- The Complete Research Material is averagely 52 pages long and it is in Ms Word Format, it has 1-5 Chapters.
- Major Attributes are Abstract, All Chapters, Figures, Appendix, References.
- Study Level: BTech, BSc, BEng, BA, HND, ND or NCE.
- Full Access Fee: ₦4,000
Get the complete project »

CHAPTER ONE
INTRODUCTION
Background to the study
Astrophysical jets are observed in the Universe in a large variety of environments and under a wide range of sizes and powers. They are generated in active galactic nuclei (AGNs) and YSOs, can travel up to a few thousands of Megaparsecs, and reach the largest powers observed in the Universe (up to ∼1047−48 erg s−1), (Zanni et al., 2003; Godfrey and Shabala, 2013). Astrophysical jets can be found in giant molecular clouds, emanating in the vicinities of young stellar objects (YSOs), and reaching distances of some parsecs (Reipurth and Bally, 2001). They are also located near neutron stars in galactic X-ray binary star systems, such as GRS 1915 + 105 that behave as microquasars generating relativistic jets (Fender, 2004). Astrophysical jets can be found in the asymptotic giant branch (post-AGB) stars as well in pre-planetary and planetary nebulae. Opposite, precessing jets are observed in the SS433 binary source, leading to a peculiar phenomenology (Frank, 2011). A jet-like structure is observed, at X-ray energies, inside the Crab Nebula departing from the embedded pulsar (Hester, 2008). Finally, jets can be at the base of the phenomenology of gamma-ray bursts, observed at the highest radiation energies that are still elusive phenomena because of their extreme distances (Granot, 2007).
Statement of problem
In recent years, we have seen many laboratory experiments that try to reproduce some aspects of the jet phenomenology, with particular concern towards YSO jets. These aspects are mainly related to the jet origin, propagation, and emission (Bellan et al 2005, 2009, Falize et al 2011, Gregory et al 2008, González et al 2009, Hartigan et al 2009, Lebedev et al 2005, Suzuki-Vidal 2010, Rus et al 2002).
With the goal to address the propagation of YSO jets and their interaction with the ambient medium, Tordella et al (2011) (Paper I) and Belan et al (2013) (Paper II) studied in the laboratory and by numerical means hypersonic hydrodynamic (HD) flows. In Paper I the authors considered as main jet parameters the Mach number M and the jet-to-ambient density ratio η and studied, both experimentally and numerically, representative cases of high and small values of density ratio. In Paper II they analyzed several cases with Mach number and density ratios consistent with those derived from the observations of YSO jets.
Objective of the study
1. In this paper we focus our attention on the measure of the spreading of the laboratory jets and the comparison with the results obtained by numerical simulations.
2. We also discuss the appearance of sinuous structures observed in some laboratory jets and the extent to which these features may develop as the response to non-axial perturbations in numerical simulations.
Significance of the study
We discuss observations used to infer the presence of accretion disks in astrophysical sources and the disks’ association with evidence for astrophysical jets. We highlight some important results from past and current literature that show parallels between the temporal behavior of an active galaxy (NGC 5128) and a galactic microquasar (GRS 1915+105). In addition, we note the remarkable observations of the time history of SCO X-1 from VLBI data at radio frequencies.
You either get what you want or your money back. T&C Apply

You can find more project topics easily, just search
-
SIMILAR PHYSICS FINAL YEAR PROJECT RESEARCH TOPICS
-
1. APPLICATION OF RADIOMETRIC METHOD TO DETERMINE RADIOGENIC HEAT AROUND RAFIN REWA HOT SPRING, LERE, KADUNA STATE, NIGERIA
» ABSTRACT Detailed ground radiometric survey covering 400m x 400m of part of Lere sheet, Kaduna state, Nigeria was carried out. The research was aimed ...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
2. DATABASE EMISSION OF CARBON IV OXIDE (CO2) IN NIGERIA
» ABSTRACT There is a general believe today that the increased emission of green house gases especially carbon dioxides (CO2) which is believed to have ...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
3. A STUDY ON THE COMPETENCY OF PHYSICS STUDENTS IN THE USE OF INFORMATION COMMUNICATION TECHNOLOGY A CASE STUDY OF UNIVERSITY OF BENIN
» ABSTRACT This study investigates the competency of physics students in the use of information and communication technology in University of Benin (UNI...Continue Reading »Item Type & Format: Project Material - Ms Word | 64 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
4. ASSESSMENT OF OCCUPATIONAL EXPOSURE AND RADIATION PROTECTION IN SOME SELECTED WELL-LOGGING AND INDUSTRIAL RADIOGRAPHY FACILITIES IN NIGERIA
» ABSTRACT Nigeria has for a very long time engaged in the peaceful application of nuclear technology. The use of ionizing radiation due to its unique p...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
5. IMPLEMENTATION OF RUNGE KUTTA ALGORITHM IN SOLVING A RADIOACTIVE DECAY EQUATION USING MICROSOFT EXCEL
» ABSTRACT This project describes a differential equation of radioactive decay is numerically solved using the fourth order Runge Kutta method. In order...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
6. EFFECTS OF PRACTICAL THEORY ARRANGEMENTS ON THE ACHIEVEMENT OF PHYSICS STUDENTS’ IN THE CONCEPT OF SIMPLE PENDULUM IN SECONDARY SCHOOLS IN EKET LOC...
» Abstract The study aimed at comparing effects of practical theory arrangements on the achievement of physics students in secondary schools in Eket Loc...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
7. DESIGN OF SUN TRACKER FOR A PV SYSTEM
» CHAPTER ONE INTRODUCTION 1.1 BACKGROUND OF THE PROJECT A solar tracker is a device for orienting a photovoltaic array solar photovoltaic panel or conc...Continue Reading »Item Type & Format: Project Material - Ms Word | 30 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
8. EFFECTIVE COMMUNICATION BETWEEN RADIOGRAPHERS AND PATIENTS: INFLUENCE ON SERVICE DELIVERY AND PATIENT SATISFACTION.
» CHAPTER ONE 1.0 INTRODUCTION 1.1 BACKGROUND OF STUDY Communication is vital to good patient care in any discipline in the health domain and there is a...Continue Reading »Item Type & Format: Project Material - Ms Word | 59 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
9. FACTOR THAT DETERMINE THE IMPROVEMENT OF ELECTRICAL/ELECTRONICS TECHNICIANS IN TECHNICAL COLLEGES IN KADUNA STATE.
» CHAPTER ONE BACKGROUND OF THE STUDY Technical education dates back to the primitive days of man’s development in Nigerian when he realizes that ...Continue Reading »Item Type & Format: Project Material - Ms Word | 32 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT
-
10. ASSESSMENT OF RADIO-FREQUENCY RADIATION EXPOSURE FROM SELECTED MOBILE BASE STATIONS IN ZARIA AND ENVIRONS, NIGERIA
» ABSTRACT Base transceiver stations (BTS) or mobile base stations produce non ionizing (RF) energy that is radiated through its antennas into space. Th...Continue Reading »Item Type & Format: Project Material - Ms Word | 52 pages |
Instant Download | Chapter 1-5 | PHYSICS DEPARTMENT