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Double-averaging can fail to characterize the long-term evolution of Lidov–Kozai Cycles and derivation of an analytical correction

Monthly notices of the Royal Astronomical Society, 2016-05, Vol.458 (3), p.3060-3074

2016

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Long-term cycling of Kozai-Lidov cycles: extreme eccentricities and inclinations excited by a distant eccentric perturber

Physical review letters, 2011-10, Vol.107 (18), p.181101-181101, Article 181101

2011

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WARM JUPITERS NEED CLOSE “FRIENDS” FOR HIGH-ECCENTRICITY MIGRATION—A STRINGENT UPPER LIMIT ON THE PERTURBER'S SEPARATION

Astrophysical journal. Letters, 2014-01, Vol.781 (1), p.1-5

2014

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An accurate and efficient numerical calculation of detonation waves in multidimensional supernova simulations using a burning limiter and adaptive quasi-statistical equilibrium

Monthly notices of the Royal Astronomical Society, 2020-04, Vol.493 (4), p.5413-5433

2020

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AMS-02 results support the secondary origin of cosmic ray positrons

Physical review letters, 2013-11, Vol.111 (21), p.211101-211101, Article 211101

2013

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Librating Kozai–Lidov Cycles with a Precessing Quadrupole Potential Are Analytically Approximately Solved

The Astronomical journal, 2024-02, Vol.167 (2), p.80

2024

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Fast Radiation Mediated Shocks and Supernova Shock Breakouts

The Astrophysical journal, 2010-06, Vol.716 (1), p.781-791

2010

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Analytic Understanding of the Resonant Nature of Kozai–Lidov Cycles with a Precessing Quadrupole Potential

Astrophysical journal. Letters, 2023-08, Vol.953 (1), p.L10

2023

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NON-RELATIVISTIC RADIATION MEDIATED SHOCK BREAKOUTS. III. SPECTRAL PROPERTIES OF SUPERNOVA SHOCK BREAKOUT

The Astrophysical journal, 2013-09, Vol.774 (1), p.1-15

2013

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Magnetic Field Evolution in Relativistic Unmagnetized Collisionless Shocks

The Astrophysical journal, 2009-03, Vol.693 (2), p.L127-L130

2009

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Radius and magnetic field from synchrotron self‐absorbed radio and inverse‐Compton X‐ray observations of supernovae

Monthly notices of the Royal Astronomical Society. Letters, 2012-02, Vol.420 (1), p.L6-L7

Katz, Boaz

2012

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NON-RELATIVISTIC RADIATION MEDIATED SHOCK BREAKOUTS. II. BOLOMETRIC PROPERTIES OF SUPERNOVA SHOCK BREAKOUT

The Astrophysical journal, 2012-03, Vol.747 (2), p.1-11

2012

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Non-relativistic Radiation-mediated Shock Breakouts. I. Exact Bolometric Planar Breakout Solutions

The Astrophysical journal, 2011-11, Vol.742 (1), p.36-jQuery1323901578005='48'

2011

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What can we really learn from positron flux ‘anomalies’?

Monthly notices of the Royal Astronomical Society, 2010-07, Vol.405 (3), p.1458-1472

2010

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ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia

The Astrophysical journal, 2019-07, Vol.880 (1), p.35

2019

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THE IMPORTANCE OF 56Ni IN SHAPING THE LIGHT CURVES OF TYPE II SUPERNOVAE

The Astrophysical journal, 2016-05, Vol.823 (2)

2016

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Polarization signatures of the head-on collision model for Type Ia supernovae: how much asymmetry is too much?

