ON DUALITY BETWEEN RESONANCES AND FREE QUARK-ANTIQUARK PAIRS

Author(s):  
J. S. BELL ◽  
J. PASUPATHY
Keyword(s):  
1981 ◽  
Vol 23 (4B) ◽  
pp. 743-753 ◽  
Author(s):  
M Basile ◽  
J Berbiers ◽  
G Cara Romeo ◽  
L Cifarelli ◽  
A Contin ◽  
...  

2001 ◽  
Vol 16 (13) ◽  
pp. 2435-2445 ◽  
Author(s):  
P. K. SAHU ◽  
S. K. PATRA

We study the effect of a strong magnetic field on interacting quark matter and apply the same to strange star. We find that interacting strange matter is less stable than noninteracting strange matter in the presence of a strong magnetic field. We then calculate strange star structure parameters such as mass and radius and find that the strange star is less compact for interacting quark matter than for free quark matter in presence of strong magnetic field. The maximum masses of strange stars are found to be within the recent observational limit.


Nature ◽  
1983 ◽  
Vol 303 (5918) ◽  
pp. 569-569
Author(s):  
John Maddox
Keyword(s):  

1979 ◽  
Vol 83 (3-4) ◽  
pp. 389-391 ◽  
Author(s):  
J.S. Bell ◽  
P. Pasupathy
Keyword(s):  

2000 ◽  
Vol 15 (1-4) ◽  
pp. 392-394
Keyword(s):  

1982 ◽  
Vol 48 (24) ◽  
pp. 1649-1652 ◽  
Author(s):  
A. Marini ◽  
I. Peruzzi ◽  
M. Piccolo ◽  
F. Ronga ◽  
D. M. Chew ◽  
...  
Keyword(s):  

2007 ◽  
Vol 22 (19) ◽  
pp. 3201-3209 ◽  
Author(s):  
WEI-MIN SUN ◽  
HONG-SHI ZONG

In this paper we propose a general method for calculating the partition function of QCD at finite chemical potential. It is found that the partition function is totally determined by the dressed quark propagator at finite chemical potential up to a multiplicative constant. From this a criterion for the phase transition between the Nambu and the Wigner phase is obtained. This general method are applied to two specific cases: the free quark theory and QCD with a model dressed quark propagator proposed in H . Pagels and S. Stokar, Phys. Rev. D20, 2947 (1979). In the first case, the standard Fermi distribution at T = 0 are reproduced. In the second case, a particular form of baryon number distribution is obtained. It is found that when μ is below a critical value, the baryon number density is identically zero, which agrees with the general conclusion in M. A. Halasz et al., Phys. Rev. D58, 096007 (1998). All the results in the present paper are obtained under the condition T = 0 and μ ≠ 0. However, they can be generalized to the the general situation T ≠ 0 and μ ≠ 0 without fundamental difficulty.


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