Orbital Period Changes for Fourteen Novae and the Critical Failures of the Predictions of Standard Theories, the Hibernation Model, and the Magnetic Braking Model
arXiv:2307.13804 · doi:10.1093/mnras/stad2223
Abstract
The evolution of novae and Cataclysmic Variables (CVs) is driven by changes in the binary orbital periods. In a direct and critical test for various evolution models and their physical mechanisms, I measure the sudden changes in the period () across 14 nova eruptions and I measure the steady period change during quiescence () for 20 inter-eruption intervals. The standard theory for is dominated by the mechanism of mass loss, and this fails completely for the five novae with negative values, and it fails to permit the for U Sco eruptions to change by one order-of-magnitude from eruption-to-eruption. The Hibernation Model of evolution is refuted because all the measures are orders of magnitude too small to cause any significant drop in accretion luminosity, and indeed, near half of the nova have negative as the opposite of the required mechanism for any hibernation state. As for the Magnetic Braking Model, this fails by many orders-of-magnitude in its predictions of the required for 9-out-of-13 novae. The observed values scatter, both positively and negatively, over a range of 10, while the predicted values are from 10 to 10. This huge scatter is not possible with standard theory, and there must be some currently-unknown mechanism to be added in, with this new mechanism 100--10000 larger in effect than the current theory allows. In all, these failed predictions demonstrate that nova systems must have unknown physical mechanisms for both and that dominate over all other effects.
arXiv commentMNRAS in press, see MNRAS webpage for published version and for the Supplementary Materials
References in corpus (30)
- Catalogue of cataclysmic binaries, low-mass X-ray binaries and related objects (Seventh edition)
- The Evolution of Cataclysmic Variables as Revealed by their Donor Stars
- An Extended Grid of Nova Models: II. The Parameter Space of Nova Outbursts
- Comprehensive Photometric Histories of All Known Galactic Recurrent Novae
- Catalog of 93 Nova Light Curves: Classification and Properties
- Revisiting the Lick Observatory Supernova Search Volume-Limited Sample: Updated Classifications and Revised Stripped-Envelope Supernova Fractions
- The Masses and Accretion Rates of White Dwarfs in Classical and Recurrent Novae
- Testing the disk instability model of cataclysmic variables
- The Nova Shell and Evolution of the Recurrent Nova T Pyxidis
- Comprehensive Catalogue of the Overall Best Distances and Properties of 402 Galactic Novae
- Orbital Periods for Three Recurrent Novae
- The Effect of Composition on Nova Ignitions
- The 2011 Outburst of Recurrent Nova T Pyx: X-ray Observations Expose the White Dwarf Mass and Ejection Dynamics
- The B & V Light Curves for Recurrent Nova T CrB From 1842--2022, the Unique Pre- and Post-Eruption High-States, the Complex Period Changes, and the Upcoming Eruption in 2025.51.3
- Novae With Long-Lasting Supersoft Emission That Drive a High Accretion Rate
- A Recurrent Nova Super-Remnant in the Andromeda Galaxy
- A Light Curve Analysis of 32 Recent Galactic Novae --- Distances and White Dwarf Masses
- The Change of the Orbital Periods Across Eruptions and the Ejected Mass For Recurrent Novae CI Aquilae and U Scorpii
- Eclipses During the 2010 Eruption of the Recurrent Nova U Scorpii
- Comprehensive Listing of 156 Reliable Orbital Periods for Novae, Including 49 New Periods
- The physics of the Applegate mechanism: Eclipsing time variations from magnetic activity
- Accurate Pre-Eruption and Post-Eruption Orbital Periods for the Dwarf/Classical Nova V1017 Sgr
- Sudden and Steady Orbital Period Changes Across Six Classical Nova Eruptions; The End of Hibernation and Two Serious Challenges for the Magnetic Braking Model of Cataclysmic Variable Evolution
- T Pyxidis: Death by a Thousand Novae
- Waldmeier Effect in Stellar Cycles
- Precise Measures of Orbital Period, Before and After Nova Eruption for QZ Aurigae
- High-speed photometry of the Recurrent Nova IM Normae
- Sudden and Steady Orbital Period Changes Across the Classical Nova Eruptions of DQ Her and BT Mon
- RR Pictoris: an old nova showing superhumps and QPOs
- On Orbital Period Changes in Nova Outbursts