Example of Advances in High Energy Physics format
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Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format
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Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format Example of Advances in High Energy Physics format
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open access Open Access

Advances in High Energy Physics — Template for authors

Publisher: Hindawi
Categories Rank Trend in last 3 yrs
Nuclear and High Energy Physics #28 of 75 down down by 7 ranks
journal-quality-icon Journal quality:
Good
calendar-icon Last 4 years overview: 484 Published Papers | 1467 Citations
indexed-in-icon Indexed in: Scopus
last-updated-icon Last updated: 09/07/2020
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Related Journals

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SJR: 0.779
SNIP: 0.693

Journal Performance & Insights

Impact Factor

CiteRatio

Determines the importance of a journal by taking a measure of frequency with which the average article in a journal has been cited in a particular year.

A measure of average citations received per peer-reviewed paper published in the journal.

1.422

27% from 2018

Impact factor for Advances in High Energy Physics from 2016 - 2019
Year Value
2019 1.422
2018 1.953
2017 2.05
2016 1.74
graph view Graph view
table view Table view

3.0

9% from 2019

CiteRatio for Advances in High Energy Physics from 2016 - 2020
Year Value
2020 3.0
2019 3.3
2018 3.2
2017 3.3
2016 3.4
graph view Graph view
table view Table view

insights Insights

  • Impact factor of this journal has decreased by 27% in last year.
  • This journal’s impact factor is in the top 10 percentile category.

insights Insights

  • CiteRatio of this journal has decreased by 9% in last years.
  • This journal’s CiteRatio is in the top 10 percentile category.

SCImago Journal Rank (SJR)

Source Normalized Impact per Paper (SNIP)

Measures weighted citations received by the journal. Citation weighting depends on the categories and prestige of the citing journal.

Measures actual citations received relative to citations expected for the journal's category.

0.59

3% from 2019

SJR for Advances in High Energy Physics from 2016 - 2020
Year Value
2020 0.59
2019 0.572
2018 0.699
2017 0.866
2016 0.967
graph view Graph view
table view Table view

0.542

6% from 2019

SNIP for Advances in High Energy Physics from 2016 - 2020
Year Value
2020 0.542
2019 0.576
2018 0.698
2017 0.808
2016 0.831
graph view Graph view
table view Table view

insights Insights

  • SJR of this journal has increased by 3% in last years.
  • This journal’s SJR is in the top 10 percentile category.

insights Insights

  • SNIP of this journal has decreased by 6% in last years.
  • This journal’s SNIP is in the top 10 percentile category.

Advances in High Energy Physics

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Hindawi

Advances in High Energy Physics

Advances in High Energy Physics is a peer-reviewed, open access journal that publishes original research articles as well as review articles in all fields of high energy physics. The journal is dedicated to both theoretical and experimental research.... Read More

Nuclear and High Energy Physics

Physics and Astronomy

i
Last updated on
09 Jul 2020
i
ISSN
1687-7357
i
Impact Factor
Medium - 0.756
i
Acceptance Rate
43%
i
Frequency
Not provided
i
Open Access
Yes
i
Sherpa RoMEO Archiving Policy
Green faq
i
Plagiarism Check
Available via Turnitin
i
Endnote Style
Download Available
i
Bibliography Name
unsrt
i
Citation Type
Numbered
[25]
i
Bibliography Example
C. W. J. Beenakker. “Specular andreev reflection in graphene”. Phys. Rev. Lett., vol. 97, no. 6, 067007, 2006.

Top papers written in this journal

open accessOpen access Journal Article DOI: 10.1155/2010/723105
Holographic Duality with a View Toward Many-Body Physics
John McGreevy1

Abstract:

These are notes based on a series of lectures given at the KITP workshop Quantum Criticality and the AdS/CFT Correspondence in July, 2009. The goal of the lectures was to introduce condensed matter physicists to the AdS/CFT correspondence. Discussion of string theory and of supersymmetry is avoided to the extent possible. These are notes based on a series of lectures given at the KITP workshop Quantum Criticality and the AdS/CFT Correspondence in July, 2009. The goal of the lectures was to introduce condensed matter physicists to the AdS/CFT correspondence. Discussion of string theory and of supersymmetry is avoided to the extent possible. read more read less

Topics:

AdS/CFT correspondence (57%)57% related to the paper, String theory (55%)55% related to the paper
View PDF
635 Citations
open accessOpen access Journal Article DOI: 10.1155/2016/2162659
Neutrinoless Double Beta Decay: 2015 Review
S. Dell'Oro1, Simone Marcocci1, Matteo Viel2, Francesco Vissani1

Abstract:

The discovery of neutrino masses through the observation of oscillations boosted the importance of neutrinoless double beta decay (). In this paper, we review the main features of this process, underlining its key role from both the experimental and theoretical point of view. In particular, we contextualize the in the panoram... The discovery of neutrino masses through the observation of oscillations boosted the importance of neutrinoless double beta decay (). In this paper, we review the main features of this process, underlining its key role from both the experimental and theoretical point of view. In particular, we contextualize the in the panorama of lepton number violating processes, also assessing some possible particle physics mechanisms mediating the process. Since the existence is correlated with neutrino masses, we also review the state of the art of the theoretical understanding of neutrino masses. In the final part, the status of current experiments is presented and the prospects for the future hunt for are discussed. Also, experimental data coming from cosmological surveys are considered and their impact on expectations is examined. read more read less

Topics:

Neutrino oscillation (61%)61% related to the paper, Neutrino (60%)60% related to the paper, Double beta decay (56%)56% related to the paper, Lepton number (54%)54% related to the paper
View PDF
423 Citations
open accessOpen access Journal Article DOI: 10.1155/2013/490495
Particle production in strong electromagnetic fields in relativistic heavy-ion collisions
Kirill Tuchin1

Abstract:

I review the origin and properties of electromagnetic fields produced in heavy-ion collisions The field strength immediately after a collision is proportional to the collision energy and reaches ~ at RHIC and ~ at LHC I demonstrate by explicit analytical calculation that after dropping by about one-two orders of mag... I review the origin and properties of electromagnetic fields produced in heavy-ion collisions The field strength immediately after a collision is proportional to the collision energy and reaches ~ at RHIC and ~ at LHC I demonstrate by explicit analytical calculation that after dropping by about one-two orders of magnitude during the first fm/c of plasma expansion, it freezes out and lasts for as long as quark-gluon plasma lives as a consequence of finite electrical conductivity of the plasma Magnetic field breaks spherical symmetry in the direction perpendicular to the reaction plane, and therefore all kinetic coefficients are anisotropic I examine viscosity of QGP and show that magnetic field induces azimuthal anisotropy on plasma flow even in spherically symmetric geometry Very strong electromagnetic field has an important impact on particle production I discuss the problem of energy loss and polarization of fast fermions due to synchrotron radiation, consider photon decay induced by magnetic field, elucidate dissociation via Lorentz ionization mechanism, and examine electromagnetic radiation by plasma I conclude that all processes in QGP are affected by strong electromagnetic field and call for experimental investigation read more read less

Topics:

Electromagnetic field (61%)61% related to the paper, Field strength (60%)60% related to the paper, Optical field (59%)59% related to the paper, Electromagnetic radiation (58%)58% related to the paper, Photon (57%)57% related to the paper
View PDF
338 Citations
open accessOpen access Journal Article DOI: 10.1155/2016/6194250
Current Status and Future Prospects of the SNO+ Experiment
S. Andringa, E. Arushanova1, S. Asahi2, M. Askins3, D. J. Auty4, A. R. Back1, Z. Barnard5, N. Barros, E. W. Beier6, A. Bialek4, S. D. Biller7, E. Blucher8, R. Bonventre6, D. Braid5, E. Caden5, E. J. Callaghan6, J. Caravaca9, J. Caravaca10, João Carvalho11, L. Cavalli7, D. Chauhan5, D. Chauhan2, M. L. Chen2, O. Chkvorets5, Karl J. Clark2, B. T. Cleveland5, I. T. Coulter6, D. Cressy5, X. Dai2, C. Darrach5, B. Davis-Purcell12, Rehan Deen6, M. M. Depatie5, F.B. Descamps9, F.B. Descamps10, F. Di Lodovico1, N. Duhaime5, F. Duncan5, J. Dunger7, E. Falk13, N. Fatemighomi2, R. Ford5, P. Gorel4, C. Grant3, S. Grullon6, E. Guillian2, A. L. Hallin4, D. Hallman5, S. Hans14, J. Hartnell13, P. J. Harvey2, M. Hedayatipour4, W. J. Heintzelman6, R. L. Helmer12, B. Hreljac5, J. Hu4, T. Iida2, C. M. Jackson9, C. M. Jackson10, N. A. Jelley7, C. J. Jillings5, C. Jones7, P. G. Jones1, K. Kamdin10, K. Kamdin9, T. Kaptanoglu6, J. Kaspar15, Paul Keener6, P. Khaghani5, L. Kippenbrock15, J. R. Klein6, R. Knapik6, J. Kofron15, L. L. Kormos16, S. Korte5, C. Kraus5, C. B. Krauss4, K. Labe8, I. Lam2, C. Lan2, B. J. Land10, B. J. Land9, S. Langrock1, A. LaTorre8, I. Lawson5, G. Lefeuvre13, E. J. Leming13, J. Lidgard7, X. Liu2, Y. Liu2, V. Lozza17, S. Maguire14, A. Maio, K. Majumdar7, S. Manecki2, J. Maneira, E. Marzec6, A. Mastbaum6, N. McCauley18, A. B. McDonald2, J. E. McMillan19, P. Mekarski4, C. Miller2, Yuvraj Mohan6, E. Mony2, M. J. Mottram1, V. M. Novikov2, H. M. O'Keeffe2, E. O'Sullivan2, G. D. Orebi Gann6, M. J. Parnell16, S. J. M. Peeters13, T. Pershing3, Z. Petriw4, G. Prior, J. C. Prouty10, J. C. Prouty9, Sarah Quirk2, A. Reichold7, Andrew Robertson18, J. Rose18, Richard Rosero14, P. M. Rost5, J. Rumleskie5, M. A. Schumaker5, M. H. Schwendener5, D. Scislowski15, J. Secrest20, M. Seddighin2, L. Segui7, S. Seibert6, T. Shantz5, T. M. Shokair6, L. Sibley4, J. R. Sinclair13, K. Singh4, P. Skensved2, A. Sörensen17, T. Sonley2, R. Stainforth18, Matthew L Strait8, M. Stringer13, Robert Svoboda3, J. Tatar15, L. Tian2, N. Tolich15, J. Tseng7, H. W. C. Tseung15, R. Van Berg6, E. Vázquez-Jáuregui, C. J. Virtue5, B. von Krosigk17, J. M.G. Walker18, Mark Walker2, O. Wasalski12, J. Waterfield13, Randall White13, J. R. Wilson1, T. J. Winchester15, A. Wright2, Minfang Yeh14, T. Zhao2, Kai Zuber17

