Physical Review is an American peer-reviewed scientific journal established in 1893 by Edward Nichols. It publishes original research as well as scientific and literature reviews on all aspects of physics. It is published by the American Physical Society (APS). The journal is in its third series, and is split in several sub-journals each covering a particular field of physics. It has a sister journal, Physical Review Letters, which publishes shorter articles of broader interest.
|Edited by||Michael Thoennessen (Editor in Chief)|
|1893–1913 Series I|
1913–1970 Series II
1970–present Series III
1970–present Phys. Rev. A, B, C, D
1993–present Phys. Rev. E
1998–present Phys. Rev. AB
2005–present Phys. Rev. PER
2011–present Phys. Rev. X
2014–present Phys. Rev. Applied
2016–present Phys. Rev. Fluids
2017–present Phys. Rev. Materials
Physical Review commenced publication in July 1893, organized by Cornell University professor Edward Nichols and helped by the new president of Cornell, J. Gould Schurman. The journal was managed and edited at Cornell in upstate New York from 1893 to 1913 by Nichols, Ernest Merritt, and Frederick Bedell. The 33 volumes published during this time constitute Physical Review Series I.
The American Physical Society (APS), founded in 1899, took over its publication in 1913 and started Physical Review Series II. The journal remained at Cornell under editor-in-chief G. S. Fulcher from 1913 to 1926, before relocating to the location of editor John Torrence Tate, Sr.[nb 1] at the University of Minnesota. In 1929, the APS started publishing Reviews of Modern Physics, a venue for longer review articles.
After Tate's death in 1950, the journals were managed on an interim basis still in Minnesota by E. L. Hill and J. William Buchta until Samuel Goudsmit and Simon Pasternack were appointed and the editorial office moved to Brookhaven National Laboratory on Eastern Long Island, New York. In July 1958, the sister journal Physical Review Letters was introduced to publish short articles of particularly broad interest, initially edited by George L. Trigg, who remained as editor until 1988.
In 1970, Physical Review split into sub-journals Physical Review A, B, C, and D. A fifth member of the family, Physical Review E, was introduced in 1993 to a large part to accommodate the huge amount of new research in nonlinear dynamics. Combined, these constitute Physical Review Series III.
The editorial office moved in 1980 to its present location across the expressway from Brookhaven National Laboratory. Goudsmit retired in 1974 and Pasternack in the mid-1970s. Past Editors in Chief include David Lazarus (1980–1990; University of Illinois at Urbana–Champaign), Benjamin Bederson (1990–1996; New York University), Martin Blume (1996–2007; Brookhaven National Laboratory), and Gene Sprouse (2007–2015; SUNY Stony Brook). The current Editor in Chief is Michael Thoennessen, whose term began in September 2017.
To celebrate the hundredth anniversary of the journal, a memoir was published jointly by the APS and AIP.
In 1998, the first issue of Physical Review Special Topics: Accelerators and Beams was published, and in 2005, Physical Review Special Topics: Physics Education Research was launched. In January 2016 the names of both journals were changed to remove "Special Topics". Physical Review also started an online magazine, Physical Review Focus, in 1998 to explain and provide historical context for selected articles from Physical Review and Physical Review Letters. This was merged into Physics in 2011. The Special Topics journals are open access; Physics Education Research requires page charges from the authors, but Accelerators and Beams does not. Though not fully open access, Physical Review Letters also requires an author page charge, although this is voluntary. The other journals require such a charge only if manuscripts are not prepared in one of the preferred formats. Authors can pay extra charges to make their papers open access. Such papers are published under the terms of the Creative Commons Attribution 3.0 License (CC-BY). Physical Review Letters celebrated their 50th birthday in 2008. The APS has a copyright policy to permit the author to reuse parts of the published article in a derivative or new work, including on Wikipedia.
The APS has an online publication entitled Physics, aiming to help physicists and physics students to learn about new developments outside of their own subfield. This now includes the general-interest articles that appeared as Physical Review Focus. It also publishes Physical Review X, an online-only open access journal. It is a peer-reviewed journal that publishes, as timely as possible, original research papers from all areas of pure, applied, and interdisciplinary physics. In 2014 Physical Review Applied began publishing research across all aspects of experimental and theoretical applications of physics, including their interactions with other sciences, engineering, and industry. In 2016 the APS launched Physical Review Fluids "to include additional areas of fluid dynamics research", and in 2017 it launched Physical Review Materials "to fill a gap" in the coverage of materials research.
