Template:NewFRBModel: Difference between revisions

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<noinclude>
This is the FRB Model template.


{{#cargo_declare:
<!-- Brings in the summary table -->
_table = frbtheory
<!-- This is an example. Change the right hand side of all these assignments -->
|frbt_category = String
{{FRBTableTemplate
|frbt_progenitor = String
|Category              = Merger
|frbt_rep_no_rep = String (hierarchy; allowed values= *Repeating,*Non-repeating,*Both)
|Progenitor            = NS-NS
|frbt_energy_mech = String
|Type                  = Single
|frbt_emission_mech = String
|EnergyMechanism        = Mag. reconnection
|frbt_cntrpts_lf_radio = String
|EmissionMechanism      = Curv.
|frbt_cntrpts_hf_radio = String
|LFRadioCounterpart    = Yes <br/>(excl. self absorption)
|frbt_cntrpts_mwave = String
|HFRadioCounterpart    = Yes
|frbt_cntrpts_thz = String
|MicrowaveCounterpart  = Maybe
|frbt_cntrpts_oir = String
|THzCounterpart        = Maybe
|frbt_cntrpts_xray = String
|OIRCounterpart        = No
|frbt_cntrpts_gamma = String
|XrayCounterpart        = Afterglow
|frbt_cntrpts_gw = String
|GammarayCounterpart    = Yes <br/> if jet aligned
|frbt_cntrpts_neu = String
|GWCounterpart          = Yes
|frbt_ref = URL
|NeutrinoCounterpart    = Not detectable
|References            = http://adsabs.harvard.edu/abs/2018arXiv180804822P, http://adsabs.harvard.edu/abs/2018arXiv180804822P
|Comments              = None
}}
}}
</noinclude>


<includeonly>
== Model Description ==
== Concise name of the FRB Theory ==
 
 
{{#cargo_store:
_table = frbtheory
|frbt_category = Merger
|frbt_progenitor = NS-NS
|frbt_rep_no_rep = Non-repeating
|frbt_energy_mech = Reconnection
|frbt_emission_mech = Curvature
|frbt_cntrpts_lf_radio = Yes
|frbt_cntrpts_hf_radio = Yes (prompt+afterglow)
|frbt_cntrpts_mwave = Maybe
|frbt_cntrpts_thz = No
|frbt_cntrpts_oir = No
|frbt_cntrpts_xray = Yes (from merger, afterglow)
|frbt_cntrpts_gamma = Yes (if jet aligned)
|frbt_cntrpts_gw = Yes (within LIGO horizon)
|frbt_cntrpts_neu = Not detectable
|frbt_ref = http://adsabs.harvard.edu/abs/2018arXiv180804822P
}}


A broader description, observational effects and detailed information.
This is an FRB model where the merger of two neutron stars would lead to the generation of an isotropic radio pulse.


<!-- DO NOT CHANGE THE FORMAT OF THIS TABLE -->
== Observational Constraints ==
<!-- Leave untouched from here -->
{| class="wikitable"
|+ Summary Table
|-
! rowspan="2" | Category !! rowspan="2" | Progenitor !! rowspan="2" | Repeating/Non-Repeating !! rowspan="2" | Energy Mechanism !! rowspan="2" | Emission Mechanism !! colspan="9" | Counterparts !! rowspan="2" | Reference !! rowspan="2" | Brief Comments
|- 
| Low Freq. Radio (3 MHz - 3 GHz) || High Freq. Radio (3 GHz - 30 GHz) || Microwave (30 - 300 GHz) || Terahertz || Optical/IR || X-rays || Gamma-rays || Neutrinos || Gravitational Waves
|-
<!-- Till here -->
<!-- Modify from here -->
| Merger
| NS - NS
| Mag. braking
| Curvature
| Maybe
| Yes
| Yes
| No
| No
| No
| Yes (merger, afterglow)
| sGRB, depending on jet angle
| Not detectable
| Yes
| [http://www.example.com link title]
|
<!-- Leave this bit untouched as well -->
|}


== Description ==
In general this model would predict that FRBs arise from old stellar populations where NS-NS binary systems have had time to form and evolve into compact orbits.
 
A broader description, observational effects and detailed information.
</includeonly>

Latest revision as of 14:55, 25 September 2018





Summary Table
Category Progenitor Type Energy Mechanism Emission Mechanism Counterparts References Brief Comments
LF Radio HF Radio Microwave Terahertz Optical/IR X-rays Gamma-rays Gravitational Waves Neutrinos
Merger NS-NS Single Mag. reconnection Curv. Yes
(excl. self absorption) 		Yes Maybe Maybe No Afterglow Yes
if jet aligned 		Yes Not detectable http://adsabs.harvard.edu/abs/2018arXiv180804822P, http://adsabs.harvard.edu/abs/2018arXiv180804822P None

Definitions: LF Radio (3 MHz to 3 GHz); HF Radio (3 GHz to 30 GHz); Microwave (30 to 300 GHz)


Model Description

A broader description, observational effects and detailed information. This is an FRB model where the merger of two neutron stars would lead to the generation of an isotropic radio pulse.

Observational Constraints

In general this model would predict that FRBs arise from old stellar populations where NS-NS binary systems have had time to form and evolve into compact orbits.

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