FP7Индивидуална стипендия2015–2016

ASTROGRAPHY · Gravity, Fundamental Physics and Astrophysics: The Missing Link

7РП — „Хора“ (Действия „Мария Кюри“)

Период
2015-01-01 → 2016-12-31
Финансиране от ЕС
179 740 €
Участници
1
Схема
MC-IEF

Линиите свързват координатора с партньорите.

Накратко на български

Гравитационните взаимодействия при черни дупки и неутронни звезди се анализират чрез нови теоретични модели за тяхната деформираемост. Това помага за по-точното изчисляване на ефектите от въртенето на тези обекти при засичането на гравитационни вълни.

Този кратък обзор е генериран от изкуствен интелект

Кратко обяснение, генерирано от езиков модел по текста на CORDIS. Оригиналът е по-долу.

Резултати накратко

Gravity, Fundamental Physics and Astrophysics: The Missing Link

Einstein's general relativity has different faces. On the one hand it presents itself as a beautiful theory which describes how matter/energy interacts with the geometry of spacetime at fundamental level. On the other hand it aims at describing all gravitational interactions at stellar, galactic and cosmological scales. Accordingly, fundamental aspects of gravitational interactions and their astrophysical implications are usually investigated by different communities. New precision observations of compact objects (black holes and neutron stars) and the imminent advent of gravitational-wave astronomy provide us with the unique opportunity to merge these disjoint efforts, and to test fundamental physics with astrophysical observations to unprecedented level. We are now entering the exciting era in which new observations can be used make contact between relativistic astrophysics and fundamental questions. The goal of this project was to connect this missing link. Some of the major outcomes of this project are: 1) We developed a new theoretical formalism to study the deformability of spinning relativistic compact objects within general relativity. We proved that the so-called “Love numbers” of a spinning black hole are precisely zero up to second order in the spin. Furthermore, we computed for the first time the Love numbers for a spinning neutron star within general relativity. These results have important implications to estimate the effect of rotation in the context of gravitational-wave astronomy with advanced detectors (aLIGO, aVIRGO, KAGRA). 2) We investigated possible strong-field tests of general relativity with present and future astrophysical observations. In particular, the scientist in charge and the principal researcher are two of the main authors of a Topical Review recently published by Classical and Quantum Gravity. The principal researcher has been Guest Editor for a Focus Issue “Black holes and Fundamental Fields” published on this topic. 3) We investigated the superradiant instability of spinning black holes in the presence of light bosonic fields. These results, together with astrophysical observations of spinning black holes, can be used to put constraints on light dark-matter candidates (see Figure 2 in the attached document). The principal researcher was the co-author of a monograph published by Springer in 2015 on this subject. Overall, the results of this project can have an impact both for gravitational-wave astronomy and for fundamental physics and make a strong case for the key role that compact objects play in various areas of research, ranging from astrophysics to particle physics. The outcomes of this project include 9 scientific papers published in leading internation peer-reviewed journals, 1 monograph published by Springer, 1 Topical Review published in Classical and Quantum Gravity, 1 Focus Issue published in Classical and Quantum Gravity, and 2 conference proceedings. Results have been disseminated at various international conferences and workshops, including the 14th Marcel Grossmann Meetings at Sapienza (Italy) and the International Conference on Black Holes at the Fields Institute (Canada), and through invited plenary talks in leading research institutes, including the Albert Einstein Institute (Germany) and Fudan University (China). An international conference, two international workshops [including a workshop supported by the Lorentz Center (Netherlands)], and a parallel session at the 14th Marcel Grossmann were organized on the topics of this project. All numerical codes developed and used during this project are publicly available at the webpage http://paolopani.weebly.com and the original papers are Open Access through the ArXiv database (http://www.arxiv.org). The principal researcher has served as senior teaching assistant for the “Electromagnetism” course in Physics at Sapienza (duties included ~3hr/week of lectures, oral evaluations and preparing and correcting exams), as the co-advisor of a PhD student (Richard Brito) and as the advisor of a master student.

Текст от CORDIS, на английски · Данни: CORDIS, © Европейски съюз

Цел на проекта

New precision observations of compact objects and the imminent advent of gravitational-wave (GW) astronomy provide us with the unique opportunity to test fundamental physics with astrophysical observations to unprecedented level. Neutron stars (NSs) and black holes (BHs) can be used as cosmic labs where matter in extreme conditions, particle physics, and even the very foundations of Einstein's theory can be put to the test. Triggered by recent breakthroughs at various levels, the area of strong gravity is experiencing a second Golden Age. In parallel with novel electromagnetic observations, advanced GW observatories in Europe and USA will open new windows to the unexplored strong-gravity regime and will finally shed light on the properties of ultradense matter in NS cores. The potential of GW astrophysics is enormous and far to be fully explored. Counterintuitive effects taking place near isolated compact objects have been recently discovered, but their GW signatures in realistic environment remain to be investigated. We are now in the exciting position of using observations to make contact between relativistic astrophysics and fundamental questions. The goal of our innovative project is to connect this missing link. We propose to investigate strong-gravity effects via precision GW phenomenology. In particular we aim to: 1) Develop semianalytical methods to study NS-NS binaries and spinning isolated NSs, and to constrain the behavior of matter at nuclear density using GW observations; 2) Develop a model-independent framework to study GW signatures of accretion onto massive BHs; 3) Investigate the interplay between “BH bomb” instabilities and accretion in the context of puzzling phenomena, such as jet emission or gamma-ray bursts; 4) Constrain dark matter candidates by studying their interaction with BHs and NSs in realistic scenarios. Our proposal is located at the interface between astrophysics and fundamental physics and can have a profound impact for both.

Оригинален текст от CORDIS (на английски).

Участници

  • UNIVERSITA DEGLI STUDI DI ROMA LA SAPIENZA · RomaКоординаторИталия

Връзки

Данни: CORDIS, © Европейски съюз