|Journal||ISO 4 abbreviation||Editor(s)||Impact factor (2016)||Published||Scope||ISSN||Website|
|Physical Review, Series I||Phys. Rev.||1893–1912||All of Physics||All volumes|
|Physical Review, Series II[nb 2]||Phys. Rev.||1913–1969||All of Physics||Archive of All volumes|
|Physical Review Letters||Phys. Rev. Lett.||Hugues Chate
Reinhardt B. Schuhmann
|8.462||1958–present||Important fundamental research in all fields of physics||ISSN 0031-9007 (print)
ISSN 1079-7114 (web)
|Physical Review A[nb 2]||Phys. Rev. A||Gordon W. F. Drake
|2.925||1970–present||Atomic, molecular, and optical physics and quantum information||ISSN 1050-2947 (print)
ISSN 1094-1622 (web)
|Physical Review B[nb 2]||Phys. Rev. B||Laurens W. Molenkamp
Anthony M. Begley
|3.836||1970–present||Condensed matter and materials physics||ISSN 1098-0121 (print)
ISSN 1550-235X (web)
|Physical Review C||Phys. Rev. C||Benjamin F. Gibson
|3.820||1970–present||Nuclear physics||ISSN 0556-2813 (print)
ISSN 1089-490X (web)
|Physical Review D||Phys. Rev. D||Erick J. Weinberg
|4.506||1970–present||Particles, fields, gravitation, and cosmology||ISSN 1550-7998 (print)
ISSN 1550-2368 (web)
|Physical Review E||Phys. Rev. E||Eli Ben-Naim
Dirk Jan Bukman
|2.366||1993–present||Statistical, nonlinear, biological and soft matter physics||ISSN 1539-3755 (print)
ISSN 1550-2376 (web)
|Physical Review X||Phys. Rev. X||Cristina Marchetti
|12.789||2011–present||"Broad subject coverage encouraging communication across related fields"||ISSN 2160-3308 (web)||All volumes|
|Physical Review Accelerators and Beams||Phys. Rev. Accel. Beams||Frank Zimmermann||1.444||1998–present||Particle accelerators and beams||ISSN 2469-9888 (web)||All volumes|
|Physical Review Physics Education Research||Phys. Rev. Phys. Ed. Res.||Charles Henderson||2.083||2005–present||Physics education research||ISSN 2469-9896 (web)||All volumes|
|Physics||Physics||Jessica Thomas||2008–present||All of Physics||ISSN 1943-2879 (web)||All volumes|
|Physical Review Applied||Phys. Rev. Appl.||Stephan Forrest
|4.808||2014–present||"All aspects of experimental and theoretical applications of physics"||ISSN 2331-7019 (web)||All volumes|
|Physical Review Fluids||Phys. Rev. Fluids||John Kim
L. Gary Leal
|2.021||2016–present||"Innovative research that will significantly advance the fundamental understanding of fluid dynamics"||ISSN 2469-990X (web)||All volumes|
|Physical Review Materials||Phys. Rev. Mater.||Chris Leighton||2017–present||"high-quality original research in materials"||ISSN 2475-9953 (web)||All volumes|
The American Physical Society (APS) is the world's second largest organization of physicists. The Society publishes more than a dozen scientific journals, including the prestigious Physical Review and Physical Review Letters, and organizes more than twenty science meetings each year. APS is a member society of the American Institute of Physics.Bibcode
The bibcode (also known as the refcode) is a compact identifier used by several astronomical data systems to uniquely specify literature references.Black hole
A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it. The theory of general relativity predicts that a sufficiently compact mass can deform spacetime to form a black hole. The boundary of the region from which no escape is possible is called the event horizon. Although the event horizon has an enormous effect on the fate and circumstances of an object crossing it, no locally detectable features appear to be observed. In many ways, a black hole acts like an ideal black body, as it reflects no light. Moreover, quantum field theory in curved spacetime predicts that event horizons emit Hawking radiation, with the same spectrum as a black body of a temperature inversely proportional to its mass. This temperature is on the order of billionths of a kelvin for black holes of stellar mass, making it essentially impossible to observe.
Objects whose gravitational fields are too strong for light to escape were first considered in the 18th century by John Michell and Pierre-Simon Laplace. The first modern solution of general relativity that would characterize a black hole was found by Karl Schwarzschild in 1916, although its interpretation as a region of space from which nothing can escape was first published by David Finkelstein in 1958. Black holes were long considered a mathematical curiosity; it was during the 1960s that theoretical work showed they were a generic prediction of general relativity. The discovery of neutron stars by Jocelyn Bell Burnell in 1967 sparked interest in gravitationally collapsed compact objects as a possible astrophysical reality.
