International Conference on Astrophysics and Particle Physics December 08-10, 2016 Dallas, USA

ConferenceSeries LLC Ltd Conferences invites all the participants from all over the world to attend “International conference on Astrophysics and Particle Physics” during December 8-10, 2016, Dallas, USA which includes prompt keynote presentations, Oral talks, Poster presentations and Exhibitions.

Particle Physics 2016 aims to bring together a multi-disciplinary group of scientists and engineers to present and exchange breakthrough ideas relating to Early Universe, Dark Matter and Dark Energy, Gravitational Physics, Particle and Nuclear Astrophysics, Large-Scale Structures, Stellar Formation and Evolution, Observational Astronomy and Astrophysics, Celestial Mechanics, Theoretical Astronomy and Astrophysics, Astronomy Subfields,Interdisciplinary Studies, Space Observation and Exploration,Structure and Evolution of the Cosmos, Unsolved Problems in Astronomy.It promotes top-level research and to globalize the quality research in general, thus making discussions, presentations and contributions more internationally competitive.

Track 1: Astrophysics

Theoretical astronomy is the study of the analytical models of physics and chemistry to observe and analyse astronomical objects and astronomical phenomena. Theoretical astronomers use a wide range of tools which consists of Analytical models and Computational numerical simulations.

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Track 2: Astronomy

After the big bang, the universe was extremely hot and dense. As the universe cooled, conditions became just right to give rise to the building blocks of matter – the quarks and electrons of which we are all made. The first galaxies began to form half a billion to 1 billion years after Big Bang. Finding such galaxies has been a challenge because their light is so faint, which makes the discovery of a 13.2 billion-year-old galaxy.

Solar physics: Because the Sun is uniquely situated for close-range observing (other stars cannot be resolved with anything like the spatial or temporal resolution that the Sun can), there is a split between the related discipline of observational astrophysics (of distant stars) and observational solar physics. The study of solar physics is also important as it is believed that changes in the solar atmosphere and solar activity can have a major impact on Earth's climate. The Sun also provides a "physical laboratory" for the study of plasma physics

Planetary physics: Galileo's study of the lunar mountains in 1609 also began the study of extra-terrestrial landscapes: his observation "that the Moon certainly does not possess a smooth and polished surface" suggested that it and other worlds might appear "just like the face of the Earth itself". Advances in telescope construction and instrumental resolution gradually allowed increased identification of the atmospheric and surface details of the planets. The Moon was initially the most heavily studied, as it always exhibited details on its surface, due to its proximity to the Earth, and the technological improvements gradually produced more detailed lunar geological knowledge. In this scientific process, the main instruments were astronomical optical telescopes (and later radio telescopes) and finally robotic exploratory spacecraft. The Solar System has now been relatively well-studied, and a good overall understanding of the formation and evolution of this planetary system exists. However, there are large numbers of unsolved questions, and the rate of new discoveries is very high, partly due to the large number of interplanetary spacecraft currently exploring the Solar System.

Stellar Astronomy is a branch of Astronomy. It studies the general regularities in evolution, structure, composition and dynamics of stellar system.  Galactic Astronomy is the study of our own Milky Way galaxy. Extragalactic Astronomy is the study of everything outside the Milky Way. Cosmology is the scientific study of the large scale properties of the universe as a whole. It endeavours to use the scientific method to understand the origin, evolution and ultimate fate of the entire Universe. Cosmology involves the formation of theories or hypotheses about the universe which make specific predictions for phenomena that can be tested with observations. Depending on the outcome of the observations, the theories will need to be abandoned, revised or extended to accommodate the data. The prevailing theory about the origin and evolution of our Universe is the so-called Big Bang theory.

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Track 3: Cosmology and Celestial Mechanics

Our universe is both ancient and vast, and expanding out farther and faster every day. This accelerating universe, the dark energy that seems to be behind it and other puzzles like the exact nature of the Big Bang and the early evolution of the universe are among the great puzzles of cosmology. Dramatic advances in observational cosmology since the 1990s, including the cosmic microwave background, distant supernovae and galaxy redshift surveys, have led to the development of a standard model of cosmology. This model requires the universe to contain large amounts of dark matter and dark energy whose nature is currently not well understood, but the model gives detailed predictions that are in excellent agreement with many diverse observations. The branch of Astronomy which deals with the motion of Celestial bodies is known as Celestial mechanics.  Celestial mechanics uses the principles of physics (classical mechanics) to astronomical objects, such as stars and planets, to produce ephemeris data. As an Astronomical field of study, celestial mechanics includes the sub-fields of Orbital mechanics and lunar theory.  Orbital mechanics deals with the orbit of an artificial satellite and lunar theory, which deals with the orbit of the Moon.

