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Is PSR B0943 10 a lowmass quark star

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... drifting pulsar. We focus on pulsar sub-pulse drifting and ... successful to sub-pulse drifting. space charge-limited flow (e.g., Arons & Scharlemenn 1979) ... – PowerPoint PPT presentation

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Title: Is PSR B0943 10 a lowmass quark star


1
Is PSR B094310 a low-mass quark star?
  • Youling Yue(???), Xiaohong Cui(???)
  • and Renxin Xu(???)
  • Astronomy department, Peking University
  • at Nanjing 2006.8

2
contents
  • Pulsar, neutron star, quark star
  • PSR B094310, quark star model, inclination angle
    effect
  • Conclusion

3
What is pulsar
  • Neutron star
  • Normal or Mixed/hybrid (quark core)
  • Quark star
  • Bare or with thin crust
  • Solid (stronger GW emission?) or fluid
  • Which one(s)??Observation

Bejger and Haensel 2003
4
Bejger and Haensel 2003
5
PSR B094310 (P 1 s), one of the best-studied
drifting pulsar
Deshpande Rankin 1999
6
  • We focus on pulsar sub-pulse drifting and polar
    gap model

7
Pulsar emission models
  • polar gap (e.g., Ruderman Sutherland 1975/RS75)
    successful to sub-pulse drifting
  • space charge-limited flow (e.g., Arons
    Scharlemenn 1979)
  • outer gap (e.g., Cheng et al. 1986)
  • core gap and annular gap (e.g., Qiao et al.
    2004)

8
Success of polar gap model (RS75)
e
e-
RS75
9
Edwards and Stappers 2002
10
To test the model
earth
hot spot In x-ray band
11
  • X-ray band observation (Zhang et al. 2005)
  • A_polar 103 m2 (observation)
  • A_polar 6x104 m2 (theory, for R10 km pulsar)

12
Zhang et al. 2005
13
To solve the problem
  • modification of polar gap model
  • a low mass bare strange quark star
  • small radius (R 2.6 km to fit the observation)
  • No binding energy problembinding energy of ion
    is nearly infinity (Xu Qiao 1999)

14
advantages
  • RS75
  • Only work when
  • the binding energy problem, need strong B
  • Our model
  • Work for both
  • Quark star has strong enough binding energy
    (binding by strong interaction)

gt 0
lt 0 and
15
Problems from potential drop
  • Philt 1012 V (critical potential drop)

Last open field line
0
16
Considering inclination angle
0
Last open field line
17
Results
18
Inclination angle
In the parameter space
rho 2rho_n
A 103 m2
Phi is well above 1012 V
19
conclusion
  • PSR B094310 could be a quark star.
  • The potential drop will be 100 times larger when
    considering inclination angle effects.

20
  • Thank you

21
Deshpande Rankin 2001
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