Black holes of stellar mass are expected to form when very massive stars collapse at the end of their life cycle. After a black hole has formed, it can continue to grow by absorbing mass from its surroundings. By absorbing other stars and merging with other black holes, supermassive black holes of millions of solar masses (M☉) may form. There is general consensus that supermassive black holes exist in the centers of most galaxies.
Despite its invisible interior, the presence of a black hole can be inferred through its interaction with other matter and with electromagnetic radiation such as visible light. Matter that falls onto a black hole can form an external accretion disk heated by friction, forming some of the brightest objects in the universe. If there are other stars orbiting a black hole, their orbits can be used to determine the black hole's mass and location. Such observations can be used to exclude possible alternatives such as neutron stars. In this way, astronomers have identified numerous stellar black hole candidates in binary systems, and established that the radio source known as Sagittarius A*, at the core of the Milky Way galaxy, contains a supermassive black hole of about 4.3 million solar masses.
On 11 February 2016, the LIGO collaboration announced the first direct detection of gravitational waves, which also represented the first observation of a black hole merger. As of December 2018, eleven gravitational wave events have been observed that originated from ten merging black holes (along with one binary neutron star merger). On 10 April 2019, the first ever direct image of a black hole and its vicinity was published, following observations made by the Event Horizon Telescope in 2017 of the supermassive black hole in Messier 87's galactic centre.Higgs boson
The Higgs boson is an elementary particle in the Standard Model of particle physics, produced by the quantum excitation of the Higgs field, one of the fields in particle physics theory. It is named after physicist Peter Higgs, who in 1964, along with five other scientists, proposed the mechanism which suggested the existence of such a particle. Its existence was confirmed in 2012 by the ATLAS and CMS collaborations based on collisions in the LHC at CERN.
On December 10, 2013, two of the physicists, Peter Higgs and François Englert, were awarded the Nobel Prize in Physics for their theoretical predictions. Although Higgs's name has come to be associated with this theory (the Higgs mechanism), several researchers between about 1960 and 1972 independently developed different parts of it.
In mainstream media the Higgs boson has often been called the "God particle", from a 1993 book on the topic, although the nickname is strongly disliked by many physicists, including Higgs himself, who regard it as sensationalism.Inflation (cosmology)
In physical cosmology, cosmic inflation, cosmological inflation, or just inflation, is a theory of exponential expansion of space in the early universe. The inflationary epoch lasted from 10−36 seconds after the conjectured Big Bang singularity to some time between 10−33 and 10−32 seconds after the singularity. Following the inflationary period, the universe continues to expand, but at a less rapid rate.Inflation theory was first developed in 1979 by theoretical physicist Alan Guth at Cornell University. It was developed further in the early 1980s. It explains the origin of the large-scale structure of the cosmos. Quantum fluctuations in the microscopic inflationary region, magnified to cosmic size, become the seeds for the growth of structure in the Universe (see galaxy formation and evolution and structure formation). Many physicists also believe that inflation explains why the universe appears to be the same in all directions (isotropic), why the cosmic microwave background radiation is distributed evenly, why the universe is flat, and why no magnetic monopoles have been observed.
The detailed particle physics mechanism responsible for inflation is unknown. The basic inflationary paradigm is accepted by most physicists, as a number of inflation model predictions have been confirmed by observation; however, a substantial minority of scientists dissent from this position. The hypothetical field thought to be responsible for inflation is called the inflaton.In 2002, three of the original architects of the theory were recognized for their major contributions; physicists Alan Guth of M.I.T., Andrei Linde of Stanford, and Paul Steinhardt of Princeton shared the prestigious Dirac Prize "for development of the concept of inflation in cosmology". In 2012, Alan Guth and Andrei Linde were awarded the Breakthrough Prize in Fundamental Physics for their invention and development of inflationary cosmology.Ionization
Ionization or ionisation, is the process by which an atom or a molecule acquires a negative or positive charge by gaining or losing electrons, often in conjunction with other chemical changes. The resulting electrically charged atom or molecule is called an ion. Ionization can result from the loss of an electron after collisions with subatomic particles, collisions with other atoms, molecules and ions, or through the interaction with electromagnetic radiation. Heterolytic bond cleavage and heterolytic substitution reactions can result in the formation of ion pairs. Ionization can occur through radioactive decay by the internal conversion process, in which an excited nucleus transfers its energy to one of the inner-shell electrons causing it to be ejected.Majorana fermion
A Majorana fermion (), also referred to as a Majorana particle, is a fermion that is its own antiparticle. They were hypothesized by Ettore Majorana in 1937. The term is sometimes used in opposition to a Dirac fermion, which describes fermions that are not their own antiparticles.
