F. K. Thielemann

Summary: Magnetorotational supernovae are a rare type of core-collapse supernovae that involve magnetic fields and rotation in the explosion dynamics. Post-processed nucleosynthesis of neutrino-MHD supernova models reveals three mechanisms for heavy r-process element production. The study highlights the role of magnetorotational supernovae in hypernovae, superluminous supernovae, and heavy element synthesis.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY (2023)

Article Astronomy & Astrophysics

Gravitational Wave Eigenfrequencies from Neutrino-driven Core-collapse Supernovae

Noah E. Wolfe, Carla Frohlich, Jonah M. Miller, Alejandro Torres-Forne, Pablo Cerda-Duran

Summary: This study builds a comprehensive suite of over 1000 exploding CCSNe models to analyze the resonant gravitational wave frequencies of the proto-neutron star (PNS). The study identifies characteristic frequencies that can measure the surface gravity of the cold remnant neutron star and constrain the hot nuclear equation of state. However, the study finds that the details of the CCSN models and whether it undergoes an explosion significantly affect the magnitude and evolution of the PNS eigenfrequencies.

ASTROPHYSICAL JOURNAL (2023)

Article Astronomy & Astrophysics

Can fermion-boson stars reconcile multimessenger observations of compact stars?

Fabrizio Di Giovanni, Nicolas Sanchis-Gual, Pablo Cerda-Duran, Jose A. Font

Summary: This study constructs equilibrium configurations of mixed fermion-boson stars with realistic equations of state for the fermionic component and different percentages of bosonic matter, and demonstrates that these solutions are in good agreement with observational data and nuclear physics constraints.

PHYSICAL REVIEW D (2022)

No Data Available