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Bizning manzil
O’zbekiston, 100052
Toshkent shahri
Astronomiya ko’chasi, 33-uy
Tel: +998 71 235-81-02
Faks: +998 71 234-48-67
E-mail: info@astrin.uz
Relyativistik astrofizika va gravitatsiya
Konferensiyaga ro'yxatdan o'tish uchun havolaga o'ting ...
Konferensiya fayllari- dastur, qatnashchilar ro'yxati, fotosuratlar ...
Bog’lanish: asmik96@astrin.uz

2021-yil 12-14 may kunlari O’zR FA Astronomiya instituti hamda O’zR FA Yadro fizikasi instituti hamkorligida «Relyativistik astrofizika va gravitatsiya» mavzusida, onlayn formatida xalqaro miqyosidagi ilmiy seminar (IWRAG-2021) o’tkazilishi rejalashtirilmoqda.

Seminardan ko’zlangan maqsad – umumiy nisbiylik nazariyasi va relyativistik astrofizika sohasiga ixtisoslashgan mintaqaviy (Markaziy Osiyo) astrofiziklarni hamda xalqaro ilmiy hamjamiyatni birlashirish, shuningdek erishilgan natijalarni o’zaro almashib, xalqaro institutlar bilan aloqalarni kengaytirish imkonini berish. IWRAG-2021 Toshkentda, O’zbekistonda muntazam tashkillashtirilishi rejalashtirilayotgan birinchi seminarlar seriyasi bo’lishi, shuningdek talabalar va shu sohaga ixtisoslashgan olimlar uchun ajoyib imkoniyatlar taqdim etishi kutilmoqda. Seminar doirasida relyativistik astrofizika sohasidagi xalqaro tadqiqotlar, O'zbekiston Respublikasi astronomiya va yadro fizikasi institutida davlat ilmiy - texnika dasturlari doirasida olib borilayotgan fundamental tadqiqotlar natijalari haqida ma'ruzalar o'qiladi.
Konferensiya dasturi
SOC/LOC
International Advisory Committee

Bobomurat Ahmedov (AI, Uzbekistan)

Daniele Malafarina (Nazarbayev University, Kazakhstan)

Ernazar Abdikamalov (Nazarbayev University, Kazakhstan)

Medeu Abishev (Al-Farabi University, Kazakhstan)

Ashfaque Bokhari (King Fahd University of Petroleum & Minerals, Saudi Arabia)

Ugur Camci (Roger Williams University, USA)

Naresh Dadhich (IUCAA, India)

Viktoriya Morozova (PennState, USA)

Luciano Rezzolla (Frankfurt, University, Germany)

Sushant Ghosh (Centre for Theoretical Physics, India)

Jutta Kunz (Oldenburg University, Germany)

Ahmadjon Abdujabbarov (AI, Uzbekistan)

Bobir Tosmatov (AI, Uzbekistan)

Farrukh Fattoyev (NY University, USA)

Cosimo Bambi (Fudan University, China)

Wenbiao Han (ShAO, China)

Zdenek Stuchlik (Opava, Czech Republic)

Martin Kolos (Opava, Czech Republic)

Asqar Qadir (Islamabad, Pakistan)

Francesco de Paolis (Lecce, Italy)

Mariafelicia De Laurentis (Napoli, Italy)

Muhammad Sharif (Punjab University, Pakistan)

Mubasher Jamil (China)