With the exception of the neutrino, all of the Standard Model fermions are known to behave as Dirac fermions at low energy (after electroweak symmetry breaking), and none are Majorana fermions. The nature of the neutrinos is not settled – they may be either Dirac or Majorana fermions.
In condensed matter physics, bound Majorana fermions can appear as quasiparticle excitations – the collective movement of several individual particles, not a single one, and they are governed by non-abelian statistics.Physical Review A
Physical Review A (also known as PRA) is a monthly peer-reviewed scientific journal published by the American Physical Society covering atomic, molecular, and optical physics and quantum information. The current Editor is Gordon W. F. Drake (University of Windsor).Physical Review B
Physical Review B: Condensed Matter and Materials Physics (also known as PRB) is a peer-reviewed, scientific journal, published by the American Physical Society (APS). The Editor of PRB is Laurens W. Molenkamp. It is part of the Physical Review family of journals. The current Editor in Chief is Michael Thoennessen. PRB currently publishes over 4500 papers a year, making it one of the largest physics journals in the world. According to the Journal Citation Reports, PRB's most recent impact factors have been 3.736 for 2014, 3.718 for 2015 and 3.836 for 2016.Physical Review E
Physical Review E is a peer-reviewed, scientific journal, published monthly by the American Physical Society. The main field of interest is many-body phenomena. It is currently edited by Eli Ben-Naim of the Los Alamos National Laboratory. While original research content requires subscription, editorials, news, and other non-research content is openly accessible.Physical Review Letters
Physical Review Letters (PRL), established in 1958, is a peer-reviewed, scientific journal that is published 52 times per year by the American Physical Society. As also confirmed by various measurement standards, which include the Journal Citation Reports impact factor and the journal h-index proposed by Google Scholar, many physicists and other scientists consider Physical Review Letters to be one of the most prestigious journals in the field of physics.PRL is published as a print journal, and is in electronic format, online and CD-ROM. Its focus is rapid dissemination of significant, or notable, results of fundamental research on all topics related to all fields of physics. This is accomplished by rapid publication of short reports, called "Letters". Papers are published and available electronically one article at a time. When published in such a manner, the paper is available to be cited by other work. The Lead Editor is Hugues Chaté. The Managing Editor is Reinhardt B. Schuhmann.Positron
The positron or antielectron is the antiparticle or the antimatter counterpart of the electron. The positron has an electric charge of +1 e, a spin of 1/2 (same as electron), and has the same mass as an electron. When a positron collides with an electron, annihilation occurs. If this collision occurs at low energies, it results in the production of two or more gamma ray photons.
Positrons can be created by positron emission radioactive decay (through weak interactions), or by pair production from a sufficiently energetic photon which is interacting with an atom in a material.Quantum cryptography
Quantum cryptography is the science of exploiting quantum mechanical properties to perform cryptographic tasks. The best known example of quantum cryptography is quantum key distribution which offers an information-theoretically secure solution to the key exchange problem. The advantage of quantum cryptography lies in the fact that it allows the completion of various cryptographic tasks that are proven or conjectured to be impossible using only classical (i.e. non-quantum) communication. For example, it is impossible to copy data encoded in a quantum state. If one attempts to read the encoded data, the quantum state will be changed (no-cloning theorem). This could be used to detect eavesdropping in quantum key distribution.Quantum machine learning
Quantum machine learning is an emerging interdisciplinary research area at the intersection of quantum physics and machine learning. The most common use of the term refers to machine learning algorithms for the analysis of classical data executed on a quantum computer. While machine learning algorithms are used to compute immense quantities of data, quantum machine learning increases such capabilities intelligently, by creating opportunities to conduct analysis on quantum states and systems. This includes hybrid methods that involve both classical and quantum processing, where computationally difficult subroutines are outsourced to a quantum device. These routines can be more complex in nature and executed faster with the assistance of quantum devices. Furthermore, quantum algorithms can be used to analyze quantum states instead of classical data. Beyond quantum computing, the term "quantum machine learning" is often associated with machine learning methods applied to data generated from quantum experiments, such as learning quantum phase transitions or creating new quantum experiments. Quantum machine learning also extends to a branch of research that explores methodological and structural similarities between certain physical systems and learning systems, in particular neural networks. For example, some mathematical and numerical techniques from quantum physics are applicable to classical deep learning and vice versa. Finally, researchers investigate more abstract notions of learning theory with respect to quantum information, sometimes referred to as "quantum learning theory".Quark
A quark () is a type of elementary particle and a fundamental constituent of matter. Quarks combine to form composite particles called hadrons, the most stable of which are protons and neutrons, the components of atomic nuclei. Due to a phenomenon known as color confinement, quarks are never directly observed or found in isolation; they can be found only within hadrons, which include baryons (such as protons and neutrons) and mesons. For this reason, much of what is known about quarks has been drawn from observations of hadrons.