Monthly notices of the Royal Astronomical Society, 2022-02, Vol.511 (2), p.2994-3004

2022

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A simple random walk model explains the disruption process of hierarchical, Eccentric three-body systems

Monthly notices of the Royal Astronomical Society, 2020-10, Vol.498 (1), p.665-673

2020

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An asymmetric explosion mechanism may explain the diversity of Si ii linewidths in Type Ia supernovae

Monthly notices of the Royal Astronomical Society, 2020-06, Vol.494 (4), p.5811-5824

2020

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Cosmic Rays from Transrelativistic Supernovae

The Astrophysical journal, 2008-02, Vol.673 (2), p.928-933

2008

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FAILURE OF A NEUTRINO-DRIVEN EXPLOSION AFTER CORE-COLLAPSE MAY LEAD TO A THERMONUCLEAR SUPERNOVA

The Astrophysical journal, 2015-10, Vol.811 (2), p.97

2015

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Type Ia supernovae have two physical width–luminosity relations and they favour sub-Chandrasekhar and direct collision models – I. Bolometric

Monthly notices of the Royal Astronomical Society, 2019-04, Vol.484 (3), p.3941-3950

2019

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Comments on ‘numerical stability of detonations in white dwarf simulations’

Monthly notices of the Royal Astronomical Society, 2020-01, Vol.491 (3), p.3760-3766

2020

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Extreme close approaches in hierarchical triple systems with comparable masses

Monthly notices of the Royal Astronomical Society, 2018-09, Vol.479 (3), p.3155-3166

2018

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Type Ia supernovae have two physical width–luminosity relations and they favour sub-Chandrasekhar and direct collision models - II. Colour evolution

Monthly notices of the Royal Astronomical Society, 2019-04, Vol.484 (3), p.3951-3967

2019

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Double-averaging can fail to characterize the long-term evolution of Lidov–Kozai Cycles and derivation of an analytical correction

Long-term cycling of Kozai-Lidov cycles: extreme eccentricities and inclinations excited by a distant eccentric perturber

WARM JUPITERS NEED CLOSE “FRIENDS” FOR HIGH-ECCENTRICITY MIGRATION—A STRINGENT UPPER LIMIT ON THE PERTURBER'S SEPARATION

An accurate and efficient numerical calculation of detonation waves in multidimensional supernova simulations using a burning limiter and adaptive quasi-statistical equilibrium

AMS-02 results support the secondary origin of cosmic ray positrons

Librating Kozai–Lidov Cycles with a Precessing Quadrupole Potential Are Analytically Approximately Solved

Fast Radiation Mediated Shocks and Supernova Shock Breakouts

Analytic Understanding of the Resonant Nature of Kozai–Lidov Cycles with a Precessing Quadrupole Potential

NON-RELATIVISTIC RADIATION MEDIATED SHOCK BREAKOUTS. III. SPECTRAL PROPERTIES OF SUPERNOVA SHOCK BREAKOUT

Magnetic Field Evolution in Relativistic Unmagnetized Collisionless Shocks

Radius and magnetic field from synchrotron self‐absorbed radio and inverse‐Compton X‐ray observations of supernovae

NON-RELATIVISTIC RADIATION MEDIATED SHOCK BREAKOUTS. II. BOLOMETRIC PROPERTIES OF SUPERNOVA SHOCK BREAKOUT

Non-relativistic Radiation-mediated Shock Breakouts. I. Exact Bolometric Planar Breakout Solutions

What can we really learn from positron flux ‘anomalies’?

ASASSN-15pz: Revealing Significant Photometric Diversity among 2009dc-like, Peculiar SNe Ia

THE IMPORTANCE OF 56Ni IN SHAPING THE LIGHT CURVES OF TYPE II SUPERNOVAE

Polarization signatures of the head-on collision model for Type Ia supernovae: how much asymmetry is too much?

A simple random walk model explains the disruption process of hierarchical, Eccentric three-body systems

An asymmetric explosion mechanism may explain the diversity of Si ii linewidths in Type Ia supernovae

Cosmic Rays from Transrelativistic Supernovae

FAILURE OF A NEUTRINO-DRIVEN EXPLOSION AFTER CORE-COLLAPSE MAY LEAD TO A THERMONUCLEAR SUPERNOVA

Type Ia supernovae have two physical width–luminosity relations and they favour sub-Chandrasekhar and direct collision models – I. Bolometric

Comments on ‘numerical stability of detonations in white dwarf simulations’

Extreme close approaches in hierarchical triple systems with comparable masses

Type Ia supernovae have two physical width–luminosity relations and they favour sub-Chandrasekhar and direct collision models - II. Colour evolution

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