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Millisecond extragalactic radio bursts as magnetar flares

Millisecond extragalactic radio bursts as magnetar flares. Sergei Popov, Konstantin Postnov (SAI MSU). mERB: millisecond extragalactic radio burst. Discovered by Lorimer et al. [Science 318, 777 (2007)] 1.4 GHz, Parkes ~30-40 Jy, < 5 msec 3 degrees from SMC.

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Millisecond extragalactic radio bursts as magnetar flares

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  1. Millisecond extragalactic radio bursts as magnetar flares Sergei Popov,Konstantin Postnov (SAI MSU)

  2. mERB: millisecond extragalactic radio burst Discovered by Lorimer et al.[Science 318, 777 (2007)] 1.4 GHz, Parkes ~30-40 Jy, < 5 msec 3 degrees from SMC

  3. mERB: millisecond extragalactic radio burst Large DM 375 cm-3 pc ExtragalacticDistance ~< 1 Gpc (>600 Mpc from optical limits on the host galaxy) Rate is about 90/day/Gpc3 This rate is much lowerthan the SN rate, andmuch larger that the rate of GRBs. [Science 318, 777 (2007)]

  4. A second example? 7.8 msec0.4 JyNearly in theGalactic plane 1206.4135

  5. New mERBs (aka FRBs) Four new bursts discovered.Now it is clear that we deal with a class of events. Origin – unknown:- magnetars- GRBs- SN- WD or NS merging - Supramassive NSs- Normal stars bursts- Primordial BHs Flux ~ 1 Jy, Fluence ~ (0.6-8) Jy ms Eradio~1038-1040 erg DM~550-1100, z~0.5-1, d~1.7-3.2 Gpc|b|>41oRate ~104+/-0.5 d-1 sky-1 up to ~3 Gpc(~100-1000 per cubic Gpc per day) 1307.1628

  6. Hypotheses • Supramassive NSs (Falcke & Rezzolla, Zhang) • WD+WD (Kashiyama et al.) • Dwarf stars (Loeb et al.) • GRBs (Zhang) • NS+NS merger (Totani) • Primrdial BHs (Keane et al.) • In all models it is expected that emission is coherent (see Katz 2013).Brightness temperature is very high: >~1034 K. Resume: “Radio Bursts, Origin Unknown” James Cordes Sci. 341, 40 (2013)

  7. A hypothesis:hyperflare of an extragalactic magnetar We note that the rate about 100 per day per cubic Gpc is about the expected rate of extragalactic hyperflares of magnetars. The possible mechanism of radio emission can be related to the tearing mode instability in the magnetar magnetosphere as discussedby Lyutikov (2002) and can produce the radio flux corresponding to the observed 30 Jy from the mERB using a simple scaling of the burst energy. Popov, Postnov arXiv:0710.2006 “Hyperflares of SGRs as an engine for millisecond extragalactic radio bursts “

  8. Rate of hyperflares Popov, Stern (2006) estimated the rate of hyperflares per galaxy ~1/1000 yrs. Lazzati et al. (2005) provide an estimate somehow larger <1/130 yrs, But this is an upper limit.THis results are based on no detection of SGR bursts by BATSEtowards local galaxies and Virgo cluster. These values are 5-50 times lower than the galactic rate of SN. So, the rate of hyperflares is expected to be ~20-200 per year per cubic Gpc. This is in good correspondence with the estimate of mERBs rate. There are candidate bursts in local galaxies:M81 group of galaxies: M81 itself, M82, M83(Frederiks et al. 2005) Now there are few other candidates (Mazets et al., Frederiks et al., Golenetskii et al., Ofek et al, Crider ....), including one in the direction of M31.

  9. Radio emission Lyutikov (2002) proposed that a standard (weak) burst of a SGRproduce a radio burst with a flux at ~1 GHz ~1 Jy from 10 kpc for a burst with Lx~1036 erg/s. For Lx=1047 erg/s and distance 600 Mpc we obtain ~30 Jyin excellent correspondence with data on mERB. The model is based on analogy with solar bursts.If so, then reconnection in a NS magnetosphere is the cause of mERBs.

  10. Timing properties The raising part of the burst 27 Dec 2004 was about 5 msec. This is about what was observed for the mERB. However, the duration of a radio burst in the model by Lyutikovcan be even smaller, down to tens of microseconds (tA~RNS/c). This does not contradict data on the mERB.

  11. Discussionon the “Lorimer burst” 1. No GRB was detected at the time of mERB This is natural as a hyperflare is undetectable from ~600 Mpc. 2. Host galaxy. SGRs are expected to be related to starformation sites. So, the host galaxy can be a starforming galaxy with dust. Then it can be closer than 600 Mpc. Observations by Spitzer are welcomed. 3. Birth of a magnetar. We note, that the rate is also coincident with an expected birthrate of SGRs. However, no corresponding SN was detected. So, this is unlikely. 4. Testing of the model by Lyutikov. We want to encourage observers to look for millisecond radio bursts coincident with weak bursts of galactic magnetars.

  12. New data • In our opinion, new data provide additional support for the magnetar hypothesis.- The rate is slightly higher than suggested by Lorimer et al., but still in good correspondence with the magnetar hypothesis. • New flux measurements are in good correspondence with earlier estimates. We need a detailed physical model of emission! 1307.4924

  13. Bursts from M31 Recently (Rubio-Herrera et al. 2013) bursts from M31 have been reported. ~1-4 Jy, millisecond duration. In one case, probably, repetitions.Compatible with magnetar activity in M31 It is necessary to assume thatone of magnetars in M31 was in active phase during observations.If so, the rate of bursts will bemuch different in future observations.

  14. Questions to plasma physics • How to produce bursts:- millisecond • coherent emission- relativistic plasma- propagation of emission • no bright long companions • at other wavelengths Reconnection?Non-linear phenomenain relativistic plasma?………..?

  15. Lyubarsky’s model Recently, Yuri Lyubarski presented a model for FRBs based on magnetars. The mechanism is:synchrotron maser emission from relativistic, magnetized shocks Two shock waves (forward and reverse)are formed after the magnetized pulsereaches the magnetar nebula.Both shock waves can result in maseremission. nebula Magnetized pulse In addition, the forward shock can also produce high-energy (TeV) emission.This prediction can be used to verifythe model. 1401.6674

  16. Kulkarni et al. analysis This authors discuss all proposed explanations for FRBsstarting with perytons – local events. Still, they can be an option.It is necessary to have more observations, in particular to havesimultaneus observations of flares by (at least two) different telescopes.The Galactic origin is absolutely ruled out (see also Tuntsov 2014).Finally, extragalactic origin seems to be more natural. After careful analysis of different possibilities, the authors favour the model related to giant flares of magnetars.We have situation similar to that with GRBs in 70s-90s! 1402.4766

  17. Conclusions • A new class of radio bursts is now established. FRBs • Origin is unknown • Galactic is excluded • Atmospheric is possible, but requiers ad hoc assumptions • Extragalactic origin seems to be the most natural • A theoretical model exists, still more studies are necessary • New radio observations a requiered to rule out atmospheric origin • Multiwavelength detection is very much desired

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