Abstract:

SNO+is a large liquid scintillator-based experiment located 2 km underground at SNOLAB, Sudbury,Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, ... SNO+is a large liquid scintillator-based experiment located 2 km underground at SNOLAB, Sudbury,Canada. It reuses the Sudbury Neutrino Observatory detector, consisting of a 12m diameter acrylic vessel which will be filled with about 780 tonnes of ultra-pure liquid scintillator. Designed as a multipurpose neutrino experiment, the primary goal of SNO+ is a search for the neutrinoless double-beta decay (0BB) of 130Te. In Phase I, the detector will be loaded with 0.3% natural tellurium, corresponding to nearly 800 kg of 130Te, with an expected effective Majorana neutrino mass sensitivity in the region of 55–133meV, just above the inverted mass hierarchy. Recently, the possibility of deploying up to ten times more natural tellurium has been investigated, which would enable SNO+ to achieve sensitivity deep into the parameter space for the inverted neutrino mass hierarchy in the future. Additionally, SNO+ aims to measure reactor antineutrino oscillations, low energy solar neutrinos, and geoneutrinos, to be sensitive to supernova neutrinos, and to search for exotic physics. A first phase with the detector filled with water will begin soon, with the scintillator phase expected to start after a few months of water data taking. The 01BB Phase I is foreseen for 2017. read more read less

Topics:

Sudbury Neutrino Observatory (65%)65% related to the paper, Neutrino detector (63%)63% related to the paper, Solar neutrino problem (61%)61% related to the paper, Solar neutrino (61%)61% related to the paper, Neutrino (59%)59% related to the paper
View PDF
302 Citations
open accessOpen access Journal Article DOI: 10.1155/2013/293986
Current Direct Neutrino Mass Experiments
Guido Drexlin1, Volker Hannen2, Susanne Mertens1, Ch. Weinheimer2

Abstract:

In this contribution, we review the status and perspectives of direct neutrino mass experiments, which investigate the kinematics of <path id="x1D6FD" d="M558 587q0 -32 -14 -61t-40 -53.5t-48.5 -41t-54.5 -36.5q144 -51 144 -174q0 -55 -43.5 -108t-104.5 -87q-77 -42 -131 -42q-31 0 -54 20t-31 47l11 18q48 -29 108 -29q79 0 119.5... In this contribution, we review the status and perspectives of direct neutrino mass experiments, which investigate the kinematics of <path id="x1D6FD" d="M558 587q0 -32 -14 -61t-40 -53.5t-48.5 -41t-54.5 -36.5q144 -51 144 -174q0 -55 -43.5 -108t-104.5 -87q-77 -42 -131 -42q-31 0 -54 20t-31 47l11 18q48 -29 108 -29q79 0 119.5 43t40.5 109t-44.5 107.5t-119.5 50.5l22 47q34 1 65 21q96 61 96 157q0 42 -24 67.5 t-62 25.5q-24 0 -43.5 -9t-35 -29.5t-27 -44t-22.5 -63t-19.5 -75.5t-18.5 -91q-57 -294 -68 -380q-26 -190 -35 -200q-26 -31 -97 -37l-4 26q19 9 48 170l77 413q23 121 52.5 187.5t83.5 114.5q70 62 148 62q51 0 88.5 -34t37.5 -91z" /> -decays of specific isotopes ( 3H, 187Re, 163Ho) to derive model-independent information on the averaged electron (anti)neutrino mass. After discussing the kinematics of -decay and the determination of the neutrino mass, we give a brief overview of past neutrino mass measurements (SN1987a-ToF studies, Mainz and Troitsk experiments for 3H, cryobolometers for 187Re). We then describe the Karlsruhe Tritium Neutrino (KATRIN) experiment currently under construction at Karlsruhe Institute of Technology, which will use the MAC-E-Filter principle to push the sensitivity down to a value of 200 meV (90% C.L.). To do so, many technological challenges have to be solved related to source intensity and stability, as well as precision energy analysis and low background rate close to the kinematic endpoint of tritium -decay at 18.6 keV. We then review new approaches such as the MARE, ECHO, and Project8 experiments, which offer the promise to perform an independent measurement of the neutrino mass in the sub-eV region. Altogether, the novel methods developed in direct neutrino mass experiments will provide vital information on the absolute mass scale of neutrinos. read more read less

Topics:

Neutrino (58%)58% related to the paper, KATRIN (56%)56% related to the paper
View PDF
249 Citations
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Advances in High Energy Physics format uses unsrt citation style.

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Frequently asked questions

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Absolutely not! Our tool has been designed to help you focus on writing. You can write your entire paper as per the Advances in High Energy Physics guidelines and auto format it.

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Yes, the template is compliant with the Advances in High Energy Physics guidelines. Our experts at SciSpace ensure that. If there are any changes to the journal's guidelines, we'll change our algorithm accordingly.

3. Can I cite my article in multiple styles in Advances in High Energy Physics?

Of course! We support all the top citation styles, such as APA style, MLA style, Vancouver style, Harvard style, and Chicago style. For example, when you write your paper and hit autoformat, our system will automatically update your article as per the Advances in High Energy Physics citation style.

4. Can I use the Advances in High Energy Physics templates for free?

Sign up for our free trial, and you'll be able to use all our features for seven days. You'll see how helpful they are and how inexpensive they are compared to other options, Especially for Advances in High Energy Physics.

5. Can I use a manuscript in Advances in High Energy Physics that I have written in MS Word?

Yes. You can choose the right template, copy-paste the contents from the word document, and click on auto-format. Once you're done, you'll have a publish-ready paper Advances in High Energy Physics that you can download at the end.

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Of course! You can do this using our intuitive editor. It's very easy. If you need help, our support team is always ready to assist you.

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SciSpace's Advances in High Energy Physics is currently available as an online tool. We're developing a desktop version, too. You can request (or upvote) any features that you think would be helpful for you and other researchers in the "feature request" section of your account once you've signed up with us.

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12. Is Advances in High Energy Physics's impact factor high enough that I should try publishing my article there?

To be honest, the answer is no. The impact factor is one of the many elements that determine the quality of a journal. Few of these factors include review board, rejection rates, frequency of inclusion in indexes, and Eigenfactor. You need to assess all these factors before you make your final call.

13. What is Sherpa RoMEO Archiving Policy for Advances in High Energy Physics?

SHERPA/RoMEO Database

We extracted this data from Sherpa Romeo to help researchers understand the access level of this journal in accordance with the Sherpa Romeo Archiving Policy for Advances in High Energy Physics. The table below indicates the level of access a journal has as per Sherpa Romeo's archiving policy.

RoMEO Colour Archiving policy
Green Can archive pre-print and post-print or publisher's version/PDF
Blue Can archive post-print (ie final draft post-refereeing) or publisher's version/PDF
Yellow Can archive pre-print (ie pre-refereeing)
White Archiving not formally supported
FYI:
  1. Pre-prints as being the version of the paper before peer review and
  2. Post-prints as being the version of the paper after peer-review, with revisions having been made.

14. What are the most common citation types In Advances in High Energy Physics?

The 5 most common citation types in order of usage for Advances in High Energy Physics are:.

S. No. Citation Style Type
1. Author Year
2. Numbered
3. Numbered (Superscripted)
4. Author Year (Cited Pages)
5. Footnote

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Yes, SciSpace provides this functionality. After signing up, you would need to import your existing references from Word or Bib file to SciSpace. Then SciSpace would allow you to download your references in Advances in High Energy Physics Endnote style according to Elsevier guidelines.

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