Local Organizing Committee

Ahmedov Bobomurat, Chairman

Abdujabbarov Ahmadjon

Toshmatov Bobir

Tursunov Arman

Abdikamalov Askar

Tojiev Sardor

Shaymatov Sanjar

Atamurotov Farruh

Mardonov Shuhrat

Rayimbaev Djavlanbek

Boboqambarova Madina

Rahimov Ozodbek

Ro'yxatdan o'tgan qatnashchilar (9)
Турсынбек Ерназаров
Mamlakat: Казахстан | Taqdimot turi: Poster
Taqdimot nomi: «слушатель»
Tashkilot: «КазНУ имени аль-Фараби»
Qisqacha ma'lumot (abstrakt) ... слушатель
Mubasher Jamil
Mamlakat: China | Taqdimot turi: Plenary talk
Taqdimot nomi: «NA»
Tashkilot: «Zhejiang University of Technology»
Qisqacha ma'lumot (abstrakt) ... NA
Bobomurat Ahmedov
Mamlakat: Uzbekistan | Taqdimot turi: Plenary talk
Taqdimot nomi: «Development and Perspectives of Relativistic Astrophysics in Uzbekistan»
Tashkilot: «Ulugh Beg Astronomical Institute»
Qisqacha ma'lumot (abstrakt) ... I will discuss successful development and establishment of scientific group specialized in general relativity and relativistic astrophysics in Uzbekistan. Summary of scientific results performed on the study in Uzbekistan in relativistic astrophysics of compact gravitational objects will be provided.
Viktoriya Giryanskaya
Mamlakat: USA | Taqdimot turi: Contributed talk
Taqdimot nomi: «The gravitational wave signal from core-collapse supernovae»
Tashkilot: «Pennsylvania State University»
Qisqacha ma'lumot (abstrakt) ... We study gravitational waves (GWs) from a set of two- and three-dimensional multi-group neutrino radiation hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to systematize the current knowledge about the post-bounce CCSN GW signal and recognize the templatable features that could be used by the ground-based laser interferometers. We demonstrate that starting from ~400ms after core bounce the dominant GW signal represents the fundamental quadrupole (l=2) oscillation mode (f-mode) of the proto-neutron star (PNS), which can be accurately reproduced by a linear perturbation analysis of the angle-averaged PNS profile. Before that, in the time interval between ~200 and ~400ms after bounce, the dominant mode has two radial nodes and represents a g-mode. We associate the high-frequency noise in the GW spectrograms above the main signal with p-modes, while below the dominant frequency there is an `excluded region' with very little power. Weak dependence of the dominant GW frequency on the progenitor mass motivates us to provide a simple fit for it as a function of time, which can be used as a prior when looking for CCSN candidates in the LIGO data.
Ernazar Abdikamalov
Mamlakat: Kazakhstan | Taqdimot turi: Plenary talk
Taqdimot nomi: «Explosions of massive stars»
Tashkilot: «Nazarbayev University»
Qisqacha ma'lumot (abstrakt) ... Core-collapse supernovae are the powerful explosions of massive stars that happen at the end of their lives. They play an important role in the evolution of the universe, enriching galaxies with heavy elements and giving birth to neutron stars and, in some cases, black holes. Despite their importance, the exact details of how they explode remain uncertain. In this talk, I will review our current understanding of the explosion mechanism with a particular emphasis on the role of multi-dimensional hydrodynamic instabilities.
DR. RABIA SALEEM
Mamlakat: Pakistan | Taqdimot turi: Contributed talk
Taqdimot nomi: «Study of Interacting Dark Sectors using Chevallier-Polarsky-Linder Type Parametrization»
Tashkilot: «COMSATS University Islamabad, Lahore Campus»
Qisqacha ma'lumot (abstrakt) ... The main focus of this paper is to investigate an interacting phenomena between dark matter-dark energy within a non-flat FLRW spacetime geometry bounded by a horizon with specific cut-off. We assume an interaction term $Q(z)$ between two dark components of the fluid and evaluate it analytically via physical quantities like energy density and pressure. We constraint the model parameters and found specific region of validity for these parameters. Considering ``Chevallier-Polarsky-Linder type parametrization" of the coincidence parameter $r(z)$, we observed that our model possess a future singularity of Type III. After finding the singular behavior, we examine the nature of our model via cosmological parameters like $q,~r,~s$. It is noted that our model is very close to $\Lambda$ cold dark matter model.
Zoha Tariq
Mamlakat: Pakistan | Taqdimot turi: Plenary talk
Taqdimot nomi: «Effects of electromagnetic field on the structure of massive compact objects»
Tashkilot: «University of the Punjab»
Qisqacha ma'lumot (abstrakt) ... This paper encompasses a set of stellar equations that administer the formation and evolution of self-gravitating, dissipative spherically symmetric fluid distributions having anisotropic stresses in the presence of electromagnetic field. The Riemann tensor is split orthogonally to procure five scalar functions named as structure scalars which are then utilized in the stellar equations. It is shown that some basic fluid properties such as energy density inhomogeneity, pressure anisotropy and heat flux are interlinked with the obtained scalars. Further, it is shown that all the solutions to Einstein equations can be written in terms of these five scalars keeping in view the static case.
Zoha Tariq
Mamlakat: Pakistan | Taqdimot turi: Plenary talk
Taqdimot nomi: «Effects of electromagnetic field on the structure of massive compact objects»
Tashkilot: «University of the Punjab»
Qisqacha ma'lumot (abstrakt) ... This paper encompasses a set of stellar equations that administer the formation and evolution of self-gravitating, dissipative spherically symmetric fluid distributions having anisotropic stresses in the presence of electromagnetic field. The Riemann tensor is split orthogonally to procure five scalar functions named as structure scalars which are then utilized in the stellar equations. It is shown that some basic fluid properties such as energy density inhomogeneity, pressure anisotropy and heat flux are interlinked with the obtained scalars. Further, it is shown that all the solutions to Einstein equations can be written in terms of these five scalars keeping in view the static case.
Muhammad Zaeem Ul Haq Bhatti
Mamlakat: Pakistan | Taqdimot turi: Contributed talk
Taqdimot nomi: «Dynamical Analysis of Self-gravitating Objects in Modified Gravity»
Tashkilot: «University of the Punjab»
Qisqacha ma'lumot (abstrakt) ... TBA
Ulug’bek nomidagi Astronomiya instituti,