| pp-waves in modi ed gravity | AHMET BAYKAL | 77–112 |
| pp-waves in modified gravity | Ahmet BAYKAL | 77–112 |
| Supergravity backgrounds and symmetry superalgebras | Ümit ERTEM | 113–126 |
| Supergravity backgrounds and symmetry superalgebras | Umit ERTEM | 113–126 |
| Neutron stars: compact objects with relativistic gravity | KAZIM YAVUZ EKŞİ | 127–138 |
| Neutron stars: compact objects with relativistic gravity | Kazım Yavuz EKŞİ | 127–138 |
| Exact solutions to the geodesic equations of linear dilaton black holes | Alan Hameed Hussein HAMO,İZZET SAKALLI | 139–145 |
| Exact solutions to the geodesic equations of linear dilaton black holes | İzzet SAKALLI, Alan Hameed Hussein HAMO | 139–145 |
| Structure and stability of primordial stars | Aysel KARAFİSTAN İBRAHİM | 146–149 |
| Structure and stability of primordial stars | Aysel KARAFİSTAN İBRAHİM | 146–149 |
| The observational status of simple in ationary models: an update | Nobuchika OKADA,VEDAT NEFER ŞENOĞUZ,Qaisar SHAFI | 150–162 |
| The observational status of simple inflationary models: an update | Nobuchika OKADA, Vedat Nefer ŞENOĞUZ, Qaisar SHAFI | 150–162 |
| Revisiting the dyonic Majumdar{Papapetrou black holes | Seyedhabibollah MAZHARIMOUSAVI,Mustafa HALİLSOY | 163–174 |
| Revisiting the dyonic Majumdar-Papapetrou black holes | Seyedhabibollah MAZHARIMOUSAVI, Mustafa HALİLSOY | 163–174 |
| It is sufficient to set the cosmological constant to zero or to a small number at aninitial time | RECAİ ERDEM | 175–179 |
| It is sufficient to set the cosmological constant to zero or to a small number at an initial time |