Quarks have various intrinsic properties, including electric charge, mass, color charge, and spin. They are the only elementary particles in the Standard Model of particle physics to experience all four fundamental interactions, also known as fundamental forces (electromagnetism, gravitation, strong interaction, and weak interaction), as well as the only known particles whose electric charges are not integer multiples of the elementary charge.
There are six types, known as flavors, of quarks: up, down, strange, charm, bottom, and top. Up and down quarks have the lowest masses of all quarks. The heavier quarks rapidly change into up and down quarks through a process of particle decay: the transformation from a higher mass state to a lower mass state. Because of this, up and down quarks are generally stable and the most common in the universe, whereas strange, charm, bottom, and top quarks can only be produced in high energy collisions (such as those involving cosmic rays and in particle accelerators). For every quark flavor there is a corresponding type of antiparticle, known as an antiquark, that differs from the quark only in that some of its properties (such as the electric charge) have equal magnitude but opposite sign.
The quark model was independently proposed by physicists Murray Gell-Mann and George Zweig in 1964. Quarks were introduced as parts of an ordering scheme for hadrons, and there was little evidence for their physical existence until deep inelastic scattering experiments at the Stanford Linear Accelerator Center in 1968. Accelerator experiments have provided evidence for all six flavors. The top quark, first observed at Fermilab in 1995, was the last to be discovered.Strange quark
The strange quark or s quark (from its symbol, s) is the third lightest of all quarks, a type of elementary particle. Strange quarks are found in subatomic particles called hadrons. Example of hadrons containing strange quarks include kaons (K), strange D mesons (Ds), Sigma baryons (Σ), and other strange particles.
According to the IUPAP the symbol s is the official name, while strange is to be considered only as a mnemonic. The name sideways has also been used because the s quark has a I3 value of 0 while the u (“up”) and d (“down”) quarks have values of +1/2 and −1/2 respectively.Along with the charm quark, it is part of the second generation of matter, and has an electric charge of −1/3 e and a bare mass of 95+9−3 MeV/c2. Like all quarks, the strange quark is an elementary fermion with spin 1/2, and experiences all four fundamental interactions: gravitation, electromagnetism, weak interactions, and strong interactions. The antiparticle of the strange quark is the strange antiquark (sometimes called antistrange quark or simply antistrange), which differs from it only in that some of its properties have equal magnitude but opposite sign.
The first strange particle (a particle containing a strange quark) was discovered in 1947 (kaons), but the existence of the strange quark itself (and that of the up and down quarks) was only postulated in 1964 by Murray Gell-Mann and George Zweig to explain the Eightfold Way classification scheme of hadrons. The first evidence for the existence of quarks came in 1968, in deep inelastic scattering experiments at the Stanford Linear Accelerator Center. These experiments confirmed the existence of up and down quarks, and by extension, strange quarks, as they were required to explain the Eightfold Way.Tetraquark
A tetraquark, in particle physics, is an exotic meson composed of four valence quarks. A tetraquark state has long been suspected to be allowed by quantum chromodynamics, the modern theory of strong interactions. A tetraquark state is an example of an exotic hadron which lies outside the conventional quark model classification.Wormhole
A wormhole (or Einstein–Rosen bridge) is a speculative structure linking disparate points in spacetime, and is based on a special solution of the Einstein field equations solved using a Jacobian matrix and determinant. A wormhole can be visualized as a tunnel with two ends, each at separate points in spacetime (i.e., different locations or different points of time). More precisely it is a transcendental bijection of the spacetime continuum, an asymptotic projection of the Calabi–Yau manifold manifesting itself in Anti-de Sitter space.
Wormholes are consistent with the general theory of relativity, but whether wormholes actually exist remains to be seen.
A wormhole could connect extremely long distances such as a billion light years or more, short distances such as a few meters, different universes, or different points in time.W′ and Z′ bosons
In particle physics, W′ and Z′ bosons (or W-prime and Z-prime bosons) refer to hypothetical gauge bosons that arise from extensions of the electroweak symmetry of the Standard Model. They are named in analogy with the Standard Model W and Z bosons.