Testing Models of Periodically Modulated FRB Activity

Abstract

The activity of the repeating FRB 20180916B is periodically modulated with a period of 16.3 days, and FRB 121102 may be similarly modulated with a period of about 160 days. In some models of this modulation the period derivative is insensitive to the uncertain parameters; these models can be tested by measurement of or bounds on the derivative. In other models values of the uncertain parameters can be constrained. Periodic modulation of aperiodic bursting activity may result from emission by a narrow beam wandering within a cone or funnel along the axis of a precessing disc, such as the accretion discs in X-ray binaries. The production of FRB 200428 by a neutron star that is neither accreting nor in a binary then shows universality: coherent emission may occur in a wide range of environments.

arXiv comment5 pp; typo in Eq. 7 corrected

References in corpus (23)

• Periodic activity from a fast radio burst source
• Possible periodic activity in the repeating FRB 121102
• Repeating behaviour of FRB 121102: periodicity, waiting times and energy distribution
• LOFAR Detection of 110-188 MHz Emission and Frequency-Dependent Activity from FRB 20180916B
• A long-period, violently-variable X-ray source in a young SNR
• A Binary Comb Model for Periodic Fast Radio Bursts
• Periodicity in recurrent fast radio bursts and the origin of ultra long period magnetars
• FRB-periodicity: mild pulsars in tight O/B-star binaries
• Precessing flaring magnetar as a source of repeating FRB 180916.J0158+65
• Periodic Fast Radio Bursts with Neutron Star Free/Radiative Precession
• The lowest frequency Fast Radio Bursts: Sardinia Radio Telescope detection of the periodic FRB 180916 at 328 MHz
• Orbit-induced spin precession as an origin of periodicity in periodically-repeating fast radio bursts
• Are Fast Radio Bursts Made By Neutron Stars?
• Periodicity in fast radio bursts due to forced precession by a fallback disk
• Orbital, Superhump, and Superorbital Periods in the Cataclysmic Variables AQ Mensae and IM Eridani
• Are FRB Wandering Narrow Beams?
• Yet Another Model of Soft Gamma Repeaters
• Periodic fast radio bursts from forcedly precessing neutron stars, anomalous torque, and internal magnetic field for FRB 180916.J0158+65 and FRB 121102
• The Environment of FRB 121102 and Possible Relation to SGR/PSR J1745-2900
• Orbital and super-orbital periods in ULX pulsars, disc-fed HMXBs, Be/X-ray binaries and double-periodic variables
• The doubling of the superorbital period of Cyg X-1
• What binary systems are the most likely sources for periodically repeating FRBs?
• Origin of sources of repeating fast radio bursts with periodicity in close binary systems

Cited by in corpus (17)

• Periodic Fast Radio Bursts from Luminous X-ray Binaries
• A non-repeating fast radio burst in a dwarf host galaxy
• Binary comb models for FRB 121102
• An accreting stellar binary model for active periodic fast radio bursts
• Rotation Measure Variations and Reversals of Repeating Fast Radio Bursts in Massive Binary Systems
• High frequency study of FRB 20180916B using the 100-m Effelsberg radio telescope
• Emission Properties of Periodic Fast Radio Bursts from the Motion of Magnetars: Testing Dynamical Models
• The periodic origin of fast radio bursts
• A Thorough Search for Short Timescale Periodicity in Four Active Repeating Fast Radio Bursts
• Precession and Jitter in FRB 180916B
• Distinguishing Time Clustering of Astrophysical Bursts
• Reconciling the 16.35-day period of FRB 20180916B with jet precession
• Empirical Assessment of Aperiodic and Periodic Radio Bursts from Young Precessing Magnetars
• Constraining the origin of the long term periodicity of FRB 20180916B with Polarization Position Angle
• Periodic Activities of Fast Radio Burst Repeaters from Precessing Magnetars with Evolving Obliquity
• Symmetry Breaking in Repeating Fast Radio Bursts
• Do the periodic activities of repeating fast radio bursts represent the spins of neutron stars?