• Sonuç bulunamadı

Charged de Sitter-like black holes: quintessence-dependent enthalpy and new extreme solutions

N/A
N/A
Protected

Academic year: 2021

Share "Charged de Sitter-like black holes: quintessence-dependent enthalpy and new extreme solutions"

Copied!
13
0
0

Yükleniyor.... (view fulltext now)

Tam metin

Şekil

Fig. 2 Plots of y = 1 − 2Mu + q 2 u 2 (dashed line) and y = 2cu 3 ω+1 (continuous line) for q 2 > M 2 and −2 ≤ 3ω+1 < 0
Fig. 3 Plots of y = 1 − 2Mu + q 2 u 2 (dashed line) and y = 2cu 3 ω+1 (continuous line) for q 2 = 9ω 2 M 2 /(9ω 2 − 1) > M 2 and −2 ≤ 3ω + 1 < 0

Referanslar

Benzer Belgeler

The Dirac equation is solved in the near horizon limit geometry of an extreme Kerr black hole.. We decouple equations first, as usual, into an axial and

Generally immunotherapy functions through a mechanism which prevents evasion of tumor cells from immune system as a result of blockade of cellu- lar checkpoints induced

Managing people can be a burdensome responsibility and it is important that anyone undertaking the role of Event Director has the capability and personality to deal effectively

Extensive property is the one that is dependent on the mass of the system such as volume, kinetic energy and potential energy.. Specific properties are

In both cases E is the energy constant and dot represents the appropriate parameter for the null geodesics. As a prediction of the HK conjecture any exact back-reaction solution that

Marmara Üniversitesi’nde lisans programında Genel Jeoloji, Mineral ve Kayaçlar, Hidrografya, Yapısal Jeomorfoloji, Coğrafya Araştırmaları, Türkiye Hidrografyası,

Uluslararası Türk Folklor Kongresi Başkan­ lığına bir önerge verilerek, Baş- göz ve Boratav’ın kongreden çı­ karılmalarının gerekçesi sorul­

e'laaşı bugünkü cumartesi günü saat l a de Osmanbeyde Şair Nigftr sokağında Fe- rldlye apartımanından kaldırılarak cenaze namazı Teşvikiye camiinde