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Track 4: Gravitational Physics

Gravity is most accurately described by the general theory of relativity (proposed by Albert Einstein in 1915) which describes gravity, not as a force, but as a consequence of the curvature of space-time caused by the uneven distribution of mass/energy; and resulting in time dilation, where time lapses more slowly in strong gravitation. Gravitational physicists explore the implications of the general theory of relativity. Modern research in gravitational physics includes studying applications of numerical relativity, black hole dynamics, sources of gravitational radiation, critical phenomena in gravitational collapse, the initial value problem of general relativity, and relativistic astrophysics.

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Track 5: Dark Matter and Dark Energy

Dark matter is a hypothetical kind of matter that cannot be seen with telescopes but would account for most of the matter in the universe. Atoms make up only 4.6% of the universe. The rest of the universe appears to be made of a mysterious, invisible substance called dark matter (25 %) and a force that repels gravity known as dark energy (70 %).

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Track 6: Stellar Formation and Evolution

The stars in the sky seem permanent and unchanging because it takes millions of billions of years for their lives to unfold. Stars are born in clusters within huge nebulas called star-forming regions. There, dark clouds of gas and dust collapse to form new stars.

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Track 7: Astrophysics and Space Science

With the development of rockets and the advances in electronics and other technologies in the 20th century, it became possible to send machines and animals and then people above Earth’s atmosphere into outer space. Well before technology made these achievements possible, however, space exploration had already captured the minds of many people, not only aircraft pilots and scientists but also writers and artists. In the 2000s, several plans for space exploration were announced; both government entities and the private sector have space exploration objectives. China has announced plans to have a 60-ton multi-module space station in orbit by 2020.

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Track 8: Telescopes

A telescope is an instrument that aids in the observation of remote objects by collecting electromagnetic radiation (such as visible light). The first known practical telescopes were invented in the Netherlands at the beginning of the 17th century, using glass lenses. They found use in terrestrial applications and astronomy.

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Track 9: Observational Large-Scale Structures

Observational astronomy is one of the classifications of the astronomical science that is related with recording data, in contrast with Theoretical astrophysics, which is mainly concerned with finding out the measurable implications of physical models. It is the practice of observing celestial objects by using telescopes and other astronomical apparatus. Radio astronomy is the branch of Astronomy which studies celestial bodies at Radio Frequencies. Infrared astronomy is the division of astronomy and astrophysics that studies astronomical objects visible in infrared (IR) radiation only. Optical Astronomy is also called as Visible Light Astronomy. Ultraviolet astronomy is the observation of electromagnetic radiation at ultraviolet wavelengths similarly X-ray Astronomy uses X-rays and Gamma ray Astronomy uses Gamma rays. Sky surveys and mappings of the various wavelength bands of electromagnetic radiation have yielded much information on the content and character of the universe's structure. The organization of structure appears to follow as a hierarchical model with organization up to the scale of super clusters and filaments.

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Track 10: Particle Physics

Particle physics is the study of nature of the particles that institute matter and radiation. It deals with very small objects. Particle physics deals with the fundamental constituents of matter and their interactions. In the past several decades a huge amount of experimental information has been gathered, and many patterns and methodical features have been observed.

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Track 11: Nuclear and Particle Physics

Nuclear physics and Particle Physics is the area of physics that studies atomic nuclei and their elements and interactions. The most commonly known kind of nuclear physics is nuclear power generation, the research has run to tenders in many fields, including nuclear medication and magnetic reverberation imaging, nuclear weapons, ion implantation in materials engineering, and radiocarbon dating in geology and archaeology.

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Track 12: Experimental Particle Physics

The experimental particle physics is to study the fundamental constituents of matter and their interaction. These activities are carried out in teamwork with international laboratories, where fundamental physics results are obtained. To study further, it is developing future detector technologies for experimentation, and computer grids for analysis of data.

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Track 13: The Future of Particle Physics

The clear and common top importance was to get all the vast science. we started the Large Hadron Collider (LHC) in 2015 and collide beams at close to its design energy of 14 TeV. The fact that we already achieved to discover the Higgs boson with beams colliding at 7 and 8 TeV is a great success. The LHC can continue delivering amazing physics from the energy frontier for two more decades.

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Track 14: Unsolved Problems in Astrophysics and Particle Physics

There are many unsolved problems in Astrophysics and Particle Physics. Some of them are Corona, Dark Energy, Dark Matter, Diffuse Interstellar Bands, Extra-terrestrial Life, Fermi Paradox, M-Sigma Relation, Mass in General Relativity, Shape of the Universe, Ultra-High-Energy Cosmic Ray, Large hadron collider, Higgs boson and Unidentified Infrared Emission, Wow! Signal.

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