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R elativistic stellar clusters G. S. Bisnovatyi-Kogan (IKI, Moscow) ,

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R elativistic stellar clusters G. S. Bisnovatyi-Kogan (IKI, Moscow) ,. ГАИШ, пятница, 21 марта 2014. Вскоре после открытия квазаров с большим красным смещением :. =1 was considered by Zeldovich and Podurets (1965). Star Clusters with Cutoff. Comments on Astrophysics 1, 134, 1969. - PowerPoint PPT Presentation
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Relativistic stellar clusters G.S.Bisnovatyi-Kogan (IKI, Moscow), ГАИШ, пятница, 21 марта 2014
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Page 1: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Relativistic stellar clustersG.S.Bisnovatyi-Kogan (IKI, Moscow),

ГАИШ, пятница, 21 марта 2014

Page 2: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Вскоре после открытия квазаров с большим красным смещением:

Page 3: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

=1 was considered by Zeldovich and Podurets (1965)

Page 4: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Star Clusters with Cutoff

Page 5: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 6: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 7: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 8: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Comments on Astrophysics 1, 134, 1969

Page 9: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 10: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

GR5: Tbilisi, 9-13 September 1968Proceedings: None.Abstracts: GR5, abstracts of the 5th international conference on gravitation and the theory of relativity, ed. V.A. Fock et al. Tbilisi University Press (1968).

Page 11: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

MODELS OF CLUSTERS OF POINT MASSES WITH LARGE CENTRAL REDSHIFTS

G. S. Bisnovatyi-Kogan and Ya. B. Zel'dovich

Astrofizika, Vot. 5, No. 2, pp. 223-234, 1969

=2/a

0.006

r(g)/r=const~a

Page 12: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Isothermal star cluster in Newtonian limit

Page 13: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 14: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Variational principle

Page 15: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Relative binding energy E(b)/M is better for

stability analysis than M

Page 16: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Publications:

Earlier publications

Page 17: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Isolated cluster

Page 18: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

is the kinetic energy cutoff.

In the Newtonian limit, formally reduces to

Similarity between clusters in the box and clusters with cutoff

Newtonian cluster in box GR cluster with cutoff

Page 19: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

E(b)/N

W(0)=const, each extremum gives birth to new dynamically

unstable mode . At W(0)> 15.8 all models are stable.

Page 20: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Dynamic stability against perturbations with constant adiabatic invariants.

Equivalent to constant entropy for stability of gaseous star

Thermodynamic stability include processes leading to thermal equilibrium, smoothing temperature over the newtonian

cluster or star

Page 21: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Clusters with cutoff : ApJ (1998), 500, 217

Page 22: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Large central density (central redshift) regime loss of dynamic stability at T=0.06

Page 23: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

DU T U

S S

DS TUDU T U

S S

DS TU

Page 24: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Astro-ph 1403.3985

Page 25: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

Interpretation: GW from the inflation (Linde)

Page 26: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

A simplified model of the formation of structures in dark matterand a background of very long gravitational waves

G. S. Bisnovatyi-Kogan1,2

1Space Research Institute, Moscow, Russia, Profsoyuznaya 84/32, Moscow 117997, Russia

2Theoretical Astrophysics Center, Juliane Maries Vej 30, Dk-2100 Copenhagen Ø, Denmark

Mon. Not. R. Astron. Soc. 347, 163–172 (2004)

Page 27: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,
Page 28: R elativistic stellar clusters G. S. Bisnovatyi-Kogan  (IKI, Moscow) ,

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